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801.1173 | Niels Asger Mortensen | Niels Asger Mortensen | Comment on "Design of a broadband highly dispersive pure silica photonic
crystal fiber" by Subbaraman et al | Comment accepted for Applied Optics | Appl. Optics 47, 3328 (2008). | 10.1364/AO.47.003328 | null | physics.optics | null | In a recent paper, Subbaraman et al report a theoretical and numerical study
of highly dispersive pure silica photonic crystal fiber supporting
group-velocity dispersion exceeding -2*10^4 ps/nm/km. This comment argues that
the authors only consider one out of the two sides of the same coin, by not
taking the corresponding beating length into account.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 07:24:38 GMT"
}
] | 2008-06-13T00:00:00 | [
[
"Mortensen",
"Niels Asger",
""
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801.1174 | Sun ChengYi | C.Y. Sun, D.H. Zhang | The Half-Integer Charged Particles of the Orbifold Models | 11pages, no figures | null | null | null | hep-th astro-ph | null | In this paper, we consider half-integer charged particles predicted by models
of orbifold compactification of the $E_8\times E_8$ heterotic string theory. We
find that it is possible for half-integer charged particles to exist in our
universe, and the location of half-interger charged particles in a galaxy
should be in the centers of the galaxy. By qualitative analysis, we find
half-interger charged particles may be helpful in explaining the formation of
SMBH at the large redshift and solving the UHECR puzzle.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 07:43:57 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Sun",
"C. Y.",
""
],
[
"Zhang",
"D. H.",
""
]
] | [
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801.1175 | Andrew Sunderland | Andrew Sunderland, Alexey V. Veryaskin, Wayne McRae, Li Ju, David G.
Blair | Direct string magnetic gradiometer for space applications | 17 single column pages, 3 figures | null | null | null | physics.ins-det | null | Recently, a novel Direct String Magnetic Gradiometer (DSMG) has been
developed, where a vibrating wire, driven by an AC current, is used as a single
sensitive element. It is designed to directly measure the local off-diagonal
components of the magnetic gradient tensor, Bxz, Byz and Bxy, provided the
distance to an object creating magnetic anomalies is much larger than the
length of the string. This requirement is well satisfied in space, if the
sensor is deployed from a satellite platform orbiting near the planet under
surveillance. Current instruments operating at $1{kPa}$ pressure achieve
sensitivity of $1.8 \times 10^{-10}{T}/{m}$ in the band $0.0001{Hz}$ to
$0.1{Hz}$. In this paper we show that proposed modifications to the current
gradiometer design, specifically aimed at the deployment in space, could have a
magnetic gradient sensitivity better than $10^{-13}{T}/{m}/\sqrt{Hz}$ in the
frequency range of interest for specific missions both for fundamental research
and for such applications as geophysical exploration on Mars and other solar
system planets. Also, by combining a few single-axis magnetic gradiometer
modules, it is possible to deploy a full tensor magnetic gradiometer.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 07:51:49 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Sunderland",
"Andrew",
""
],
[
"Veryaskin",
"Alexey V.",
""
],
[
"McRae",
"Wayne",
""
],
[
"Ju",
"Li",
""
],
[
"Blair",
"David G.",
""
]
] | [
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] |
801.1176 | Smirnov#2 | H. Boos, M. Jimbo, T. Miwa, F. Smirnov, Y. Takeyama | Hidden Grassmann Structure in the XXZ Model II: Creation Operators | null | Commun.Math.Phys.286:875-932,2009 | 10.1007/s00220-008-0617-z | null | hep-th | null | In this article we unveil a new structure in the space of operators of the
XXZ chain. We consider the space of all quasi-local operators, which are
products of the disorder field with arbitrary local operators. In analogy with
CFT the disorder operator itself is considered as primary field. In our
previous paper, we have introduced the annhilation operators which mutually
anti-commute and kill the primary field. Here we construct the creation
counterpart and prove the canonical anti-commutation relations with the
annihilation operators. We show that the ground state averages of quasi-local
operators created by the creation operators from the primary field are given by
determinants.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 08:01:47 GMT"
},
{
"version": "v2",
"created": "Sun, 23 Mar 2008 10:55:10 GMT"
},
{
"version": "v3",
"created": "Wed, 7 May 2008 20:06:03 GMT"
}
] | 2009-02-19T00:00:00 | [
[
"Boos",
"H.",
""
],
[
"Jimbo",
"M.",
""
],
[
"Miwa",
"T.",
""
],
[
"Smirnov",
"F.",
""
],
[
"Takeyama",
"Y.",
""
]
] | [
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] |
801.1177 | Oliver Wienand | Michael Brickenstein, Alexander Dreyer, Gert-Martin Greuel, Markus
Wedler, Oliver Wienand | New developments in the theory of Groebner bases and applications to
formal verification | 44 pages, 8 figures, submitted to the Special Issue of the Journal of
Pure and Applied Algebra | null | null | null | math.AC | null | We present foundational work on standard bases over rings and on Boolean
Groebner bases in the framework of Boolean functions. The research was
motivated by our collaboration with electrical engineers and computer
scientists on problems arising from formal verification of digital circuits. In
fact, algebraic modelling of formal verification problems is developed on the
word-level as well as on the bit-level. The word-level model leads to Groebner
basis in the polynomial ring over Z/2n while the bit-level model leads to
Boolean Groebner bases. In addition to the theoretical foundations of both
approaches, the algorithms have been implemented. Using these implementations
we show that special data structures and the exploitation of symmetries make
Groebner bases competitive to state-of-the-art tools from formal verification
but having the advantage of being systematic and more flexible.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 08:13:45 GMT"
},
{
"version": "v2",
"created": "Mon, 4 Feb 2008 12:10:11 GMT"
}
] | 2008-02-04T00:00:00 | [
[
"Brickenstein",
"Michael",
""
],
[
"Dreyer",
"Alexander",
""
],
[
"Greuel",
"Gert-Martin",
""
],
[
"Wedler",
"Markus",
""
],
[
"Wienand",
"Oliver",
""
]
] | [
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] |
801.1178 | Can Ataca | C. Ataca, S. Cahangirov, E. Durgun, Y.-R. Jang, S. Ciraci | Light Transition Metal Monatomic Chains | 13 pages, 9 figures | null | null | null | cond-mat.mtrl-sci | null | In this paper we investigated structural, electronic and magnetic properties
of 3d (light) transition metal (TM) atomic chains using first-principles
pseudopotential plane wave calculations. Periodic linear, dimerized linear and
planar zigzag chain structures and their short segments consisting of finite
number of atoms have been considered. Like Cu, the periodic, linear chains of
Mn, Co and Ni correspond to a local shallow minimum. However, for most of the
infinite periodic chains, neither linear nor dimerized linear structures are
favored; to lower their energy the chains undergo a structural transformation
to form planar zigzag and dimerized zigzag geometry. Dimerization in both
infinite and finite chains are much stronger than the usual Peierls distortion
and appear to depend on the number of 3d-electrons. As a result of
dimerization, a significant energy lowering occurs which, in turn, influences
the stability and physical properties. Metallic linear chain of Vanadium
becomes half-metallic upon dimerization. Infinite linear chain of Scandium also
becomes half-metallic upon transformation to zigzag structure. An interplay
between the magnetic ground state and atomic as well as electronic structure of
the chain has been revealed. The end effects influence the geometry, energetics
and magnetic ground state of the finite chains. Structure optimization
performed using noncollinear approximation indicates significant differences
from the collinear approximation. Variation of the cohesive energy of infinite
and finite-size chains with respect to the number of 3d-electrons are found to
mimic the bulk behavior pointed out by Friedel. The spin-orbit coupling of
finite chains are found to be negligibly small.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 08:18:02 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Ataca",
"C.",
""
],
[
"Cahangirov",
"S.",
""
],
[
"Durgun",
"E.",
""
],
[
"Jang",
"Y. -R.",
""
],
[
"Ciraci",
"S.",
""
]
] | [
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] |
801.1179 | Bernard Jacquemin | Bernard Jacquemin (ISC, UMR 7044, GERIICO), Sabine Ploux (ISC) | Corpus sp{\'e}cialis{\'e} et ressource de sp{\'e}cialit{\'e} | 16 pages, in French | Appears in Fran\c{c}ois Maniez; Pascaline Dury; Nathalie Arlin;
Claire Rougemont. Corpus et dictionnaires de langues de sp{\'e}cialit{\'e},
Presses Universitaires de Granoble, pp.197-212, 2008 | null | null | cs.IR cs.CL | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | "Semantic Atlas" is a mathematic and statistic model to visualise word senses
according to relations between words. The model, that has been applied to
proximity relations from a corpus, has shown its ability to distinguish word
senses as the corpus' contributors comprehend them. We propose to use the model
and a specialised corpus in order to create automatically a specialised
dictionary relative to the corpus' domain. A morpho-syntactic analysis
performed on the corpus makes it possible to create the dictionary from
syntactic relations between lexical units. The semantic resource can be used to
navigate semantically - and not only lexically - through the corpus, to create
classical dictionaries or for diachronic studies of the language.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 08:21:26 GMT"
},
{
"version": "v2",
"created": "Fri, 19 Jun 2015 12:22:39 GMT"
}
] | 2015-06-22T00:00:00 | [
[
"Jacquemin",
"Bernard",
"",
"ISC, UMR 7044, GERIICO"
],
[
"Ploux",
"Sabine",
"",
"ISC"
]
] | [
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801.118 | Yves Revaz | Y. Revaz, D. Pfenniger, F. Combes, F. Bournaud | Simulations of galactic disks including a dark baryonic component | 4 pages, 2 figures. To appear in the proceedings of "Formation and
Evolution of Galaxy Disks", ed. J. Funes & E. Corsini. Higher resolution
version may be downloaded at
https://obswww.unige.ch/~revaz/public/Rome2007/revaz.pdf | null | 10.1051/0004-6361/200809883 | null | astro-ph | null | $\Lambda$CDM numerical simulations predict that the "missing baryons" reside
in a Warm-Hot gas phase in the over-dense cosmic filaments. However, there are
now several theoretical and observational arguments that support the fact that
galactic disks may be more massive than usually thought, containing a
substantial fraction of the "missing baryons". Hereafter, we present new N-body
simulations of galactic disks, where the gas content has been multiplied by a
factor 5. The stability of the disk is ensured by assuming that the ISM is
composed out of two partially coupled phases, a warm phase, corresponding the
observed CO and HI gas and a cold collisionless phase corresponding to the
unseen baryons.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 08:30:12 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Revaz",
"Y.",
""
],
[
"Pfenniger",
"D.",
""
],
[
"Combes",
"F.",
""
],
[
"Bournaud",
"F.",
""
]
] | [
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0.0233541969,
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] |
801.1181 | David Martin de Diego | M. de Leon, J.C. Marrero, D. Martin de Diego | A Geometric Hamilton-Jacobi Theory for Classical Field Theories | 11 pages | null | null | null | math-ph math.MP | null | In this paper we extend the geometric formalism of the Hamilton-Jacobi theory
for hamiltonian mechanics to the case of classical field theories in the
framework of multisymplectic geometry and Ehresmann connections.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 08:30:16 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"de Leon",
"M.",
""
],
[
"Marrero",
"J. C.",
""
],
[
"de Diego",
"D. Martin",
""
]
] | [
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] |
801.1182 | Yury Zinoviev | Yury M. Zinoviev | Relativistic Quantum Coulomb Law | 22 pages | null | null | null | hep-th | null | The relativistic quantum mechanics equations for the electromagnetic
interaction are propososed.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 08:31:12 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Zinoviev",
"Yury M.",
""
]
] | [
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] |
801.1183 | Mahdou Najib | D. Bennis | Rings over which the class of Gorenstein flat modules is closed under
extensions | null | null | null | null | math.AC | null | A ring $R$ is called left GF-closed, if the class of all Gorenstein flat left
$R$-modules is closed under extensions. The class of left GF-closed rings
includes strictly the one of right coherent rings and the one of rings of
finite weak dimension.
In this paper, we investigate the Gorenstein flat dimension over left
GF-closed rings. Namely, we generalize the fact that the class of all
Gorenstein flat left modules is projectively resolving over right coherent
rings to left GF-closed rings. Also, we generalize the characterization of
Gorenstein flat left modules (then of Gorenstein flat dimension of left
modules) over right coherent rings to left GF-closed rings. Finally, using
direct products of rings, we show how to construct a left GF-closed ring that
is neither right coherent nor of finite weak dimension.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 08:36:24 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Bennis",
"D.",
""
]
] | [
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801.1184 | Andrea Cimatti | A. Cimatti (Universita` di Bologna - Dipartimento di Astronomia), P.
Cassata (LAM), L. Pozzetti (INAF - OABO), J. Kurk (MPIA Heidelberg), M.
Mignoli (INAF - OABO), A. Renzini (INAF - OAPD), E. Daddi (CEA Saclay), M.
Bolzonella (INAF - OABO), M. Brusa (MPE Garching), G. Rodighiero (Universita`
di Padova - Dipartimento di Astronomia), M. Dickinson (NOAO), A. Franceschini
(Universita` di Padova - Dipartimento di Astronomia), G. Zamorani (INAF -
OABO), S. Berta (MPE Garching), P. Rosati (ESO), C. Halliday (INAF - OAA) | GMASS Ultradeep Spectroscopy of Galaxies at 1.4<z<2. II. Superdense
passive galaxies: how did they form and evolve ? | 22 pages, 23 figures, Astronomy & Astrophysics, in press | Astron.Astrophys.482:21-42,2008 | 10.1051/0004-6361:20078739 | null | astro-ph | null | We combine ultradeep optical spectroscopy from the GMASS project ("Galaxy
Mass Assembly ultradeep Spectroscopic Survey") with GOODS multi-band photometry
and HST imaging to study a sample of passive galaxiesat 1.39<z<1.99 selected at
4.5 microns. A stacked spectrum with an equivalent integration time of ~500
hours was obtained is publicly released. The spectral and photometric SED
properties indicate very weak or absent star formation, moderately old stellar
ages of ~1 Gyr (for solar metallicity) and stellar masses in the range of
10^{10-11} solar masses, thus implying that the major star formation and
assembly processes for these galaxies occurred at z>2. These galaxies have
morphologies that are predominantly compact and spheroidal.However, their sizes
(R_e <~ 1 kpc) are much smaller than those of spheroids in the present--day
Universe. Their stellar mass surface densities are consequently higher by ~1
dex if compared to spheroids at z~0 with the same mass. Their rest-frame B-band
surface brightness scales with the effective radius, but the offset with
respect to the surface brightness of the local Kormendy relation is too large
to be explained by simple passive evolution. At z~1, a larger fraction of
passive galaxies follows the z~0 size -- mass relation. Superdense relics with
R_e~1 kpc are extremely rare at z~0 with respect to z>1, and absent if R_e<1
kpc. Because of the similar sizes and mass densities, we suggest that the
superdense passive galaxies at 1<z<2 are the remnants of the powerful
starbursts occurring in submillimeter--selected galaxies at z>2. The results
are compared with theoretical models and the main implications discussed in the
framework of massive galaxy formation and evolution.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 08:37:07 GMT"
}
] | 2011-05-05T00:00:00 | [
[
"Cimatti",
"A.",
"",
"Universita` di Bologna - Dipartimento di Astronomia"
],
[
"Cassata",
"P.",
"",
"LAM"
],
[
"Pozzetti",
"L.",
"",
"INAF - OABO"
],
[
"Kurk",
"J.",
"",
"MPIA Heidelberg"
],
[
"Mignoli",
"M.",
"",
"INAF - OABO"
],
[
"Renzini",
"A.",
"",
"INAF - OAPD"
],
[
"Daddi",
"E.",
"",
"CEA Saclay"
],
[
"Bolzonella",
"M.",
"",
"INAF - OABO"
],
[
"Brusa",
"M.",
"",
"MPE Garching"
],
[
"Rodighiero",
"G.",
"",
"Universita`\n di Padova - Dipartimento di Astronomia"
],
[
"Dickinson",
"M.",
"",
"NOAO"
],
[
"Franceschini",
"A.",
"",
"Universita` di Padova - Dipartimento di Astronomia"
],
[
"Zamorani",
"G.",
"",
"INAF -\n OABO"
],
[
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"S.",
"",
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],
[
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"P.",
"",
"ESO"
],
[
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"C.",
"",
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]
] | [
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801.1185 | Jaspreet Singh | Jaspreet Singh, Onkar Dabeer and Upamanyu Madhow | Capacity of the Discrete-Time AWGN Channel Under Output Quantization | To appear at ISIT 2008. (Some changes in the content (in Section IV)
compared to the first version uploaded on Jan 08, 2008.) | null | null | null | cs.IT math.IT | null | We investigate the limits of communication over the discrete-time Additive
White Gaussian Noise (AWGN) channel, when the channel output is quantized using
a small number of bits. We first provide a proof of our recent conjecture on
the optimality of a discrete input distribution in this scenario. Specifically,
we show that for any given output quantizer choice with K quantization bins
(i.e., a precision of log2 K bits), the input distribution, under an average
power constraint, need not have any more than K + 1 mass points to achieve the
channel capacity. The cutting-plane algorithm is employed to compute this
capacity and to generate optimum input distributions. Numerical optimization
over the choice of the quantizer is then performed (for 2-bit and 3-bit
symmetric quantization), and the results we obtain show that the loss due to
low-precision output quantization, which is small at low signal-to-noise ratio
(SNR) as expected, can be quite acceptable even for moderate to high SNR
values. For example, at SNRs up to 20 dB, 2-3 bit quantization achieves 80-90%
of the capacity achievable using infinite-precision quantization.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 08:39:04 GMT"
},
{
"version": "v2",
"created": "Thu, 15 May 2008 20:54:16 GMT"
}
] | 2008-05-15T00:00:00 | [
[
"Singh",
"Jaspreet",
""
],
[
"Dabeer",
"Onkar",
""
],
[
"Madhow",
"Upamanyu",
""
]
] | [
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801.1186 | Troels Markussen | Troels Markussen, Riccardo Rurali, Antti-Pekka Jauho, Mads Brandbyge | Transport in Silicon Nanowires: Role of Radial Dopant Profile | Submitted to Journal of Computational Electronics, presented in
IWCE-12 | null | null | null | cond-mat.mes-hall cond-mat.mtrl-sci | null | We consider the electronic transport properties of phosphorus (P) doped
silicon nanowires (SiNWs). By combining ab initio density functional theory
(DFT) calculations with a recursive Green's function method, we calculate the
conductance distribution of up to 200 nm long SiNWs with different
distributions of P dopant impurities. We find that the radial distribution of
the dopants influences the conductance properties significantly: Surface doped
wires have longer mean-free paths and smaller sample-to-sample fluctuations in
the cross-over from ballistic to diffusive transport. These findings can be
quantitatively predicted in terms of the scattering properties of the single
dopant atoms, implying that relatively simple calculations are sufficient in
practical device modeling
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 08:41:28 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Markussen",
"Troels",
""
],
[
"Rurali",
"Riccardo",
""
],
[
"Jauho",
"Antti-Pekka",
""
],
[
"Brandbyge",
"Mads",
""
]
] | [
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] |
801.1187 | Daniel Schaerer | Daniel Schaerer (ObsGE, OMP), Anne Verhamme (ObsGE) | 3D Lya radiation transfer. II. Fitting the Lyman break galaxy MS
1512-cB58 and implications for Lya emission in high-z starbursts | Accepted for publication in A&A | null | 10.1051/0004-6361:20078913 | null | astro-ph | null | Using our 3D Lya radiation transfer code, we compute the radiation transfer
of Lya and UV continuum photons including dust. Observational constraints on
the neutral gas (column density, kinematics, etc.) are taken from other
analysis of this object. RESULTS: The observed Lya profile of MS 1512--cB58 is
reproduced for the first time taking radiation transfer and all observational
constraints into account. The observed absorption profile is found to result
naturally from the observed amount of dust and the relatively high HI column
density. Radiation transfer effects and suppresion by dust transform a strong
intrinsic Lya emission with EW(Lya)>~ 60 Ang into the observed faint superposed
Lya emission peak. We propose that the vast majority of LBGs have intrinsically
EW(Lya)~60-80 Ang or larger, and that the main physical parameter responsible
for the observed variety of Lya strengths and profiles in LBGs is N_H and the
accompanying variation of the dust content. Observed EW(Lya) distributions, Lya
luminosity functions, and related quantities must therefore be corrected for
radiation transfer and dust effects. The implications from our scenario on the
duty-cycle of Lya emitters are also discussed.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 08:43:12 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Schaerer",
"Daniel",
"",
"ObsGE, OMP"
],
[
"Verhamme",
"Anne",
"",
"ObsGE"
]
] | [
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] |
801.1188 | Jean-Yves Veuillen | Fran\c{c}ois Varchon (NEEL), Pierre Mallet (NEEL), Laurence Magaud
(NEEL), Jean-Yves Veuillen (NEEL) | Few layers graphene on 6H-SiC(000-1): an STM study | 20 pages | Physical Review B 77 (2008) 165415 | 10.1103/PhysRevB.77.165415 | null | cond-mat.mtrl-sci | null | We have analyzed by Scanning Tunnelling Microscopy (STM) thin films made of
few (3-5) graphene layers grown on the C terminated face of 6H-SiC in order to
identify the nature of the azimuthal disorder reported in this material. We
observe superstructures which are interpreted as Moir\'e patterns due to a
misorientation angle between consecutive layers. The presence of stacking
faults is expected to lead to electronic properties reminiscent of single layer
graphene even for multilayer samples. Our results indicate that this apparent
electronic decoupling of the layers can show up in STM data.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 09:11:33 GMT"
}
] | 2008-04-23T00:00:00 | [
[
"Varchon",
"François",
"",
"NEEL"
],
[
"Mallet",
"Pierre",
"",
"NEEL"
],
[
"Magaud",
"Laurence",
"",
"NEEL"
],
[
"Veuillen",
"Jean-Yves",
"",
"NEEL"
]
] | [
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] |
801.1189 | E. Ahmed | Hala El-Saka, E. Ahmed, M. I. Shehata and A. M. A. -El-Sayed | On stability, persistence and Hopf bifurcation of fractional order
dynamical system | 6 pages | null | null | null | nlin.CG nlin.CD | null | This is a preliminary study for bifurcation in fractional order dynamical
systems. Stability, persistence and hopf bifurcation are studied. Some studies
are also done for functional equations.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 09:12:38 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"El-Saka",
"Hala",
""
],
[
"Ahmed",
"E.",
""
],
[
"Shehata",
"M. I.",
""
],
[
"-El-Sayed",
"A. M. A.",
""
]
] | [
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] |
801.119 | Yujin Yang | Yujin Yang (1), Ann Zabludoff (1), Dennis Zaritsky (1), Christopher
Mihos (2) ((1) Steward Observatory, University of Arizona, (2) Case Western
Reserve University) | The Detailed Evolution of E+A Galaxies into Early Types | A typo fixed in the abstract | Astrophys.J.688:945-971,2008; Erratum-ibid.702:1683,2009 | 10.1086/591656 10.1088/0004-637X/702/2/1683 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Post-starburst, or E+A galaxies, are the best candidates for galaxies in
transition from being gas-rich and star-forming to gas-poor and
passively-evolving via galaxy-galaxy mergers. To determine what E+A galaxies
become after their young stellar populations fade away, we present the detailed
morphologies of 21 E+As using HST images. We find that E+As are similar to
early types in that they have large bulge fractions (median B/T = 0.59), high
Sersic index (n > 4), and high concentration indices (C > 4.3). The large
fraction (70%) of E+As with positive color gradients (i.e., bluer nuclei)
indicates that the young stellar populations are more concentrated than the old
populations. We show that these positive color gradients can evolve into the
negative gradients typical in E/S0s if the central parts of these galaxies are
metal enhanced. E+A galaxies stand apart from the E/S0s in the edge-on
projection of the Fundamental Plane, implying that E+As have, on average, a M/L
that is ~3.8 times smaller than that of E/S0s. The tilt of the E+A FP indicates
that the variation among stellar populations in these galaxies is closely tied
to their structural parameters such that smaller or less massive galaxies have
smaller M/L. We find a population of unresolved compact sources in nine E+As
(45%). Their colors and luminosities are consistent with the hypothesis that
these are newly formed star clusters. The bright end of the cluster LF is
fainter in redder E+A's, suggesting that the young star cluster systems have
faded or been disrupted as the merger remnant aged. In summary, the
morphologies, color profiles, scaling relations, and cluster populations are
all consistent with the hypothesis that E+As galaxies are the results of
mergers that evolve into early-type galaxies.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 09:15:55 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Jul 2008 19:47:31 GMT"
},
{
"version": "v3",
"created": "Fri, 10 Jul 2009 18:31:36 GMT"
}
] | 2009-09-28T00:00:00 | [
[
"Yang",
"Yujin",
""
],
[
"Zabludoff",
"Ann",
""
],
[
"Zaritsky",
"Dennis",
""
],
[
"Mihos",
"Christopher",
""
]
] | [
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] |
801.1191 | J\"org Sichelschmidt | Cornelius Krellner, Tobias Foerster, Hirale Jeevan, Christoph Geibel,
Joerg Sichelschmidt | Relevance of ferromagnetic correlations for the Electron Spin Resonance
in Kondo lattice systems | 5 pages, 2 figures, 1 table | Phys. Rev. Lett. 100, 066401(2008) | 10.1103/PhysRevLett.100.066401 | null | cond-mat.str-el | null | Electron Spin Resonance (ESR) measurements of the ferromagnetic Kondo lattice
system CeRuPO show a well defined ESR signal which is related to the magnetic
properties of the Ce3+ moment. In contrast, no ESR signal could be observed in
the antiferromagnetic homologue CeOsPO. Additionally, we detect an ESR signal
in a further ferromagnetic Yb compound, YbRh, while it was absent in a number
of Ce or Yb intermetallic compounds with dominant antiferromagnetic exchange,
independently of the presence of a strong Kondo interaction or the proximity to
a (quantum) critical point. Thus, the observation of an ESR signal in a Kondo
lattice is neither specific to Yb nor to the proximity of a quantum critical
point, but seems to be connected to the presence of ferromagnetic fluctuations.
These conclusions not only provide a basic concept to understand the ESR in
Kondo lattice systems even well below the Kondo temperature as observed in the
heavy fermion metal YbRh2Si2 but point out ESR as a prime method to investigate
directly the spin dynamics of the Kondo ion.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 09:16:10 GMT"
}
] | 2008-04-18T00:00:00 | [
[
"Krellner",
"Cornelius",
""
],
[
"Foerster",
"Tobias",
""
],
[
"Jeevan",
"Hirale",
""
],
[
"Geibel",
"Christoph",
""
],
[
"Sichelschmidt",
"Joerg",
""
]
] | [
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] |
801.1192 | Tomas Jungwirth | B. G. Park, J. Wunderlich, D. A. Williams, S. J. Joo, K. Y. Jung, K.
H. Shin, K. Olejnik, A. B. Shick, and T. Jungwirth | Tunneling anisotropic magnetoresistance in multilayer-(Co/Pt)/AlOx/Pt
structures | 4 pages, 5 figures, to be published in Phys. Rev. Lett | null | 10.1103/PhysRevLett.100.087204 | null | cond-mat.mtrl-sci | null | We report observations of tunneling anisotropic magnetoresitance (TAMR) in
vertical tunnel devices with a ferromagnetic multilayer-(Co/Pt) electrode and a
non-magnetic Pt counter-electrode separated by an AlOx barrier. In stacks with
the ferromagnetic electrode terminated by a Co film the TAMR magnitude
saturates at 0.15% beyond which it shows only weak dependence on the magnetic
field strength, bias voltage, and temperature. For ferromagnetic electrodes
terminated by two monolayers of Pt we observe order(s) of magnitude enhancement
of the TAMR and a strong dependence on field, temperature and bias. Discussion
of experiments is based on relativistic ab initio calculations of magnetization
orientation dependent densities of states of Co and Co/Pt model systems.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 09:17:42 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Park",
"B. G.",
""
],
[
"Wunderlich",
"J.",
""
],
[
"Williams",
"D. A.",
""
],
[
"Joo",
"S. J.",
""
],
[
"Jung",
"K. Y.",
""
],
[
"Shin",
"K. H.",
""
],
[
"Olejnik",
"K.",
""
],
[
"Shick",
"A. B.",
""
],
[
"Jungwirth",
"T.",
""
]
] | [
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] |
801.1193 | Claire Halliday | C. Halliday, E. Daddi, A. Cimatti, J. Kurk, A. Renzini, M. Mignoli, M.
Bolzonella, L. Pozzetti, M. Dickinson, G. Zamorani, S. Berta, A.
Franceschini, P. Cassata, G. Rodighiero and P. Rosati | GMASS Ultradeep Spectroscopy of Galaxies at redshift z~2. I. The stellar
metallicity | Accepted for publication in Astronomy and Astrophysics on 18 December
2007, 9 pages, 8 figures, aa.bst and aa.cls A&A style files | null | 10.1051/0004-6361:20078673 | null | astro-ph | null | Context: Galaxy metallicities have been measured to redshift z~2 by gas-phase
oxygen abundances of the interstellar medium using the R23 and N2 methods.
Galaxy stellar metallicities provide crucial data for chemical evolution models
but have not been assessed reliably much outside the local Universe. Aims: We
determine the iron-abundance, stellar metallicity of star-forming galaxies
(SFGs) at redshift z~2, observed as part of the Galaxy Mass Assembly ultra-deep
Spectroscopic Survey (GMASS). Methods: We compute the equivalent width of a
rest-frame mid-ultraviolet, photospheric absorption-line index, the 1978 index
found to vary monotonically with stellar metallicity by Rix and collaborators.
We normalise and combine 75 SFG spectra from the GMASS survey to produce a
spectrum corresponding to a total integration time 1652.5 hours (and a
signal-to-noise ratio ~100 for our 1.5 angstrom binning) of FORS2 spectroscopic
observations at the Very Large Telescope. Results: We measure an
iron-abundance, stellar metallicity of log (Z/Zsolar) = -0.574+/-0.159 for our
spectrum representative of a galaxy of stellar mass 9.4 x 10^9 Msolar assuming
a Chabrier IMF. We find that the R04 model SFG spectrum for log (Z/Zsolar) =
-0.699 solar metallicity provides the best description of our GMASS coadded
spectrum. For similar galaxy stellar mass, our stellar metallicity is ~0.25 dex
lower than the oxygen-abundance, gas-phase metallicity quantified by Erb and
collaborators for UV-selected star-forming galaxies at z=2. Conclusions: We
conclude that we are witnessing the establishment of a light-element
overabundance in galaxies as they are being formed at redshift z~2. Our
measurements are reminiscent of the alpha-element enhancement seen in
low-redshift, galactic bulges and early-type galaxies. (Abridged)
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 09:22:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Halliday",
"C.",
""
],
[
"Daddi",
"E.",
""
],
[
"Cimatti",
"A.",
""
],
[
"Kurk",
"J.",
""
],
[
"Renzini",
"A.",
""
],
[
"Mignoli",
"M.",
""
],
[
"Bolzonella",
"M.",
""
],
[
"Pozzetti",
"L.",
""
],
[
"Dickinson",
"M.",
""
],
[
"Zamorani",
"G.",
""
],
[
"Berta",
"S.",
""
],
[
"Franceschini",
"A.",
""
],
[
"Cassata",
"P.",
""
],
[
"Rodighiero",
"G.",
""
],
[
"Rosati",
"P.",
""
]
] | [
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] |
801.1194 | Zengxiu Zhao | Huayu Hu and Jianmin Yuan | Non-perturbative QED Model with Dressed States to Tackle HHG in
Ultrashort Intense Laser Pulses | 4 pages, 2 figures | null | 10.1103/PhysRevA.78.063826 | null | physics.atom-ph | null | A generalization of non-perturbative QED model for high harmonic generation
is developed for the multi-mode optical field case. By introducing
classical-field-dressed quantized Volkov states analytically, a formula to
calculate HHG for hydrogen-like atom in ultrashort intense laser pulse is
obtained, which has a simple intuitive interpretation. The dressed state QED
model indicates a new perspective to understand HHG, for example, the presence
of the weak even-order harmonic photons, which has been verified by both
theoretical analysis and numerical computation. Long wavelength approximation
and strong field approximation are involved in the development of the
formalism.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 09:30:52 GMT"
}
] | 2013-05-29T00:00:00 | [
[
"Hu",
"Huayu",
""
],
[
"Yuan",
"Jianmin",
""
]
] | [
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] |
801.1195 | Thomas Ward | Thomas Ward and Yuki Yayama | Markov partitions reflecting the geometry of x2,x3 | 6 eps figures | Discrete and Continuous Dynamical Systems 24, No. 2, 613-624
(2009) | 10.3934/dcds.2009.24.613 | null | math.DS | null | We give an explicit geometric description of the $\times2,\times3$ system,
and use his to study a uniform family of Markov partitions related to those of
Wilson and Abramov. The behaviour of these partitions is stable across
expansive cones and transitions in this behaviour detects the non-expansive
lines.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 09:33:08 GMT"
}
] | 2009-09-22T00:00:00 | [
[
"Ward",
"Thomas",
""
],
[
"Yayama",
"Yuki",
""
]
] | [
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801.1196 | Gert De Cooman | Gert de Cooman, Filip Hermans | Imprecise probability trees: Bridging two theories of imprecise
probability | 30 pages, 8 figures | null | null | null | math.PR math.ST stat.ML stat.TH | null | We give an overview of two approaches to probability theory where lower and
upper probabilities, rather than probabilities, are used: Walley's behavioural
theory of imprecise probabilities, and Shafer and Vovk's game-theoretic account
of probability. We show that the two theories are more closely related than
would be suspected at first sight, and we establish a correspondence between
them that (i) has an interesting interpretation, and (ii) allows us to freely
import results from one theory into the other. Our approach leads to an account
of probability trees and random processes in the framework of Walley's theory.
We indicate how our results can be used to reduce the computational complexity
of dealing with imprecision in probability trees, and we prove an interesting
and quite general version of the weak law of large numbers.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 09:46:44 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"de Cooman",
"Gert",
""
],
[
"Hermans",
"Filip",
""
]
] | [
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] |
801.1197 | Juan Diego Urbina | Juan Diego Urbina and Klaus Richter | Random Wave Functions with boundary and normalization constraints:
Quantum statistical physics meets quantum chaos | Contribution to the Chladni meeting, Wittemberg 24-28 June 2006.
Slightly improved version of published paper | Eur. Phys. J. ST. 145 (2007) 255-269 | null | null | nlin.CD cond-mat.mes-hall math-ph math.MP quant-ph | null | We present an improved version of Berry's ansatz able to incorporate exactly
the existence of boundaries and the correct normalization of the eigenfunction
into an ensemble of random waves. We then reformulate the Random Wave
conjecture showing that in its new version it is a statement about the
universal nature of eigenfunction fluctuations in systems with chaotic
classical dynamics. The emergence of the universal results requires the use of
both semiclassical methods and a new expansion for a very old problem in
quantum statistical physics
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 09:52:22 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Urbina",
"Juan Diego",
""
],
[
"Richter",
"Klaus",
""
]
] | [
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] |
801.1198 | Fernando Atrio-Barandela | F. Atrio-Barandela, J.P. Muecket, R. Genova-Santos | Kinematic Sunyaev-Zeldovich Cosmic Microwave Background Temperature
Anisotropies Generated by Gas in Cosmic Structures | ApJ Lett, to be published | null | 10.1086/529139 | null | astro-ph | null | If the gas in filaments and halos shares the same velocity field than the
luminous matter, it will generate measurable temperature anisotropies due to
the Kinematic Sunyaev-Zeldovich effect. We compute the distribution function of
the KSZ signal produced by a typical filament and show it is highly
non-gaussian. The combined contribution of the Thermal and Kinematic SZ effects
of a filament of size $L\simeq 5$Mpc and electron density $n_e\simeq
10^3m^{-3}$ could explain the cold spots of $\delta\sim -200\mu$K on scales of
30' found in the Corona Borealis Supercluster by the VSA experiment. PLANCK,
with its large resolution and frequency coverage, could provide the first
evidence of the existence of filaments in this region. The KSZ contribution of
the network of filaments and halo structures to the radiation power spectrum
peaks around $l\sim 400$, a scale very different from that of clusters of
galaxies, with a maximum amplitude $l(l+1)C_l/2\pi\sim 10-25 (\mu K)^2$,
depending on model parameters, i.e., $\sigma_8$ and the Jeans length. About 80%
of the signal comes from filaments with redshift $z\le 0.1$. Adding this
component to the intrinsic Cosmic Microwave Background temperature anisotropies
of the concordance model improves the fit to WMAP 3yr data by
$\Delta\chi^2\simeq 1$. The improvement is not statistically significant but a
more systematic study could demonstrate that gas could significantly contribute
to the anisotropies measured by WMAP.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 10:42:28 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Atrio-Barandela",
"F.",
""
],
[
"Muecket",
"J. P.",
""
],
[
"Genova-Santos",
"R.",
""
]
] | [
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] |
801.1199 | George Lukes Gerakopoulos | Georgios Lukes-Gerakopoulos, Spyros Basilakos, George Contopoulos | Dynamics and chaos in the unified scalar field Cosmology | 9 pages, 5 figures, accepted for publication by Phys. Rev. D | Phys.Rev.D77:043521,2008 | 10.1103/PhysRevD.77.043521 | null | astro-ph | null | We study the dynamics of the closed scalar field FRW cosmological models in
the framework of the so called Unified Dark Matter (UDM) scenario. Performing a
theoretical as well as a numerical analysis we find that there is a strong
indication of chaos in agreement with previous studies. We find that a positive
value of the spatial curvature is essential for the appearance of chaoticity,
though the Lyapunov number seems to be independent of the curvature value.
Models that are close to flat exhibit a chaotic behavior after a long time
while pure flat models do not exhibit any chaos. Moreover, we find that some of
the semiflat models in the UDM scenario exhibit similar dynamical behavior with
the Lambda cosmology despite their chaoticity.
Finally, we compare the measured evolution of the Hubble parameter derived
from the differential ages of passively evolving galaxies with that expected in
the semiflat unified scalar field cosmology. Based on a specific set of initial
conditions we find that the UDM scalar field model matches well the
observational data.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:42:04 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Jan 2008 09:46:28 GMT"
},
{
"version": "v3",
"created": "Thu, 7 Feb 2008 10:51:50 GMT"
},
{
"version": "v4",
"created": "Fri, 15 Feb 2008 16:13:35 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Lukes-Gerakopoulos",
"Georgios",
""
],
[
"Basilakos",
"Spyros",
""
],
[
"Contopoulos",
"George",
""
]
] | [
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] |
801.12 | Edmond Orignac | S. De Palo, E. Orignac, R. Citro and M. L. Chiofalo | The low-energy excitation spectrum of one-dimensional dipolar quantum
gases | 5 pages, 3 EPS figures, RevTeX 4 | Phys. Rev. B 77, 212101 (2008) | 10.1103/PhysRevB.77.212101 | null | cond-mat.str-el cond-mat.other | null | We determine the excitation spectrum of a bosonic dipolar quantum gas in a
one-dimensional geometry, from the dynamical density-density correlation
functions simulated by means of Reptation Quantum Monte Carlo techniques. The
excitation energy is always vanishing at the first vector of the reciprocal
lattice in the whole crossover from the liquid-like at low density to the
quasi-ordered state at high density, demonstrating the absence of a roton
minimum. Gaps at higher reciprocal lattice vectors are seen to progressively
close with increasing density, while the quantum state evolves into a
quasi-periodic structure. The simulational data together with the
uncertainty-principle inequality also provide a rigorous proof of the absence
of long-range order in such a super-strongly correlated system. Our conclusions
confirm that the dipolar gas is in a Luttinger-liquid state, significantly
affected by the dynamical correlations. The connection with ongoing experiments
is also discussed.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 10:30:16 GMT"
}
] | 2008-06-24T00:00:00 | [
[
"De Palo",
"S.",
""
],
[
"Orignac",
"E.",
""
],
[
"Citro",
"R.",
""
],
[
"Chiofalo",
"M. L.",
""
]
] | [
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] |
801.1201 | Jesko Sirker | J. Sirker, S. Fujimoto, N. Laflorencie, S. Eggert, I. Affleck | Thermodynamics of impurities in the anisotropic Heisenberg spin-1/2
chain | 30 pages, 11 figures | J. Stat. Mech. (2008) P02015 | 10.1088/1742-5468/2008/02/P02015 | null | cond-mat.str-el | null | The thermodynamics of finite open antiferromagnetic XXZ chains is studied
using field theory, Bethe Ansatz and quantum Monte Carlo methods. For the
susceptibility a parameter-free result as a function of the number of sites L
and temperature T beyond the scaling limit is derived. The limiting cases T/J
>> 1/L (J being the exchange constant), where the boundary correction shows a
logarithmically suppressed Curie behaviour, and T/J << 1/L, where a crossover
to the ground state behaviour takes place, are discussed in detail. Based on
this analysis we present a simple formula for the averaged susceptibility of a
spin-1/2 chain doped with non-magnetic impurities. We show that the effective
Curie constant has a highly non-trivial temperature dependence and shows
scaling in the low-temperature limit. Finally, corrections due to intra- and
interchain couplings and implications for experiments on Sr_2 Cu_{1-x}Pd_x
O_{3+\delta} and related compounds are discussed.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 10:31:53 GMT"
}
] | 2008-03-03T00:00:00 | [
[
"Sirker",
"J.",
""
],
[
"Fujimoto",
"S.",
""
],
[
"Laflorencie",
"N.",
""
],
[
"Eggert",
"S.",
""
],
[
"Affleck",
"I.",
""
]
] | [
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] |
801.1202 | Doron Cohen | Swarnali Bandopadhyay and Doron Cohen | Renormalization of the dephasing by zero point fluctuations | 8 pages, 8 figures, improved version | Phys. Rev. B 77, 155438 (2008) | 10.1103/PhysRevB.77.155438 | null | cond-mat.mes-hall | null | We study the role of zero-point-fluctuations (ZPF) in dephasing at low
temperature. Unlike the Caldeira-Leggett model where the interaction is with an
homogeneous fluctuating field of force, here we consider the effect of short
range scattering by localized bath modes. We find that in presence of ZPF the
inelastic cross-section gets renormalized. Thus indirectly ZPF might contribute
to the dephasing at low temperature.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:03:34 GMT"
},
{
"version": "v2",
"created": "Fri, 28 Mar 2008 09:41:28 GMT"
}
] | 2008-05-02T00:00:00 | [
[
"Bandopadhyay",
"Swarnali",
""
],
[
"Cohen",
"Doron",
""
]
] | [
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] |
801.1203 | Marek Strumik | Marek Strumik and Wieslaw M. Macek | Testing for Markovian Character and Modeling of Intermittency in Solar
Wind Turbulence | null | null | 10.1103/PhysRevE.78.026414 | null | physics.plasm-ph physics.space-ph | null | We present results of statistical analysis of solar wind turbulence using an
approach based on the theory of Markov processes. It is shown that the
Chapman-Kolmogorov equation is approximately satisfied for the turbulent
cascade. We evaluate the first two Kramers-Moyal coefficients from experimental
data and show that the solution of the resulting Fokker-Planck equation agrees
well with experimental probability distributions. Our results suggest the
presence of a local transfer mechanism for magnetic field fluctuations in solar
wind turbulence.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:07:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Strumik",
"Marek",
""
],
[
"Macek",
"Wieslaw M.",
""
]
] | [
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] |
801.1204 | Narayan Banerjee | Narayan Banerjee, Sudipta Das, Koyel Ganguly | Chameleon field and the late time acceleration of the universe | 7 pages, 2 figures | Pramana 74:L481-L489,2010 | 10.1007/s12043-010-0044-5 | null | gr-qc astro-ph | null | In the present work, it is shown that a chameleon scalar field having a
nonminimal coupling with dark matter can give rise to a smooth transition from
a decelerated to an accelerated phase of expansion for the universe. It is
surprising to note that the coupling with the chameleon scalar field hardly
affects the evolution of the dark matter sector, which still redshifts as
$a^{-3}$.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:09:56 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Banerjee",
"Narayan",
""
],
[
"Das",
"Sudipta",
""
],
[
"Ganguly",
"Koyel",
""
]
] | [
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] |
801.1205 | Josep Marti | J. R. Sanchez-Sutil, J. Marti, J. A. Combi, P. Luque-Escamilla, A. J.
Munoz-Arjonilla, J. M. Paredes and G. Pooley | Faint arc-minute extended radio emission around Cygnus X-3 | 7 pages, 5 figures. Accepted for publication by Astronomy &
Astrophysics | null | 10.1051/0004-6361:20078498 | null | astro-ph | null | Aims. We revisit the vicinity of the microquasar Cygnus X-3 at radio
wavelengths. We aim to improve our previous search for possible associated
extended radio features/hot spots in the position angle of the Cygnus X-3
relativistic jets focusing on shorter angular scales than previously explored.
Methods. Our work is mostly based on analyzing modern survey and archive
radio data, mainly including observations carried out with the Very Large Array
and the Ryle Telescopes. We also used deep near-infrared images that we
obtained in 2005.
Results. We present new radio maps of the Cygnus X-3 field computed after
combining multi-configuration Very Large Array archive data at 6 cm and
different observing runs at 2 cm with the Ryle Telescope. These are probably
among the deepest radio images of Cygnus X-3 reported to date at cm
wavelengths. Both interferometers reveal an extended radio feature within a few
arc-minutes of the microquasar position, thus making our detection more
credible. Moreover, this extended emission is possibly non-thermal, although
this point still needs confirmation. Its physical connection with the
microquasar is tentatively considered under different physical scenarios. We
also report on the serendipitous discovery of a likely Fanaroff-Riley type II
radio galaxy only 3 arc-minute away from Cygnus X-3.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:14:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Sanchez-Sutil",
"J. R.",
""
],
[
"Marti",
"J.",
""
],
[
"Combi",
"J. A.",
""
],
[
"Luque-Escamilla",
"P.",
""
],
[
"Munoz-Arjonilla",
"A. J.",
""
],
[
"Paredes",
"J. M.",
""
],
[
"Pooley",
"G.",
""
]
] | [
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] |
801.1206 | Marcin Daszkiewicz | Marcin Daszkiewicz (University of Wroclaw) | Canonical and Lie-algebraic twist deformations of Galilei algebra | 14 pages, no figures, v2: the page numbers for all references in
preprint version are provided; one reference is added (as in journal version) | Mod.Phys.Lett.A23:505-517,2008 | 10.1142/S0217732308026479 | IFT UWr LV-420 | hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We describe various nonrelativistic contractions of two classes of twisted
Poincare algebra: canonical one ($\theta_{\mu\nu}$-deformation) and the one
leading to Lie-algebraic models of noncommutative space-times. The cases of
contraction-independent and contraction-dependent twist parameters are
considered. We obtain five models of noncommutative nonrelativistic
space-times, in particular, two new Lie-algebraic nonrelativistic deformations
of space-time, respectively, with quantum time/classical space and with quantum
space/classical time.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:16:33 GMT"
},
{
"version": "v2",
"created": "Tue, 27 Jan 2009 11:34:05 GMT"
}
] | 2009-01-27T00:00:00 | [
[
"Daszkiewicz",
"Marcin",
"",
"University of Wroclaw"
]
] | [
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] |
801.1207 | Kossivi Adjamagbo | Kossivi Adjamagbo | Adjamagbo Determinant and Serre conjecture for linear groups over Weyl
algebras | null | null | null | null | math.KT math.RA | null | Thanks to the theory of determinants over an Ore domain, also called
Adjamagbo determinant by the Russian school of non commutative algebra, we
extend to any Weyl algebra over a field of characteristic zero Suslin theorem
solving what Suslin himself called the $K_1$-analogue of the well-known Serre
Conjecture and asserting that for any integer $n$ greater than 2, any $n$ by
$n$ matrix with coefficients in any algebra of polynomials over a field and
with determinant one is the product of elementary matrices with coefficients in
this algebra
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:26:45 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Adjamagbo",
"Kossivi",
""
]
] | [
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] |
801.1208 | Guangwen Li | Guangwen Li, Dashe Li, Yuling Wang, Wenyan Sun | Hybrid Decoding of Finite Geometry LDPC Codes | 19 pages, 5 figures, 5 tables | null | null | null | cs.IT math.IT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | For finite geometry low-density parity-check codes, heavy row and column
weights in their parity check matrix make the decoding with even Min-Sum (MS)
variants computationally expensive. To alleviate it, we present a class of
hybrid schemes by concatenating a parallel bit flipping (BF) variant with an
Min-Sum (MS) variant. In most SNR region of interest, without compromising
performance or convergence rate, simulation results show that the proposed
hybrid schemes can save substantial computational complexity with respect to MS
variant decoding alone. Specifically, the BF variant, with much less
computational complexity, bears most decoding load before resorting to MS
variant. Computational and hardware complexity is also elaborated to justify
the feasibility of the hybrid schemes.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:29:44 GMT"
},
{
"version": "v2",
"created": "Tue, 7 Oct 2008 14:51:48 GMT"
},
{
"version": "v3",
"created": "Tue, 20 Jan 2009 06:38:30 GMT"
},
{
"version": "v4",
"created": "Thu, 2 Jul 2009 18:24:34 GMT"
}
] | 2009-07-02T00:00:00 | [
[
"Li",
"Guangwen",
""
],
[
"Li",
"Dashe",
""
],
[
"Wang",
"Yuling",
""
],
[
"Sun",
"Wenyan",
""
]
] | [
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] |
801.1209 | Ludkovsky Sergey Victor | S.V. Ludkovsky | Stochastic processes and their spectral representations over
non-archimedean fields | null | 2010, Indian J. of Mathem., V. 52:1 | null | null | math.PR math.FA | null | The article is devoted to stochastic processes with values in finite- and
infinite-dimensional vector spaces over infinite fields $\bf K$ of zero
characteristics with non-trivial non-archimedean norms. For different types of
stochastic processes controlled by measures with values in $\bf K$ and in
complete topological vector spaces over $\bf K$ stochastic integrals are
investigated. Vector valued measures and integrals in spaces over $\bf K$ are
studied. Theorems about spectral decompositions of non-archimedean stochastic
processes are proved.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:30:02 GMT"
}
] | 2018-12-18T00:00:00 | [
[
"Ludkovsky",
"S. V.",
""
]
] | [
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] |
801.121 | Daniel Lombra\~na Gonz\'alez | Daniel Lombrana Gonzalez, Francisco Fernandez de Vega, L. Trujillo, G.
Olague, F. Chavez de la O, M. Cardenas, L. Araujo, P. Castillo, K. Sharman | Increasing GP Computing Power via Volunteer Computing | First draft, preparing for PPSN 2008 | null | null | null | cs.DC | null | This paper describes how it is possible to increase GP Computing Power via
Volunteer Computing (VC) using the BOINC framework. Two experiments using
well-known GP tools -Lil-gp & ECJ- are performed in order to demonstrate the
benefit of using VC in terms of computing power and speed up. Finally we
present an extension of the model where any GP tool or framework can be used
inside BOINC regardless of its programming language, complexity or required
operating system.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:36:35 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Gonzalez",
"Daniel Lombrana",
""
],
[
"de Vega",
"Francisco Fernandez",
""
],
[
"Trujillo",
"L.",
""
],
[
"Olague",
"G.",
""
],
[
"de la O",
"F. Chavez",
""
],
[
"Cardenas",
"M.",
""
],
[
"Araujo",
"L.",
""
],
[
"Castillo",
"P.",
""
],
[
"Sharman",
"K.",
""
]
] | [
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] |
801.1211 | Alok Gupta Dr. | A. C. Gupta (1), W. G. Deng (2,1), U. C. Joshi (3), J. M. Bai (1) and
M. G. Lee (4) ((1) National Astronomical Observatories / Yunnan Observatory,
CAS, Kunming, Yunnan, China (2) Department of Physics, Yunnan University,
Kunming, Yunnan, China (3) Astronomy and Astrophysics Division, Physical
Research Laboratory, Navrangpura, Ahmedabad, India (4) Astronomy Program,
Seoul National University, Seoul, South Korea) | Multi-color Optical Variability of the TeV Blazar Mrk 501 in the
Low-State | 4 figures, 4 tables, Accepted for publication in New Astronomy | New Astron.13:375-384,2008 | 10.1016/j.newast.2007.12.001 | null | astro-ph | null | We report results based on the monitoring of the BL Lac object Mrk 501 in the
optical (B, V and R) passbands from March to May 2000. Observations spread over
12 nights were carried out using 1.2 meter Mount Abu Telescope, India and 61 cm
Telescope at Sobaeksan Astronomy Observatory, South Korea. The aim is to study
the intra-day variability (IDV), short term variability and color variability
in the low state of the source. We have detected flux variation of 0.05 mag in
the R-band in time scale of 15 min in one night. In the B and V passbands, we
have less data points and it is difficult to infer any IDVs. Short term flux
variations are also observed in the V and R bands during the observing run. No
significant variation in color (B$-$R) has been detected but (V$-$R) shows
variation during the present observing run.
Assuming the shortest observed time scale of variability (15 min) to
represent the disk instability or pulsation at a distance of 5 Schwarschild
radii from the black hole (BH), mass of the central BH is estimated $\sim$ 1.20
$\times$ 10$^{8} M_{\odot}$.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:49:06 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Gupta",
"A. C.",
""
],
[
"Deng",
"W. G.",
""
],
[
"Joshi",
"U. C.",
""
],
[
"Bai",
"J. M.",
""
],
[
"Lee",
"M. G.",
""
]
] | [
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] |
801.1212 | Martin Goldstern | Martin Goldstern | The typical countable algebra | null | null | null | null | math.RA math.LO | null | We argue that it makes sense to talk about ``typical'' properties of
lattices, and then show that there is, up to isomorphism, a unique countable
lattice L* (the Fraisse limit of the class of finite lattices) that has all
``typical'' properties.
Among these properties are: L* is simple and locally finite, every order
preserving function can be interpolated by a lattice polynomial, and every
finite lattice or countable locally finite lattice embeds into L*.
The same arguments apply to other classes of algebras assuming they have a
Fraisse limit and satisfy the finite embeddability property.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:58:03 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Goldstern",
"Martin",
""
]
] | [
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] |
801.1213 | Ryan Houghton | R. C. W. Houghton, N. Thatte | The Central Region of M83 | Accepted for publication in MNRAS. 24 pages, 11 figures | null | 10.1111/j.1365-2966.2008.12893.x | null | astro-ph | null | We combine VLT/ISAAC NIR spectroscopy with archival HST/WFPC2 and HST/NICMOS
imaging to study the central 20"x20" of M83. Our NIR indices for clusters in
the circumnuclear star-burst region are inconsistent with simple instantaneous
burst models. However, models of a single burst dispersed over a duration of 6
Myrs fit the data well and provide the clearest evidence yet of an age gradient
along the star forming arc, with the youngest clusters nearest the north-east
dust lane. The long slit kinematics show no evidence to support previous claims
of a second hidden mass concentration, although we do observe changes in
molecular gas velocity consistent with the presence of a shock at the edge of
the dust lane.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:55:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Houghton",
"R. C. W.",
""
],
[
"Thatte",
"N.",
""
]
] | [
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801.1214 | Kossivi Adjamagbo | Kossivi Adjamagbo | Sur le Th\'eor\`eme Principal de Zariski en G\'eom\'etrie Alg\'ebrique
et G\'eom\'etrie Analytique | null | null | null | null | math.AG math.CV | null | On Zariski Main Theorem in Algebraic Geometry and Analytic Geometry. We fill
a surprising gap of Complex Analytic Geometry by proving the analogue of
Zariski Main Theorem in this geometry, i.e. proving that an holomorphic map
from an irreducible analytic space to a normal irreducible one is an open
embedding if and only if all its fibers are discrete and it induces a
bimeromorphic map on its image. We prove more generally the "Generalized
Zariski Main Theorem for analytic spaces", which claims that an holomorphic map
from an irreducible analytic space to a irreducible locally irreducible one is
an open embedding if and only if it is flat and induces a bimeromorphic map on
its image. Thanks to the "analytic criterion of regularity" of Serre-Samuel in
GAGA [12] and to "Lefschetz Principle", we finally deduce the "Generalized
Zariski Main Theorem for algebraic varieties of characteristical zero", which
claims that a morphism from such an irreducible variety to an irreducible
unibranch one is an open immersion if and only if it is birational and flat.
-----
Nous comblons une lacune \'etonnante de la G\'eom\'etrie Analytique Complexe
en prouvant l'analogue du Th\'eor\`eme Principal de Zariski dans cette
g\'eom\'etrie, c'est-\`a-dire en prouvant que toute application holomorphe d'un
espace analytique irreductible dans un espace analytique normal et irreductible
est un plongement ouvert si et seulement si toutes ses fibres sont discr\`etes
et si elle induit une application bim\'eromorphe sur son image. Nous prouvons
plus g\'en\'eralement le ``Th\'eor\`eme Principal de Zariski G\'en\'eralis\'e
pour les espaces analytiques'', qui affirme qu'une application holomorphe d'un
espace analytique irreductible dans un espace analytique irreductible et
localement irreductible est un plongement ouvert si et seulement si elle est
plate et induit une application bim\'eromorphe sur son image. Gr\^ace au
``crit\^ere analytique de r\'egularit\'e'' de Serre-Samuel dans GAGA
\cite{serre} et au ``Principe de Lefschetz'', nous en d\'eduisons enfin le
``Th\'eor\`eme Principal de Zariski G\'en\'eralis\'e pour les vari\'et\'es
alg\'ebriques de caract\'eristique nulle'', qui affirme qu'un morphisme d'une
telle vari\'et\'e irreductible dans une autre unibranche est une immersion
ouverte si et seulement s'il est birationnel et plat.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 11:58:56 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Adjamagbo",
"Kossivi",
""
]
] | [
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] |
801.1215 | Robert Dunn | R. J. H. Dunn (1) and A. C. Fabian (2) ((1) University of Southampton,
UK (2) Institute of Astronomy, Cambridge, UK) | Investigating Heating and Cooling in the BCS & B55 Cluster Samples | 12 pages, 9 figures, accepted for publication in MNRAS | null | 10.1111/j.1365-2966.2008.12898.x | null | astro-ph | null | We study clusters in the BCS cluster sample which are observed by Chandra and
are more distant than redshift, z>0.1. We select from this subsample the
clusters which have both a short central cooling time and a central temperature
drop, and also those with a central radio source. Six of the clusters have
clear bubbles near the centre. We calculate the heating by these bubbles and
express it as the ratio r_heat/r_cool=1.34+/-0.20. This result is used to
calculate the average size of bubbles expected in all clusters with central
radio sources. In three cases the predicted bubble sizes approximately match
the observed radio lobe dimensions.
We combine this cluster sample with the B55 sample studied in earlier work to
increase the total sample size and redshift range. This extended sample
contains 71 clusters in the redshift range 0<z<0.4. The average distance out to
which the bubbles offset the X-ray cooling in the combined sample is at least
r_heat/r_cool=0.92+/-0.11. The distribution of central cooling times for the
combined sample shows no clusters with clear bubbles and t_cool>1.2Gyr. An
investigation of the evolution of cluster parameters within the redshift range
of the combined samples does not show any clear variation with redshift.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 12:23:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dunn",
"R. J. H.",
""
],
[
"Fabian",
"A. C.",
""
]
] | [
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801.1216 | Damiano Anselmi | Damiano Anselmi | Weighted scale invariant quantum field theories | 29 pages, 3 figures; v2: JHEP version | JHEP 0802:051,2008 | 10.1088/1126-6708/2008/02/051 | IFUP-TH 2007/34 | hep-th | null | We study a class of Lorentz violating quantum field theories that contain
higher space derivatives, but no higher time derivatives, and become
renormalizable in the large N expansion. The fixed points of their
renormalization-group flows provide examples of exactly "weighted scale
invariant" theories, which are noticeable Lorentz violating generalizations of
conformal field theories. We classify the scalar and fermion models that are
causal, stable and unitary. Solutions exist also in four and higher dimensions,
even and odd. In some explicit four dimensional examples, we compute the
correlation functions to the leading order in 1/N and the critical exponents to
the subleading order. We construct also RG flows interpolating between pairs of
fixed points.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 12:16:57 GMT"
},
{
"version": "v2",
"created": "Sun, 17 Feb 2008 15:36:50 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Anselmi",
"Damiano",
""
]
] | [
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] |
801.1217 | Alok Gupta Dr. | A. C. Gupta (1), J. H. Fan (2), J. M. Bai (1) and S. J. Wagner (3)((1)
National Astronomical Observatories / Yunnan Observatory, CAS, Kunming,
Yunnan, China (2) Center for Astrophysics, Guangzhou University, Guangzhou,
China (3) Landessternwarte, Konigstuhl, Heidelberg, Germany) | Optical Intra-day Variability in Blazars | 7 figures, 4 tables, Accepted for publication in Astronomical Journal | Astronomical Journal, 135, 1384-1394, (2008) | 10.1088/0004-6256/135/4/1384 | null | astro-ph | null | We selected a sample of a dozen blazars which are the prime candidates for
simultaneous multi-wavelength observing campaigns in their outburst phase. We
searched for optical outbursts, intra-day variability and short term
variability in these blazars. We carried out optical photometric monitoring of
nine of these blazars in 13 observing nights during our observing run October
27, 2006 - March 20, 2007 by using the 1.02 meter optical telescope. From our
observations, our data favor the hypothesis that three blazars were in the
outburst state; one blazar was in the post outburst state; three blazars were
in the pre/post outburst state; one blazar was in the low-state; and the state
of one blazar was not known because there is not much optical data available
for the blazar to compare with our observations. Out of three nights of
observations of AO 0235+164, intra-day variability was detected in two nights.
Out of five nights of observations of S5 0716+714, intra-day variability was
detected in two nights. In one night of observations of PKS 0735+178, intra-day
variability was detected. Out of six nights of observations of 3C 454.3,
intra-day variability was detected in three nights. No intra-day variability
was detected in S2 0109+224, OJ 287, ON 231, 3C 279 and 1ES 2344+514 in their
1, 4, 1, 2 and 1 nights of observations respectively. AO 0235+164, S5 0716+714,
OJ 287, 3C 279 and 3C 454.3 were observed in more than one night and short term
variations in all these blazars were also noticed. From our observations and
the available data, we found that the predicted optical outburst with the time
interval of ~ 8 years in AO 0235+164 and ~ 3 years in S5 0716+714 have possibly
occurred.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 12:17:26 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gupta",
"A. C.",
""
],
[
"Fan",
"J. H.",
""
],
[
"Bai",
"J. M.",
""
],
[
"Wagner",
"S. J.",
""
]
] | [
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801.1218 | Arun Kenath Mr | C Sivaram (Indian Institute of Astrophysics, Bangalore, India) | Scaling Relations for self-Similar Structures and the Cosmological
Constant | 7 pages, 17 equations | null | null | null | astro-ph | null | Scaling relations for the mass, angular momentum and other properties of a
wide range of self-similar structures in the universe are seen to have
universal features. As a consequence of the ideas elaborated in earlier papers
these relations can be connected to a background constant curvature given by
the cosmological constant dominating cosmical dynamics.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 12:26:53 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Sivaram",
"C",
"",
"Indian Institute of Astrophysics, Bangalore, India"
]
] | [
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] |
801.1219 | Andrey Breslav | Andrey Breslav | DSL development based on target meta-models. Using AST transformations
for automating semantic analysis in a textual DSL framework | 15 pages, 3 figures | null | null | null | cs.PL | null | This paper describes an approach to creating textual syntax for Do-
main-Specific Languages (DSL). We consider target meta-model to be the main
artifact and hence to be developed first. The key idea is to represent analysis
of textual syntax as a sequence of transformations. This is made by explicit
opera- tions on abstract syntax trees (ATS), for which a simple language is
proposed. Text-to-model transformation is divided into two parts: text-to-AST
(developed by openArchitectureWare [1]) and AST-to-model (proposed by this
paper). Our approach simplifies semantic analysis and helps to generate as much
as possi- ble.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 12:28:18 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Breslav",
"Andrey",
""
]
] | [
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] |
801.122 | Stephen Connor | Stephen B. Connor, Saul D. Jacka | Optimal co-adapted coupling for the symmetric random walk on the
hypercube | 14 pages; added references and publication information | Journal of Applied Probability 45(1) (2008) 703-713 | null | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let X and Y be two simple symmetric continuous-time random walks on the
vertices of the n-dimensional hypercube. We consider the class of co-adapted
couplings of these processes, and describe an intuitive coupling which is shown
to be the fastest in this class.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 12:32:46 GMT"
},
{
"version": "v2",
"created": "Thu, 16 Oct 2008 08:40:44 GMT"
}
] | 2008-10-16T00:00:00 | [
[
"Connor",
"Stephen B.",
""
],
[
"Jacka",
"Saul D.",
""
]
] | [
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] |
801.1221 | Laurent Bruneau | Laurent Bruneau and Francois Germinet | On the singularity of random matrices with independent entries | to be published in the Proc. Amer. Math. Soc | null | null | null | math.PR | null | We consider n by n real matrices whose entries are non-degenerate random
variables that are independent but non necessarily identically distributed, and
show that the probability that such a matrix is singular is O(1/sqrt{n}). The
purpose of this note is to provide a short and elementary proof of this fact
using a Bernoulli decomposition of arbitrary non degenerate random variables.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 12:49:33 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Bruneau",
"Laurent",
""
],
[
"Germinet",
"Francois",
""
]
] | [
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] |
801.1222 | Nils Bluemer | N. Bl\"umer | Multigrid Hirsch-Fye quantum Monte Carlo method for dynamical mean-field
theory | 4+e pages, 6 figures | null | null | null | cond-mat.str-el | null | We present a new algorithm which allows for direct numerically exact
solutions within dynamical mean-field theory (DMFT). It is based on the
established Hirsch-Fye quantum Monte Carlo (HF-QMC) method. However, the DMFT
impurity model is solved not at fixed imaginary-time discretization Delta_tau,
but for a range of discretization grids; by extrapolation, unbiased Green
functions are obtained in each DMFT iteration. In contrast to conventional
HF-QMC, the multigrid algorithm converges to the exact DMFT fixed points. It
extends the useful range of Delta_tau, is precise and reliable even in the
immediate vicinity of phase transitions and is more efficient, also in
comparison to continuous-time methods. Using this algorithm, we show that the
spectral weight transfer at the Mott transition has been overestimated in a
recent density matrix renormalization group study.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:41:02 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Blümer",
"N.",
""
]
] | [
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] |
801.1223 | Karin \"Oberg | Karin I. Oberg, A. C. Adwin Boogert, Klaus M. Pontoppidan, Geoffrey A.
Blake, Neal J. Evans, Fred Lahuis and Ewine F. van Dishoeck | The c2d Spitzer spectroscopy survey of ices around low-mass young
stellar objects, III: CH4 | 27 pages, 7 figures, accepted by ApJ | null | 10.1086/533432 | null | astro-ph | null | CH4 is proposed to be the starting point of a rich organic chemistry. Solid
CH4 abundances have previously been determined mostly toward high mass star
forming regions. Spitzer/IRS now provides a unique opportunity to probe solid
CH4 toward low mass star forming regions as well. Infrared spectra from the
Spitzer Space Telescope are presented to determine the solid CH4 abundance
toward a large sample of low mass young stellar objects. 25 out of 52 ice
sources in the $c2d$ (cores to disks) legacy have an absorption feature at 7.7
um, attributed to the bending mode of solid CH4. The solid CH4 / H2O abundances
are 2-8%, except for three sources with abundances as high as 11-13%. These
latter sources have relatively large uncertainties due to small total ice
column densities. Toward sources with H2O column densities above 2E18 cm-2, the
CH4 abundances (20 out of 25) are nearly constant at 4.7+/-1.6%. Correlation
plots with solid H2O, CH3OH, CO2 and CO column densities and abundances
relative to H2O reveal a closer relationship of solid CH4 with CO2 and H2O than
with solid CO and CH3OH. The inferred solid CH4 abundances are consistent with
models where CH4 is formed through sequential hydrogenation of C on grain
surfaces. Finally the equal or higher abundances toward low mass young stellar
objects compared with high mass objects and the correlation studies support
this formation pathway as well, but not the two competing theories: formation
from CH3OH and formation in gas phase with subsequent freeze-out.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 13:28:14 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Oberg",
"Karin I.",
""
],
[
"Boogert",
"A. C. Adwin",
""
],
[
"Pontoppidan",
"Klaus M.",
""
],
[
"Blake",
"Geoffrey A.",
""
],
[
"Evans",
"Neal J.",
""
],
[
"Lahuis",
"Fred",
""
],
[
"van Dishoeck",
"Ewine F.",
""
]
] | [
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] |
801.1224 | Bartlomiej Waclaw | B. Waclaw, Z. Burda | Counting metastable states of Ising spin glasses on arbitrary graphs | 8 pages, 4 figures (one in color), additional materials can be found
under http://www.physik.uni-leipzig.de/~waclaw/glasses-data.htm | Phys. Rev. E 77, 041114 (2008) | 10.1103/PhysRevE.77.041114 | null | cond-mat.dis-nn cond-mat.stat-mech | null | Using a field-theoretical representation of the Tanaka-Edwards integral we
develop a method to systematically compute the number N_s of 1-spin-stable
states (local energy minima) of a glassy Ising system with nearest-neighbor
interactions and random Gaussian couplings on an arbitrary graph. In
particular, we use this method to determine N_s for K-regular random graphs and
d-dimensional regular lattices for d=2,3. The method works also for other
graphs. Excellent accuracy of the results allows us to observe that the number
of local energy minima depends mainly on local properties of the graph on which
the spin glass is defined.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 13:10:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Waclaw",
"B.",
""
],
[
"Burda",
"Z.",
""
]
] | [
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] |
801.1225 | Thomas Borek | Thomas Borek | Arakelov theory of noncommutative arithmetic surfaces | 20 pages | null | null | null | math.NT math.AG | null | The purpose of this paper is to initiate Arakelov theory in a noncommutative
setting. More precisely, we are concerned with noncommutative arithmetic
surfaces. We introduce a version of arithmetic intersection theory on
noncommutative arithmetic surfaces and we prove an arithmetic Riemann-Roch
theorem in this setup.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 13:12:30 GMT"
},
{
"version": "v2",
"created": "Mon, 24 Mar 2008 00:30:14 GMT"
}
] | 2008-03-24T00:00:00 | [
[
"Borek",
"Thomas",
""
]
] | [
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] |
801.1226 | Christoph Lehner | C. Lehner, T. Wettig, T. Guhr, Y. Wei | Character expansion method for supergroups and extended superversions of
the Leutwyler-Smilga and Berezin-Karpelevich integrals | 18 pages, 2 figures; added acknowledgment; added appendices, minor
changes, as published in J. Math. Phys. | J.Math.Phys.49:063510,2008 | 10.1063/1.2940572 | null | math-ph hep-th math.MP | null | We introduce an extension of the character expansion method to the case of
supergroups. This method allows us to calculate a superversion of the
Leutwyler-Smilga integral which, to the best of our knowledge, has not been
calculated before. We also use the method to generalize a previously calculated
superversion of the Berezin-Karpelevich integral. Our character expansion
method should also allow for the calculation of other supergroup integrals.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 18:09:09 GMT"
},
{
"version": "v2",
"created": "Sat, 16 Feb 2008 16:35:17 GMT"
},
{
"version": "v3",
"created": "Sat, 24 May 2008 17:21:48 GMT"
}
] | 2009-01-28T00:00:00 | [
[
"Lehner",
"C.",
""
],
[
"Wettig",
"T.",
""
],
[
"Guhr",
"T.",
""
],
[
"Wei",
"Y.",
""
]
] | [
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] |
801.1227 | Qiang Yuan | Xiao-Jun Bi (1,2), Tian-Lu Chen (3,4), Yue Wang (1), Qiang Yuan (1,4)
((1)Key Laboratory of Particle Astrophysics, Institute of High Energy
Physics, Chinese Academy of Sciences; (2)Center for High Energy Physics,
Peking University; (3)Physics Department of Science School, Tibet University;
(4)The Key Laboratory of Cosmic Rays, Ministry of Education) | The diffuse GeV-TeV $\gamma$-ray emission of the Cygnus region | 14 pages (aastex), 5 figures, accepted for publication by The
Astrophysical Journal | Astrophys.J.695:883-887,2009 | 10.1088/0004-637X/695/2/883 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Recently the Milagro experiment observed diffuse multi-TeV gamma-ray emission
in the Cygnus region, which is significantly stronger than what predicted by
the Galactic cosmic ray model. However, the sub-GeV observation by EGRET shows
no excess to the prediction based on the same model. This TeV excess implies
possible high energy cosmic rays populated in the region with harder spectrum
than that observed on the Earth. In the work we studied this theoretical
speculation in detail. We find that, a diffuse proton source with power index
$\alpha_p\lesssim 2.3$, or a diffuse electron source with power index
$\alpha_e\lesssim2.6$ can reproduce the Milagro's observation without
conflicting with the EGRET data. Further detections on neutrinos, a diagnostic
of the hadronic model, and hard X-ray synchrontron radiation, a diagnostic of
the lepton model, help to break this degeneracy. In combination with the gamma
ray observations to several hundred GeV by Fermi, we will be able to understand
the diffuse emission mechanisms in the Cygnus region better.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 13:20:21 GMT"
},
{
"version": "v2",
"created": "Fri, 6 Feb 2009 01:55:01 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Bi",
"Xiao-Jun",
""
],
[
"Chen",
"Tian-Lu",
""
],
[
"Wang",
"Yue",
""
],
[
"Yuan",
"Qiang",
""
]
] | [
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] |
801.1228 | Wagner L. F. Marcolino | W. L. F. Marcolino (LAM) | WELS - Ultraviolet Spectra and Expanding Atmosphere Models | To appear in the proceedings of the "Hydrogen-Deficient Stars"
meeting, held in Tuebingen, Germany, Sept. 17-21, 2007. 4 pages | null | null | null | astro-ph | null | The ultraviolet spectra of all "weak emission line central stars of planetary
nebulae" (WELS) with available IUE data is analyzed. We found that the WELS can
be divided in three different groups regarding their UV: (1) Strong P-Cygni
profiles (mainly in C IV 1549); (2) Weak P-Cygni features and (3) Absence of
P-Cygni profiles. We have measured wind terminal velocities for all objects
presenting P-Cygni profiles in N V 1238 and/or C IV 1549. The results obtained
were compared to the UV data of the two prototype stars of the [WC]-PG 1159
class, namely, A30 and A78. They indicate that WELS are distinct from the
[WC]-PG 1159 stars, in contrast to previous claims in the literature. In order
to gain a better understanding about the WELS, we clearly need to determine
their physical parameters and chemical abundances. First non LTE expanding
atmosphere models (using the CMFGEN code) for the UV and optical spectra of the
star Hen 2-12 are presented.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 13:21:01 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Marcolino",
"W. L. F.",
"",
"LAM"
]
] | [
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] |
801.1229 | Hjalmar Rosengren | Hjalmar Rosengren | An Izergin-Korepin-type identity for the 8VSOS model, with applications
to alternating sign matrices | 22 pages. Essential changes in Section 8, explaining relation to
three-colour model | Adv. Appl. Math. 43 (2009), 137-155 | null | null | math.CO math-ph math.MP nlin.SI | null | We obtain a new expression for the partition function of the 8VSOS model with
domain wall boundary conditions, which we consider to be the natural extension
of the Izergin-Korepin formula for the six-vertex model. As applications, we
find dynamical (in the sense of the dynamical Yang-Baxter equation)
generalizations of the enumeration and 2-enumeration of alternating sign
matrices. The dynamical enumeration has a nice interpretation in terms of
three-colourings of the square lattice.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 13:43:13 GMT"
},
{
"version": "v2",
"created": "Wed, 7 May 2008 09:34:05 GMT"
}
] | 2014-06-16T00:00:00 | [
[
"Rosengren",
"Hjalmar",
""
]
] | [
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] |
801.123 | Nakamura Kentaro | Kentaro Nakamura | Classification of two dimensional split trianguline representations of
$p$-adic fields | 1st version 47pages, 2nd version 52pages | null | 10.1112/S0010437X09004059 | null | math.NT math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The aim of this paper is to classify two dimensional split trianguline
representations of $p$-adic fields. This is a generalization of a result of
Colmez who classified two dimensional split trianguline representations of
$\mathrm{Gal}(\bar{\mathbb{Q}}_p/\mathbb{Q}_p)$ by using
$(\phi,\Gamma)$-modules over Robba ring. In this paper, we classify two
dimensional split trianguline representations of $\mathrm{Gal}(\bar{K}/K)$ for
general $p$-adic field $K$ by using $B$-pairs defined by Berger.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 13:34:09 GMT"
},
{
"version": "v2",
"created": "Sat, 1 Nov 2008 20:07:27 GMT"
}
] | 2014-01-14T00:00:00 | [
[
"Nakamura",
"Kentaro",
""
]
] | [
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] |
801.1231 | Dieter Bauer | M. Kundu, D. Bauer | Optimizing the ionization and energy absorption of laser-irradiated
clusters | 10 page, 8 figures, RevTeX | null | 10.1063/1.2896578 | null | physics.plasm-ph physics.atm-clus physics.optics | null | It is known that rare-gas or metal clusters absorb incident laser energy very
efficiently. However, due to the intricate dependencies on all the laser and
cluster parameters it is difficult to predict under which circumstances
ionization and energy absorption is optimal.
With the help of three-dimensional particle-in-cell simulations of xenon
clusters (up to 17256 atoms) we find that for a given laser pulse energy and
cluster an optimum wavelength exists which corresponds to the approximate
wavelength of the transient, linear Mie-resonance of the ionizing cluster at an
early stage of negligible expansion. In a single ultrashort laser pulse, the
linear resonance at this optimum wavelength yields much higher absorption
efficiency than in the conventional, dual-pulse pump-probe set-up of linear
resonance during cluster expansion.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 13:38:58 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kundu",
"M.",
""
],
[
"Bauer",
"D.",
""
]
] | [
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] |
801.1232 | Xiangxiang Xue | X.-X. Xue, H.-W. Rix, G. Zhao, P. Re Fiorentin, T. Naab, M. Steinmetz,
F. C. van den Bosch, T. C. Beers, Y. S. Lee, E. F. Bell, C. Rockosi, B.
Yanny, H. Newberg, R. Wilhelm, X. Kang, M. C. Smith, and D. P. Schneider | The Milky Way's Circular Velocity Curve to 60 kpc and an Estimate of the
Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch
Stars | 42 pages, 17 figures and 3 table. Accepted by APJ | Astrophys.J.684:1143-1158,2008 | 10.1086/589500 | null | astro-ph | null | We derive new constraints on the mass of the Milky Way's dark matter halo,
based on a set of halo stars from SDSS as kinematic tracers. Our sample
comprises 2401 rigorously selected Blue Horizontal-Branch (BHB) halo stars
drawn from SDSS DR-6. To interpret these distributions, we compare them to
matched mock observations drawn from two different cosmological galaxy
formation simulations designed to resemble the Milky Way, which we presume to
have an appropriate orbital distribution of halo stars. We then determine which
value of $\rm V_{cir}(r)$ brings the observed distribution into agreement with
the corresponding distributions from the simulations. This procedure results in
an estimate of the Milky Way's circular velocity curve to $\sim 60$ kpc, which
is found to be slightly falling from the adopted value of $\rm 220 km s^{-1}$
at the Sun's location, and implies M$(<60 \rm kpc) = 4.0\pm 0.7\times
10^{11}$M$_\odot$. The radial dependence of $\rm V_{cir}(r)$, derived in
statistically independent bins, is found to be consistent with the expectations
from an NFW dark matter halo with the established stellar mass components at
its center. If we assume an NFW halo profile of characteristic concentration
holds, we can use the observations to estimate the virial mass of the Milky
Way's dark matter halo, M$_{\rm vir}=1.0^{+0.3}_{-0.2} \times
10^{12}$M$_\odot$, which is lower than many previous estimates. This estimate
implies that nearly 40% of the baryons within the virial radius of the Milky
Way's dark matter halo reside in the stellar components of our Galaxy. A value
for M$_{\rm vir}$ of only $\sim 1\times10^{12}$M$_\odot$ also (re-)opens the
question of whether all of the Milky Way's satellite galaxies are on bound
orbits.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:13:45 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Jan 2008 11:35:05 GMT"
},
{
"version": "v3",
"created": "Mon, 14 Jan 2008 09:38:06 GMT"
},
{
"version": "v4",
"created": "Fri, 11 Apr 2008 22:02:20 GMT"
},
{
"version": "v5",
"created": "Wed, 28 May 2008 22:06:02 GMT"
}
] | 2008-11-07T00:00:00 | [
[
"Xue",
"X. -X.",
""
],
[
"Rix",
"H. -W.",
""
],
[
"Zhao",
"G.",
""
],
[
"Fiorentin",
"P. Re",
""
],
[
"Naab",
"T.",
""
],
[
"Steinmetz",
"M.",
""
],
[
"Bosch",
"F. C. van den",
""
],
[
"Beers",
"T. C.",
""
],
[
"Lee",
"Y. S.",
""
],
[
"Bell",
"E. F.",
""
],
[
"Rockosi",
"C.",
""
],
[
"Yanny",
"B.",
""
],
[
"Newberg",
"H.",
""
],
[
"Wilhelm",
"R.",
""
],
[
"Kang",
"X.",
""
],
[
"Smith",
"M. C.",
""
],
[
"Schneider",
"D. P.",
""
]
] | [
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801.1233 | Reiji Tomatsu | Reiji Tomatsu | A Galois correspondence for compact quantum group actions | 18 pages | null | null | null | math.OA | null | We establish a Galois correspondence for a minimal action of a compact
quantum group ${\mathbb G}$ on a von Neumann factor $M$. This extends the
result of Izumi, Longo and Popa who treated the case of a Kac algebra. Namely,
there exists a one-to-one correspondence between the lattice of left coideals
of ${\mathbb G}$ and that of intermediate subfactors of $M^{\mathbb G}\subset
M$.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 13:55:37 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Tomatsu",
"Reiji",
""
]
] | [
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] |
801.1234 | Dr. Paul J. Werbos | Paul J. Werbos | Bell's Theorem, Many Worlds and Backwards-Time Physics: Not Just a
Matter of Interpretation | 15 pages, 29 refs, 2 figures, 11 equations. Revision adds brief
appendix on opto-electronic circuit design issues to detect or exploit
backwards time effects | Intl J Theoretical Physics, e-pub date 2 April 2008 | 10.1007/s10773-008-9719-9 | ISSN 0020-7748 (print version) | physics.gen-ph | null | The classic "Bell's Theorem" of Clauser, Holt, Shimony and Horne tells us
that we must give up at least one of: (1) objective reality (aka "hidden
variables"); (2) locality; or (3) time-forwards macroscopic statistics (aka
"causality"). The orthodox Copenhagen version of physics gives up the first.
The many-worlds theory of Everett and Wheeler gives up the second. The
backwards-time theory of physics (BTP) gives up the third. Contrary to
conventional wisdom, empirical evidence strongly favors Everett-Wheeler over
orthodox Copenhagen. BTP has two major variations -- a many-worlds version, and
a neoclassical version of partial differential equations (PDE) in the spirit of
Einstein. Section 2 discusses quantum measurement according to BTP, focusing on
how we represent condensed matter objects like polarizers in a Bell's Theorem
experiment or in tests of Hawking's cosmology. The Backwards Time Telegraph,
though speculative, is discussed.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:02:49 GMT"
},
{
"version": "v2",
"created": "Tue, 25 Mar 2008 14:03:20 GMT"
}
] | 2008-04-21T00:00:00 | [
[
"Werbos",
"Paul J.",
""
]
] | [
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] |
801.1235 | Jan Timmermans | The DELPHI Collaboration, J. Abdallah, et al | Study of W boson polarisations and Triple Gauge boson Couplings in the
reaction e+e- -> W+W- at LEP 2 | 34 pages, 17 figures, Accepted by Eur. Phys. J. C | Eur.Phys.J.C54:345-364,2008 | 10.1140/epjc/s10052-008-0528-3 | CERN-PH-EP/2007-036 | hep-ex | null | A determination of the single W Spin Density Matrix (SDM) elements in the
reaction e+e- -> W+W- -> l nu q qbar (l=e/mu) is reported at centre-of-mass
energies between 189 and 209 GeV. The data sample used corresponds to an
integrated luminosity of 520 pb^{-1} taken by DELPHI between 1998 and 2000. The
single W SDM elements, rho_{tau tau'}^{W+-} (tau,tau' = +/-1 or 0), are
determined as a function of the W- production angle with respect to the e- beam
direction and are obtained from measurements of the W decay products by the
application of suitable projection operators, Lambda_{tau tau'}, which assume
the V-A coupling of the W boson to fermions. The measured SDM elements are used
to obtain the fraction of longitudinally polarised Ws, with the result:
sigma_L/sigma_tot = 24.9 +/- 4.5(stat) +/- 2.2(syst) % at a mean energy of 198
GeV. The SDM elements are also used to determine the Triple Gauge Couplings
Delta g_1^Z, Delta kappa_gamma, lambda_gamma and g_4^Z, kappa_Z and lambda_Z.
For the CP-violating couplings the results of single parameter fits are: g_4^Z
= -0.39 +0.19 -0.20 kappa_Z = -0.09 +0.08 -0.05 lambda_Z = -0.08 +/- 0.07 . The
errors are a combination of statistical and systematic errors. All results are
consistent with the Standard Model.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:05:55 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"The DELPHI Collaboration",
"",
""
],
[
"Abdallah",
"J.",
""
]
] | [
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801.1236 | Claudia M. Raiteri | C.M. Raiteri, M. Villata, V.M. Larionov, M.F. Aller, U. Bach, et al | Radio-to-UV monitoring of AO 0235+164 by the WEBT and Swift during the
2006--2007 outburst | 9 pages, 7 figures, in press for Astronomy and Astrophysics | null | 10.1051/0004-6361:20079044 | null | astro-ph | null | The blazar AO 0235+164 was claimed to show a quasi-periodic behaviour in the
radio and optical bands. Moreover, an extra emission component contributing to
the UV and soft X-ray flux was detected, whose nature is not yet clear. A
predicted optical outburst was observed in late 2006/early 2007. We here
present the radio-to-optical WEBT light curves during the outburst, together
with UV data acquired by Swift in the same period. We found the optical
outburst to be as strong as the big outbursts of the past: starting from late
September 2006, a brightness increase of 5 mag led to the outburst peak in
February 19-21, 2007. We also observed an outburst at mm and then at cm
wavelengths, with an increasing time delay going toward lower frequencies
during the rising phase. Cross-correlation analysis indicates that the 1 mm and
37 GHz flux variations lagged behind the R-band ones by about 3 weeks and 2
months, respectively. These short time delays suggest that the corresponding
jet emitting regions are only slightly separated and/or misaligned. In
contrast, during the outburst decreasing phase the flux faded contemporaneously
at all cm wavelengths. This abrupt change in the emission behaviour may suggest
the presence of some shutdown mechanism of intrinsic or geometric nature. The
behaviour of the UV flux closely follows the optical and near-IR one. By
separating the synchrotron and extra component contributions to the UV flux, we
found that they correlate, which suggests that the two emissions have a common
origin.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:10:27 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Raiteri",
"C. M.",
""
],
[
"Villata",
"M.",
""
],
[
"Larionov",
"V. M.",
""
],
[
"Aller",
"M. F.",
""
],
[
"Bach",
"U.",
""
]
] | [
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] |
801.1237 | Aude Alapini | Aude Alapini (1), Suzanne Aigrain (1) ((1) University of Exeter) | Reconstruction of the transit signal in the presence of stellar
variability | 4 pages, 2 figures. Accepted for publication in the Proceedings of
IAU Symposium 249: Exoplanet: Detection, Formation and Dynamics | null | null | null | astro-ph | null | Intrinsic stellar variability can hinder the detection of shallow transits,
particularly in space-based data. Therefore, this variability has to be
filtered out before running the transit search. Unfortunately, filtering out
the low frequency signal of the stellar variability also modifies the transit
shape. This results in errors in the measured transit depth and duration used
to derive the planet radius, and orbital inclination. We present an evaluation
of the magnitude of this effect based on 20 simulated light curves from the
CoRoT blind exercise 2 (BT2). We then present an iterative filter which uses
the strictly periodic nature of the transits to separate them from other forms
of variability, so as to recover the original transit shape before deriving the
planet parameters. On average with this filter, we improve the estimation of
the transit depth and duration by 15% and 10% respectively.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:11:58 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Alapini",
"Aude",
"",
"University of Exeter"
],
[
"Aigrain",
"Suzanne",
"",
"University of Exeter"
]
] | [
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801.1238 | Mathieu Sti\'enon | Gregory Ginot, Mathieu Stienon | G-gerbes, principal 2-group bundles and characteristic classes | Presentation improved, 38 pages | J. Symplectic Geom. 13 (2015), no. 4, 1001-1047 | 10.4310/JSG.2015.v13.n4.a6 | null | math.AT hep-th math.CT math.DG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let $G$ be a Lie group and $G\to\Aut(G)$ be the canonical group homomorphism
induced by the adjoint action of a group on itself. We give an explicit
description of a 1-1 correspondence between Morita equivalence classes of, on
the one hand, principal 2-group $[G\to\Aut(G)]$-bundles over Lie groupoids and,
on the other hand, $G$-extensions of Lie groupoids (i.e.\ between principal
$[G\to\Aut(G)]$-bundles over differentiable stacks and $G$-gerbes over
differentiable stacks). This approach also allows us to identify $G$-bound
gerbes and $[Z(G)\to 1]$-group bundles over differentiable stacks, where $Z(G)$
is the center of $G$. We also introduce universal characteristic classes for
2-group bundles. For groupoid central $G$-extensions, we introduce
Dixmier--Douady classes that can be computed from connection-type data
generalizing the ones for bundle gerbes. We prove that these classes coincide
with universal characteristic classes. As a corollary, we obtain further that
Dixmier--Douady classes are integral.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:41:39 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Jan 2008 10:46:56 GMT"
},
{
"version": "v3",
"created": "Sun, 2 Nov 2014 06:05:23 GMT"
}
] | 2019-10-15T00:00:00 | [
[
"Ginot",
"Gregory",
""
],
[
"Stienon",
"Mathieu",
""
]
] | [
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] |
801.1239 | Alexander Kelmans | Alexander Kelmans | Packing 3-vertex paths in cubic 3-connected graphs | 24 pages and 11 figures | null | null | RUTCOR Research Report 23-2005, Rutgers University (2005) | math.CO | null | Let v(G) and p(G) be the number of vertices and the maximum number of
disjoint 3-vertex paths in G, respectively. We discuss the following old
Problem: Is the following claim (P) true ?
(P) if G is a 3-connected and cubic graph, then p(G) = [v(G)/3], where
[v(G)/3] is the floor of v(G)/3.
We show, in particular, that claim (P) is equivalent to some seemingly
stronger claims. It follows that if claim (P) is true, then Reed's dominating
graph conjecture (see [14]) is true for cubic 3-connected graphs.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 03:55:11 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Kelmans",
"Alexander",
""
]
] | [
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] |
801.124 | Bortolo Matteo Mognetti | Bortolo Matteo Mognetti, Leonid Yelash, Peter Virnau, Wolfgang Paul,
Kurt Binder, Marcus Mueller, Luis Gonzalez MacDowell | Efficient prediction of thermodynamic properties of quadrupolar fluids
from simulation of a coarse-grained model: The case of carbon dioxide | J. Chem. Phys. (2008), to appear | J. Chem. Phys. 128: 104501, 2008 | null | null | cond-mat.stat-mech | null | Monte Carlo simulations are presented for a coarse-grained model of real
quadrupolar fluids. Molecules are represented by particles interacting with
Lennard-Jones forces plus the thermally averaged quadrupole-quadrupole
interaction. The properties discussed include the vapor-liquid coexistence
curve, the vapor pressure along coexistence, and the surface tension. The full
isotherms are also accessible over a wide range of temperatures and densities.
It is shown that the critical parameters (critical temperature, density, and
pressure) depend almost linearly on a quadrupolar parameter $q=Q^{*4} /T^*$,
$Q^*$ is the reduced quadrupole moment of the molecule and $T^*$ the reduced
temperature.
The model can be applied to a variety of small quadrupolar molecules. We
focus on carbon dioxide as a test case, but consider nitrogen and benzene, too.
Experimental critical temperature, density and quadrupolar moment are
sufficient to fix the parameters of the model. The resulting agreement with
experiments is excellent and marks a significant improvement over approaches
which neglect quadrupolar effects. The same coarse-grained model was also
applied in the framework of Perturbation Theory (PT) in the Mean Spherical
Approximation (MSA). As expected, the latter deviates from the Monte Carlo
results in the critical region, but is reasonably accurate at lower
temperatures.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:43:05 GMT"
}
] | 2008-03-10T00:00:00 | [
[
"Mognetti",
"Bortolo Matteo",
""
],
[
"Yelash",
"Leonid",
""
],
[
"Virnau",
"Peter",
""
],
[
"Paul",
"Wolfgang",
""
],
[
"Binder",
"Kurt",
""
],
[
"Mueller",
"Marcus",
""
],
[
"MacDowell",
"Luis Gonzalez",
""
]
] | [
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] |
801.1241 | David Poulin | David Poulin and Yeojin Chung | On the iterative decoding of sparse quantum codes | To appear in QIC | QIC Vol.8 No.10 p.987 (2008) | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We address the problem of decoding sparse quantum error correction codes. For
Pauli channels, this task can be accomplished by a version of the belief
propagation algorithm used for decoding sparse classical codes. Quantum codes
pose two new challenges however. Firstly, their Tanner graph unavoidably
contain small loops which typically undermines the performance of belief
propagation. Secondly, sparse quantum codes are by definition highly
degenerate. The standard belief propagation algorithm does not exploit this
feature, but rather it is impaired by it. We propose heuristic methods to
improve belief propagation decoding, specifically targeted at these two
problems. While our results exhibit a clear improvement due to the proposed
heuristic methods, they also indicate that the main source of errors in the
quantum coding scheme remains in the decoding.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:25:30 GMT"
},
{
"version": "v2",
"created": "Tue, 1 Jul 2008 15:09:21 GMT"
}
] | 2008-09-16T00:00:00 | [
[
"Poulin",
"David",
""
],
[
"Chung",
"Yeojin",
""
]
] | [
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] |
801.1242 | Alexander B. Shick | Alexander B. Shick (1), and Alexander I. Lichtenstein (2),
((1)Institute of Physics ASCR, Prague, Czech Republic, (2)University of
Hamburg, Germany) | Orbital moment of a single Co atom on a Pt(111) surface - a view from
correlated band theory | null | J. Phys.: Cond. Matter. 20 (2008) 015002 | 10.1088/0953-8984/20/01/015002 | null | cond-mat.mtrl-sci cond-mat.str-el | null | The orbital magnetic moment of a Co adatom on a Pt(111) surface is calculated
in good agreement with experimental data making use of the LSDA+U method. It is
shown that both electron correlation induced orbital polarization and
structural relaxation play essential roles in orbital moment formation. The
microscopic origins of the orbital moment enhancement are discussed.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:31:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Shick",
"Alexander B.",
""
],
[
"Lichtenstein",
"Alexander I.",
""
]
] | [
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] |
801.1243 | Dietrich Stauffer | Andrzej Gecow | Structural tendencies - Effects of adaptive evolution of complex
(chaotic) systems | 20 pages with fugures, to be published in Int. J. Mod. Phys. C | null | 10.1142/S0129183108012418 | null | cond-mat.dis-nn | null | We describe systems using Kauffman and similar networks. They are directed
funct ioning networks consisting of finite number of nodes with finite number
of discr ete states evaluated in synchronous mode of discrete time. In this
paper we introduce the notion and phenomenon of `structural tendencies'.
Along the way we expand Kauffman networks, which were a synonym of Boolean
netw orks, to more than two signal variants and we find a phenomenon during
network g rowth which we interpret as `complexity threshold'. For simulation we
define a simplified algorithm which allows us to omit the problem of periodic
attractors. We estimate that living and human designed systems are chaotic (in
Kauffman sens e) which can be named - complex. Such systems grow in adaptive
evolution. These two simple assumptions lead to certain statistical effects
i.e. structural tendencies observed in classic biology but still not explained
and not investigated on theoretical way. E.g. terminal modifications or
terminal predominance of additions where terminal means: near system outputs.
We introduce more than two equally probable variants of signal, therefore our
networks generally are not Boolean networks. T hey grow randomly by additions
and removals of nodes imposed on Darwinian elimination. Fitness is defined on
external outputs of system. During growth of the system we observe a phase
transition to chaos (threshold of complexity) in damage spreading. Above this
threshold we identify mechanisms of structural tendencies which we investigate
in simulation for a few different networks types, including scale-free BA
networks.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:31:46 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gecow",
"Andrzej",
""
]
] | [
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] |
801.1244 | Christian Gollwitzer | Christian Gollwitzer, Alexander Turanov, Marina Krekhova, G\"unter
Lattermann, Ingo Rehberg, Reinhard Richter | Measuring the deformation of a ferrogel sphere in a homogeneous magnetic
field | 5 pages, 8 figures | null | 10.1063/1.2905212 | null | cond-mat.soft | null | A sphere of a ferrogel is exposed to a homogeneous magnetic field. In
accordance to theoretical predictions, it gets elongated along the field lines.
The time-dependence of the elastic shear modulus causes the elongation to
increase with time analogously to mechanic creep experiments, and the rapid
excitation causes the sphere to vibrate. Both phenomena can be well described
by a damped harmonic oscillator model. By comparing the elongation along the
field with the contraction perpendicular to it, we can calculate Poisson's
ratio of the gel. The magnitude of the elongation is compared with the
theoretical predictions for elastic spheres in homogeneous fields.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:33:24 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gollwitzer",
"Christian",
""
],
[
"Turanov",
"Alexander",
""
],
[
"Krekhova",
"Marina",
""
],
[
"Lattermann",
"Günter",
""
],
[
"Rehberg",
"Ingo",
""
],
[
"Richter",
"Reinhard",
""
]
] | [
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] |
801.1245 | Pedro Pablo P\'erez Velasco | Pedro Pablo Perez Velasco | Matrix Graph Grammars | 321 pages, 75 figures. This book has is publisehd by VDM verlag, ISBN
978-3639212556 | null | null | null | cs.DM | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This book objective is to develop an algebraization of graph grammars.
Equivalently, we study graph dynamics. From the point of view of a computer
scientist, graph grammars are a natural generalization of Chomsky grammars for
which a purely algebraic approach does not exist up to now. A Chomsky (or
string) grammar is, roughly speaking, a precise description of a formal
language (which in essence is a set of strings). On a more discrete
mathematical style, it can be said that graph grammars -- Matrix Graph Grammars
in particular -- study dynamics of graphs. Ideally, this algebraization would
enforce our understanding of grammars in general, providing new analysis
techniques and generalizations of concepts, problems and results known so far.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 06:04:37 GMT"
},
{
"version": "v2",
"created": "Tue, 17 Nov 2009 20:52:12 GMT"
}
] | 2009-11-17T00:00:00 | [
[
"Velasco",
"Pedro Pablo Perez",
""
]
] | [
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] |
801.1246 | Giovanni Calvaruso | Giovanni Calvaruso and Rosa Anna Marinosci | Homogeneous geodesics of non-unimodular Lorentzian Lie groups and
naturally reductive Lorentzian spaces in dimension three | null | null | null | null | math.DG | null | We determine, for all three-dimensional non-unimodular Lie groups equipped
with a Lorentzian metric, the set of homogeneous geodesics through a point.
Together with the results of [C] and [CM2], this leads to the full
classification of three-dimensional Lorentzian g.o. spaces and naturally
reductive spaces.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:44:08 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Calvaruso",
"Giovanni",
""
],
[
"Marinosci",
"Rosa Anna",
""
]
] | [
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] |
801.1247 | Vahid Karimipour | S. Alipour, S. Baghbanzadeh and V. Karimipour | Exact symmetry breaking ground states for quantum spin chains | 4 pages, RevTex. 4 figures, minor changes, new references | Europhysics Letters (EPL), 84 (2008) 67006. | 10.1209/0295-5075/84/67006 | null | cond-mat.str-el math-ph math.MP quant-ph | null | We introduce a family of spin-1/2 quantum chains, and show that their exact
ground states break the rotational and translational symmetries of the original
Hamiltonian. We also show how one can use projection to construct a spin-3/2
quantum chain with nearest neighbor interaction, whose exact ground states
break the rotational symmetry of the Hamiltonian. Correlation functions of both
models are determined in closed form. Although we confine ourselves to
examples, the method can easily be adapted to encompass more general models.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 20:43:28 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jan 2008 18:21:43 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Alipour",
"S.",
""
],
[
"Baghbanzadeh",
"S.",
""
],
[
"Karimipour",
"V.",
""
]
] | [
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] |
801.1248 | Peter Hamlington | Peter E. Hamlington, J\"org Schumacher, Werner J.A. Dahm | Local and Nonlocal Strain Rate Fields and Vorticity Alignment in
Turbulent Flows | 9 pages, to appear in Physical Review E | Physical Review E 77, 026303 (2008) | 10.1103/PhysRevE.77.026303 | null | physics.flu-dyn | null | Local and nonlocal contributions to the total strain rate tensor at any point
in a flow are formulated from an expansion of the vorticity field in a local
spherical neighborhood of radius R centered on x. The resulting exact
expression allows the nonlocal (background) strain rate tensor to be obtained
from the total strain rate tensor. In turbulent flows, where the vorticity
naturally concentrates into relatively compact structures, this allows the
local alignment of vorticity with the most extensional principal axis of the
background strain rate tensor to be evaluated. In the vicinity of any vortical
structure, the required radius R and corresponding order n to which the
expansion must be carried are determined by the viscous lengthscale. We
demonstrate the convergence to the background strain rate field with increasing
R and n for an equilibrium Burgers vortex, and show that this resolves the
anomalous alignment of vorticity with the intermediate eigenvector of the total
strain rate tensor. We then evaluate the background strain field in DNS of
homogeneous isotropic turbulence where, even for the limited R and n
corresponding to the truncated series expansion, the results show an increase
in the expected equilibrium alignment of vorticity with the most extensional
principal axis of the background strain rate tensor.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:45:18 GMT"
}
] | 2008-02-18T00:00:00 | [
[
"Hamlington",
"Peter E.",
""
],
[
"Schumacher",
"Jörg",
""
],
[
"Dahm",
"Werner J. A.",
""
]
] | [
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] |
801.1249 | Wenxu Xu | Wenxu Xu, Minghong Liao | Quantum algorithm for the longest common subsequence problem | This paper has been withdrawn | null | null | null | quant-ph | null | This paper has been withdrawn by the author(s), due a crucial error on the
entanglement of $\Gamma$ registers.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 14:55:53 GMT"
},
{
"version": "v2",
"created": "Sat, 19 Jan 2008 03:12:22 GMT"
}
] | 2008-01-19T00:00:00 | [
[
"Xu",
"Wenxu",
""
],
[
"Liao",
"Minghong",
""
]
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801.125 | Manfred Sch\"ussler | M Schuessler and A. Voegler | Strong horizontal photospheric magnetic field in a surface dynamo
simulation | Astronomy & Astrophysics, in press | null | 10.1051/0004-6361:20078998 | null | astro-ph | null | Observations with the Hinode spectro-polarimeter have revealed strong
horizontal internetwork magnetic fields in the quiet solar photosphere. We aim
at interpreting the observations by means of results from numerical
simulations. Radiative MHD simulations of dynamo action by near-surface
convection are analyzed with respect to the relation between vertical and
horizontal magnetic field components. The dynamo-generated fields show a clear
dominance of the horizontal field in the height range where the spectral lines
used for the observations are formed. The ratio between the averaged horizontal
and vertical field components is consistent with the values derived from the
observations. This behavior results from the intermittent nature of the dynamo
field with polarity mixing on small scales in the surface layers. Our results
provide further evidence that local near-surface dynamo action contributes
significantly to the solar internetwork fields.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:11:17 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Schuessler",
"M",
""
],
[
"Voegler",
"A.",
""
]
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] |
801.1251 | Andrew Pitts | Andrew M. Pitts and Mark R. Shinwell | Generative Unbinding of Names | null | Logical Methods in Computer Science, Volume 4, Issue 1 (March 18,
2008) lmcs:916 | 10.2168/LMCS-4(1:4)2008 | null | cs.PL cs.LO | null | This paper is concerned with the form of typed name binding used by the
FreshML family of languages. Its characteristic feature is that a name binding
is represented by an abstract (name,value)-pair that may only be deconstructed
via the generation of fresh bound names. The paper proves a new result about
what operations on names can co-exist with this construct. In FreshML the only
observation one can make of names is to test whether or not they are equal.
This restricted amount of observation was thought necessary to ensure that
there is no observable difference between alpha-equivalent name binders. Yet
from an algorithmic point of view it would be desirable to allow other
operations and relations on names, such as a total ordering. This paper shows
that, contrary to expectations, one may add not just ordering, but almost any
relation or numerical function on names without disturbing the fundamental
correctness result about this form of typed name binding (that object-level
alpha-equivalence precisely corresponds to contextual equivalence at the
programming meta-level), so long as one takes the state of dynamically created
names into account.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:04:56 GMT"
},
{
"version": "v2",
"created": "Tue, 18 Mar 2008 18:23:41 GMT"
}
] | 2015-07-01T00:00:00 | [
[
"Pitts",
"Andrew M.",
""
],
[
"Shinwell",
"Mark R.",
""
]
] | [
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] |
801.1252 | Jean Cleymans | B. Becker, S. Chattopadhyay, C. Cicalo J. Cleymans, G. de Vaux, R.W.
Fearick, V. Lindenstruth, M. Richter, D. Rorich, F. Staley, T.M. Steinbeck,
A. Szostak, H. Tilsner, R. Weis and Z.Z. Vilakazi | Real Time Global Tests of the ALICE High Level Trigger Data Transport
Framework | 8 pages 4 figures | IEEE Trans.Nucl.Sci.55:703-709,2008 | 10.1109/TNS.2008.918521 | null | physics.ins-det | null | The High Level Trigger (HLT) system of the ALICE experiment is an online
event filter and trigger system designed for input bandwidths of up to 25 GB/s
at event rates of up to 1 kHz. The system is designed as a scalable PC cluster,
implementing several hundred nodes. The transport of data in the system is
handled by an object-oriented data flow framework operating on the basis of the
publisher-subscriber principle, being designed fully pipelined with lowest
processing overhead and communication latency in the cluster. In this paper, we
report the latest measurements where this framework has been operated on five
different sites over a global north-south link extending more than 10,000 km,
processing a ``real-time'' data flow.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:06:13 GMT"
}
] | 2011-04-11T00:00:00 | [
[
"Becker",
"B.",
""
],
[
"Chattopadhyay",
"S.",
""
],
[
"Cleymans",
"C. Cicalo J.",
""
],
[
"de Vaux",
"G.",
""
],
[
"Fearick",
"R. W.",
""
],
[
"Lindenstruth",
"V.",
""
],
[
"Richter",
"M.",
""
],
[
"Rorich",
"D.",
""
],
[
"Staley",
"F.",
""
],
[
"Steinbeck",
"T. M.",
""
],
[
"Szostak",
"A.",
""
],
[
"Tilsner",
"H.",
""
],
[
"Weis",
"R.",
""
],
[
"Vilakazi",
"Z. Z.",
""
]
] | [
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] |
801.1253 | Damiano Mazza | Patrick Baillot and Damiano Mazza | Linear Logic by Levels and Bounded Time Complexity | 63 pages. To appear in Theoretical Computer Science. This version
corrects minor fonts problems from v2 | Theoretical Computer Science 411 (2010) 470-503 | 10.1016/j.tcs.2009.09.015 | null | cs.LO cs.CC | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We give a new characterization of elementary and deterministic polynomial
time computation in linear logic through the proofs-as-programs correspondence.
Girard's seminal results, concerning elementary and light linear logic, achieve
this characterization by enforcing a stratification principle on proofs, using
the notion of depth in proof nets. Here, we propose a more general form of
stratification, based on inducing levels in proof nets by means of indexes,
which allows us to extend Girard's systems while keeping the same complexity
properties. In particular, it turns out that Girard's systems can be recovered
by forcing depth and level to coincide. A consequence of the higher flexibility
of levels with respect to depth is the absence of boxes for handling the
paragraph modality. We use this fact to propose a variant of our polytime
system in which the paragraph modality is only allowed on atoms, and which may
thus serve as a basis for developing lambda-calculus type assignment systems
with more efficient typing algorithms than existing ones.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:08:20 GMT"
},
{
"version": "v2",
"created": "Mon, 20 Jul 2009 19:00:04 GMT"
},
{
"version": "v3",
"created": "Sun, 26 Jul 2009 13:07:48 GMT"
}
] | 2012-07-17T00:00:00 | [
[
"Baillot",
"Patrick",
""
],
[
"Mazza",
"Damiano",
""
]
] | [
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] |
801.1254 | Pieter Van Isacker | P. Van Isacker (GANIL), S. Heinze | Partial conservation of seniority and nuclear isomerism | Accepted for publication in Physical Review Letters | Phys.Rev.Lett.100:052501,2008 | 10.1103/PhysRevLett.100.052501 | null | nucl-th | null | We point out the possibility of the {\em partial} conservation of the
seniority quantum number when most eigenstates are mixed in seniority but some
remain pure. This situation occurs in nuclei for the $g_{9/2}$ and $h_{9/2}$
shells where it is at the origin of the existence of seniority isomers in the
ruthenium and palladium isotopes. It also occurs for $f$ bosons.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:13:16 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Van Isacker",
"P.",
"",
"GANIL"
],
[
"Heinze",
"S.",
""
]
] | [
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] |
801.1255 | Alexandre Krassilchtchikov | A. M. Bykov, A. M. Krassilchtchikov, Yu. A. Uvarov (Ioffe Inst.,
St.Petersburg), H. Bloemen (SRON, Utrecht), F. Bocchino (INAF, Palermo), G.
M. Dubner, E. B. Giacani (IAFE, Buenos Aires), G. G. Pavlov (Penn. State
Univ.) | Isolated X-ray -- infrared sources in the region of interaction of the
supernova remnant IC 443 with a molecular cloud | The Astrophysical Journal, v. 677 (April 2008), in press | The Astrophysical Journal, v. 676, p. 1050-1063, 2008 | 10.1086/529117 | null | astro-ph | null | The nature of the extended hard X-ray source XMMU J061804.3+222732 and its
surroundings is investigated using XMM-Newton, Chandra, and Spitzer
observations. This source is located in an interaction region of the IC 443
supernova remnant with a neighboring molecular cloud. The X-ray emission
consists of a number of bright clumps embedded in an extended structured
non-thermal X-ray nebula larger than 30" in size. Some clumps show evidence for
line emission at ~1.9 keV and ~3.7 keV at the 99% confidence level. Large-scale
diffuse radio emission of IC 443 passes over the source region, with an
enhancement near the source. An IR source of about 14" x 7" size is prominent
in the 24 um, 70 um, and 2.2 um bands, adjacent to a putative Si K-shell X-ray
line emission region. The observed IR/X-ray morphology and spectra are
consistent with those expected for J/C-type shocks of different velocities
driven by fragmented supernova ejecta colliding with the dense medium of a
molecular cloud. The IR emission of the source detected by Spitzer can be
attributed to both continuum emission from an HII region created by the ejecta
fragment and line emission excited by shocks. This source region in IC 443 may
be an example of a rather numerous population of hard X-ray/IR sources created
by supernova explosions in the dense environment of star-forming regions.
Alternative Galactic and extragalactic interpretations of the observed source
are also discussed.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:30:46 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bykov",
"A. M.",
"",
"Ioffe Inst.,\n St.Petersburg"
],
[
"Krassilchtchikov",
"A. M.",
"",
"Ioffe Inst.,\n St.Petersburg"
],
[
"Uvarov",
"Yu. A.",
"",
"Ioffe Inst.,\n St.Petersburg"
],
[
"Bloemen",
"H.",
"",
"SRON, Utrecht"
],
[
"Bocchino",
"F.",
"",
"INAF, Palermo"
],
[
"Dubner",
"G. M.",
"",
"IAFE, Buenos Aires"
],
[
"Giacani",
"E. B.",
"",
"IAFE, Buenos Aires"
],
[
"Pavlov",
"G. G.",
"",
"Penn. State\n Univ."
]
] | [
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] |
801.1256 | Tadafumi Ohsaku | Tadafumi Ohsaku | Dynamical Dirac Mass Generation in the Supersymmetric
Nambu--Jona-Lasinio Model with the Seesaw Mechanism of Neutrinos | 8 pages, 10 figures, submitted for publication | null | null | null | hep-ph cond-mat.mes-hall cond-mat.str-el cond-mat.supr-con gr-qc hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The dynamical generation of Dirac mass in the supersymmetric
Nambu$-$Jona-Lasinio (SNJL) model with the seesaw mechanism of neutrino is
investigeted. The right and left handed Majorana mass parameters are introduced
into the SNJL model; we regard them as external model parameters. The question
on the origin of these Majorana masses are set aside, and we concentrate on the
examination of the effect of the Majorana mass parameters on the dynamical
generation of Dirac mass. The effective potential of the model and the gap
equation for the self-consistent determination of Dirac mass are derived and
solved. We use both the four-dimensional covariant and three-dimensional
non-covariant cutoff schemes for the regularizations of the effective
potential. We find there are cases of the first and second order phase
transitions with respect to variation of the coupling constant of the
Nambu$-$Jona-Lasinio-type four-body interaction of the SNJL model. In the case
of second-order phase transition, the dynamically generated Dirac mass
$|\phi_{S}|$ can arbitrarily be small compared with the right-handed Majorana
mass parameter $|M|$ and thus the seesaw condition $0<|\phi_{S}|\ll|M|$ can be
satisfied by a fine tuning of the coupling constant, while at the first-order
case it seems very difficult and/or "unnatural" to satisfy the condition. The
numerical results do not depend on the difference of the cutoff schemes
qualitatively.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:29:45 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Jan 2008 22:08:41 GMT"
},
{
"version": "v3",
"created": "Sun, 27 Jan 2008 15:41:20 GMT"
},
{
"version": "v4",
"created": "Mon, 28 Apr 2008 10:34:00 GMT"
},
{
"version": "v5",
"created": "Thu, 9 Oct 2008 19:04:59 GMT"
}
] | 2016-09-08T00:00:00 | [
[
"Ohsaku",
"Tadafumi",
""
]
] | [
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] |
801.1257 | Tomaz Prosen | Tomaz Prosen | Third quantization: a general method to solve master equations for
quadratic open Fermi systems | 24 pages, with 8 eps figures - few minor corrections to the published
version, e.g. anti-symmetrizing the matrix given by eq. (27) | New J. Phys. 10, 043026 (2008) | 10.1088/1367-2630/10/4/043026 | null | quant-ph cond-mat.stat-mech nlin.SI | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Lindblad master equation for an arbitrary quadratic system of n fermions
is solved explicitly in terms of diagonalization of a 4n x 4n matrix, provided
that all Lindblad bath operators are linear in the fermionic variables. The
method is applied to the explicit construction of non-equilibrium steady states
and the calculation of asymptotic relaxation rates in the far from equilibrium
problem of heat and spin transport in a nearest neighbor Heisenberg XY spin 1/2
chain in a transverse magnetic field.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:54:37 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Apr 2008 09:16:36 GMT"
},
{
"version": "v3",
"created": "Thu, 4 Dec 2008 22:10:08 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Prosen",
"Tomaz",
""
]
] | [
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] |
801.1258 | Giovanni Carraro dr | Gabriela Parisi (IAR-LaPlata), Giovanni Carraro (ESO-Santiago),
Michele Maris (OATS), Adrian Brunini (LaPlata) | Constraints to Uranus' Great Collision. IV. The Origin of Prospero | 11 pages, 1 eps figure, accepted for publication in A&A. Abstract
rephrased to fit in; V2: some problem in the latex of V1 fixed | null | null | null | astro-ph | null | It is widely accepted that the large obliquity of Uranus is the result of a
great tangential collision (GC) with an Earth size proto-planet at the end of
the accretion. We attempt to constraint the GC scenario as the cause of Uranus'
obliquity as well as on the mechanisms able to give origin to the Uranian
irregulars. Different capture mechanisms for irregulars operate at different
stages on the giant planets formation process. The mechanisms able to capture
the uranian irregulars before and after the GC are analysed. Assuming that they
were captured before the GC, we calculate the orbital transfer of the nine
irregulars by the impulse imparted by the GC. If their orbital transfer results
dynamically implausible, they should have originated after the GC. We
investigate and discuss the dissipative mechanisms able to operate later. In
particular Prospero could not exist at the time of the GC. Different capture
mechanisms for Prospero after the GC are investigated. Gas drag by
Uranus'envelope and pull-down capture are not plausible mechanisms. Capture of
Prospero through a collisionless interaction seems to be difficult. The GC
itself provides a mechanism of permanent capture. However, the capture of
Prospero by the GC is a low probable event. Catastrophic collisions could be a
possible mechanism for the birth of Prospero and the other irregulars after the
GC. Orbital and physical clusterings should then be expected. Either Prospero
had to originate after the GC or the GC did not occur. In the former case, the
mechanism for the origin of Prospero after the GC remains an open question. In
the latter case, another theory to account for Uranus' obliquity and the
formation of the Uranian regular satellites on the equatorial plane of the
planet would be needed.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:46:28 GMT"
},
{
"version": "v2",
"created": "Thu, 10 Jan 2008 11:28:57 GMT"
}
] | 2008-01-10T00:00:00 | [
[
"Parisi",
"Gabriela",
"",
"IAR-LaPlata"
],
[
"Carraro",
"Giovanni",
"",
"ESO-Santiago"
],
[
"Maris",
"Michele",
"",
"OATS"
],
[
"Brunini",
"Adrian",
"",
"LaPlata"
]
] | [
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] |
801.1259 | Alok Gupta Dr. | Alok C. Gupta (1), B. S. Acharya (2), Debanjan Bose (2), Varsha R.
Chitnis (2) and Jun-Hui Fan (1) ((1) Center for Astrophysics, Guangzhou
University, Guangzhou, China (2) Tata Institute of Fundamental Research, Homi
Bhabha Road, Colaba, Mumbai, India) | Simultaneous multi-wavelength observations of the TeV Blazar Mrk 421
during February - March 2003: X-ray and NIR correlated variability | 11 pages, 5 figures, Accepted for Publication in ChJAA | 2008, ChJAA, 8, 395-403 | 10.1088/1009-9271/8/4/03 | null | astro-ph | null | In the present paper, we have reported the result of simultaneous
multi-wavelength observations of the TeV blazar Mrk 421 during February $-$
March 2003. In this period, we have observed Mrk 421 using Pachmarhi Array of
\v{C}erenkov Telescopes (PACT) of Tata Institute of Fundamental Research at
Pachmarhi, India. Other simultaneous data were taken from the published
literature and public data archives. We have analyzed the high quality X-ray
(2-20 keV) observations from the NASA Rossi X-Ray Timing Explorer (RXTE). We
have seen a possible correlated variability between X-ray and J band (1.25
$\mu$) near infrared (NIR) wavelength. This is the first case of X-ray and NIR
correlated variability in Mrk 421 or any high energy peaked (HBL) blazar. The
correlated variability reported here is indicating a similar origin for NIR and
X-ray emission. The emission is not affected much by the environment of the
surrounding medium around the central engine of the Mrk 421. The observations
are consistent with the shock-in-jet model for the emission of radiations.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:47:00 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gupta",
"Alok C.",
""
],
[
"Acharya",
"B. S.",
""
],
[
"Bose",
"Debanjan",
""
],
[
"Chitnis",
"Varsha R.",
""
],
[
"Fan",
"Jun-Hui",
""
]
] | [
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801.126 | Malwina J. Luczak | Malwina J. Luczak, Colin McDiarmid | Balanced routing of random calls | Published at http://dx.doi.org/10.1214/14-AAP1023 in the Annals of
Applied Probability (http://www.imstat.org/aap/) by the Institute of
Mathematical Statistics (http://www.imstat.org) | Annals of Applied Probability 2015, Vol. 25, No. 3, 1279-1324 | 10.1214/14-AAP1023 | IMS-AAP-AAP1023 | math.PR math.CO | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider an online network routing problem in continuous time, where calls
have Poisson arrivals and exponential durations. The first-fit dynamic
alternative routing algorithm sequentially selects up to $d$ random two-link
routes between the two endpoints of a call, via an intermediate node, and
assigns the call to the first route with spare capacity on each link, if there
is such a route. The balanced dynamic alternative routing algorithm
simultaneously selects $d$ random two-link routes, and the call is accepted on
a route minimising the maximum of the loads on its two links, provided neither
of these two links is saturated. We determine the capacities needed for these
algorithms to route calls successfully and find that the balanced algorithm
requires a much smaller capacity. In order to handle such interacting random
processes on networks, we develop appropriate tools such as lemmas on biased
random walks.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 20:51:25 GMT"
},
{
"version": "v2",
"created": "Thu, 31 Mar 2011 09:11:05 GMT"
},
{
"version": "v3",
"created": "Mon, 29 Jun 2015 06:10:48 GMT"
}
] | 2015-06-30T00:00:00 | [
[
"Luczak",
"Malwina J.",
""
],
[
"McDiarmid",
"Colin",
""
]
] | [
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] |
801.1261 | Pedro Jesus Salas | Pedro J. Salas | Noise effect on Grover algorithm | Accepted to be published in Eur. Phys. J. D (2008) | null | 10.1140/epjd/e2007-00295-1 | null | quant-ph | null | The decoherence effect on Grover algorithm has been studied numerically
through a noise modelled by a depolarizing channel. Two types of error are
introduced characterizing the qubit time evolution and gate application, so the
noise is directly related to the quantum network construction. The numerical
simulation concludes an exponential damping law for the successive probability
of the maxima as time increases. We have obtained an allowed-error law for the
algorithm: the error threshold for the allowed noise behaves as Eth(N) ~ 1/N1.1
(N being the size of the data set). As the power of N is almost one, we
consider the Grover algorithm as robust to a certain extent against
decoherence. This law also provides an absolute threshold: if the free
evolution error is greater than 0.043, Grover algorithm does not work for any
number of qubits affected by the present error model. The improvement in the
probability of success, in the case of two qubits has been illustrated by using
a fault-tolerant encoding of the initial state by means of the [[7,1,3]]
quantum code.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:52:00 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Salas",
"Pedro J.",
""
]
] | [
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] |
801.1262 | Gianluca Cassese | Gianluca Cassese | Finitely Additive Supermartingales | null | null | null | null | math.PR | null | The concept of finitely additive supermartingales, originally due to Bochner,
is revived and developed. We exploit it to study measure decompositions over
filtered probability spaces and the properties of the associated
Dol\'{e}ans-Dade measure. We obtain versions of the Doob Meyer decomposition
and, as an application, we establish a version of the Bichteler and Dellacherie
theorem with no exogenous probability measure.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:52:13 GMT"
},
{
"version": "v2",
"created": "Mon, 21 Apr 2008 10:53:55 GMT"
}
] | 2008-04-21T00:00:00 | [
[
"Cassese",
"Gianluca",
""
]
] | [
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] |
801.1263 | Richard A. Mould | Richard A. Mould | Experimental Test | 5 pages, 1 figure | null | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | An experiment is described that empirically distinguishes the previously
proposed q-rules governing the collapse of a wave function, and contrasts it
with the conventional idea of a collapse as well as the current leading theory
of collapse advanced by Ghirardi and Pearle. Keywords: foundation theory,
measurement, qRules, state reduction, wave collapse.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:54:37 GMT"
},
{
"version": "v2",
"created": "Wed, 9 Jan 2008 17:16:40 GMT"
},
{
"version": "v3",
"created": "Wed, 10 Dec 2008 20:29:15 GMT"
},
{
"version": "v4",
"created": "Mon, 14 Nov 2011 15:32:06 GMT"
}
] | 2011-11-15T00:00:00 | [
[
"Mould",
"Richard A.",
""
]
] | [
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] |
801.1264 | Brian Punsly | Kajal K. Ghosh and Brian Punsly | The Discovery of Soft X-ray Loud Broad Absorption Line Quasars | To appear in ApJ Letters | null | 10.1086/529138 | null | astro-ph | null | It is been known for more than a decade that BALQSOs (broad absorption line
quasars) are highly attenuated in the X-ray regime compared to other quasars,
especially in the soft band ($< $ 1 keV). Using X-ray selection techniques we
have found "soft X-ray loud" BALQSOs that, by definition, have soft X-ray (0.3
keV) to UV ($3000 \AA$) flux density ratios that are higher than typical nonBAL
radio quiet quasars. Our sample of 3 sources includes one LoBALQSO (low
ionization BALQSO) which are generally considered to be the most highly
attenuated in the X-rays. The three QSOs are the only known BALQSOs that have
X-ray observations that are consistent with no intrinsic soft X-ray absorption.
The existence of a large X-ray luminosity and the hard ionizing continuum that
it presents to potential UV absorption gas is in conflict with the ionization
states that are conducive to line driving forces within BAL winds (especially
for the LoBALs).
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 15:57:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ghosh",
"Kajal K.",
""
],
[
"Punsly",
"Brian",
""
]
] | [
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] |
801.1265 | Gert De Cooman | Gert de Cooman, Erik Quaeghebeur, Enrique Miranda | Exchangeable lower previsions | 1 figure. 26 pages. Submitted for publication | null | null | null | math.PR math.ST stat.ME stat.TH | null | We extend de Finetti's (1937) notion of exchangeability to finite and
countable sequences of variables, when a subject's beliefs about them are
modelled using coherent lower previsions rather than (linear) previsions. We
prove representation theorems in both the finite and the countable case, in
terms of sampling without and with replacement, respectively. We also establish
a convergence result for sample means of exchangeable sequences. Finally, we
study and solve the problem of exchangeable natural extension: how to find the
most conservative (point-wise smallest) coherent and exchangeable lower
prevision that dominates a given lower prevision.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 16:13:29 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"de Cooman",
"Gert",
""
],
[
"Quaeghebeur",
"Erik",
""
],
[
"Miranda",
"Enrique",
""
]
] | [
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] |
801.1266 | Simone Paganelli | Simone Paganelli and Sergio Ciuchi | Charge transfer and coherence dynamics of tunnelling system coupled to a
harmonic oscillator | null | Journal of Physics: Condensed Matter 20, 235203 (2008) | 10.1088/0953-8984/20/23/235203 | null | cond-mat.other cond-mat.stat-mech | null | We study the transition probability and coherence of a two-site system,
interacting with an oscillator. Both properties depend on the initial
preparation. The oscillator is prepared in a thermal state and, even though it
cannot be considered as an extended bath, it produces decoherence because of
the large number of states involved in the dynamics. In the case in which the
oscillator is intially displaced a coherent dynamics of change entangled with
oscillator modes takes place. Coherency is however degraded as far as the
oscillator mass increases producing a increasingly large recoherence time.
Calculations are carried on by exact diagonalization and compared with two
semiclassical approximations. The role of the quantum effects are highlighted
in the long-time dynamics, where semiclassical approaches give rise to a
dissipative behaviour. Moreover, we find that the oscillator dynamics has to be
taken into account, even in a semiclassical approximation, in order to
reproduce a thermally activated enhancement of the transition probability.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 16:09:28 GMT"
},
{
"version": "v2",
"created": "Fri, 4 Apr 2008 10:11:12 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Paganelli",
"Simone",
""
],
[
"Ciuchi",
"Sergio",
""
]
] | [
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] |
801.1267 | Ernst Jan Vesseur | E. J. R. Vesseur, R. de Waele, A. Polman, H. J. Lezec, H. A. Atwater
and F. J. Garc\'ia de Abajo | Surface plasmon polariton modes in a single-crystal Au nanoresonator
fabricated using focused-ion-beam milling | 4 pages, 4 figures | null | 10.1063/1.2885344 | null | physics.optics | null | We use focused-ion-beam milling of a single-crystal Au surface to fabricate a
590-nm-long linear ridge that acts as a surface plasmon nanoresonator.
Cathodoluminescence imaging spectroscopy is then used to excite and image
surface plasmons on the ridge. Principal component analysis reveals distinct
plasmonic modes, which proves confinement of surface-plasmon oscillations to
the ridge. Boundary-element-method calculations confirm that a linear ridge is
able to support highly-localized surface-plasmon modes (mode diameter < 100
nm). The results demonstrate that focused-ion-beam milling can be used in rapid
prototyping of nanoscale single-crystal plasmonic components.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 16:42:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Vesseur",
"E. J. R.",
""
],
[
"de Waele",
"R.",
""
],
[
"Polman",
"A.",
""
],
[
"Lezec",
"H. J.",
""
],
[
"Atwater",
"H. A.",
""
],
[
"de Abajo",
"F. J. García",
""
]
] | [
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] |
801.1268 | Fabian Heidrich-Meisner | F. Heidrich-Meisner, A. Honecker and W. Brenig | Transport in quasi one-dimensional spin-1/2 systems | 11 pages, 7 figures | Eur. Phys. J. Special Topics 151, 135-145 (2007) | null | null | cond-mat.str-el cond-mat.stat-mech | null | We present numerical results for the spin and thermal conductivity of
one-dimensional (1D) quantum spin systems. We contrast the properties of
integrable models such as the spin-1/2 XXZ chain against nonintegrable ones
such as frustrated and dimerized chains. The thermal conductivity of the XXZ
chain is ballistic at finite temperatures, while in the nonintegrable models,
this quantity is argued to vanish. For the case of frustrated and dimerized
chains, we discuss the frequency dependence of the transport coefficients.
Finally, we give an overview over related theoretical work on intrinsic and
extrinsic scattering mechanisms of quasi-1D spin systems.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 16:19:38 GMT"
}
] | 2008-01-09T00:00:00 | [
[
"Heidrich-Meisner",
"F.",
""
],
[
"Honecker",
"A.",
""
],
[
"Brenig",
"W.",
""
]
] | [
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] |
801.1269 | Prasanta Das Kumar | Prasanta Kumar Das, V H Satheeshkumar and P. K. Suresh | Plasmon Annihilation into Kaluza-Klein Graviton: New Astrophysical
Constraints on Large Extra Dimensions | 13 pages, 1 ps figure, text is modified a little bit, conclusion
unchanged, new references are added, version accepted for publication in PRD | Phys.Rev.D78:063011,2008 | 10.1103/PhysRevD.78.063011 | BITSGoa-2008/01/001 | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In large extra dimensional Kaluza-Klein (KK) scenario, where the usual
Standard Model (SM) matter is confined to a 3+1-dimensional hypersurface called
the 3-brane and gravity can propagate to the bulk (D=4+d, d being the number of
extra spatial dimensions), the light graviton KK modes can be produced inside
the supernova core due to the usual nucleon-nucleon bremstrahlung,
electron-positron and photon-photon annihilations. This photon inside the
supernova becomes plasmon due to the plasma effect. In this paper, we study the
energy-loss rate of SN 1987A due to the KK gravitons produced from the
plasmon-plasmon annihilation. We find that the SN 1987A cooling rate leads to
the conservative bound $M\_D$ > 22.9 TeV and 1.38 TeV for the case of two and
three space-like extra dimensions.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 16:21:48 GMT"
},
{
"version": "v2",
"created": "Wed, 20 Aug 2008 07:21:33 GMT"
}
] | 2009-02-23T00:00:00 | [
[
"Das",
"Prasanta Kumar",
""
],
[
"Satheeshkumar",
"V H",
""
],
[
"Suresh",
"P. K.",
""
]
] | [
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] |
801.127 | Franck Pereira Dos Santos | J. Le Gou\"et (SYRTE), Tanja Mehlst\"aubler (PTB), Jaewan Kim,
S\'ebastien Merlet (SYRTE), Andre Clairon (SYRTE), Arnaud Landragin (SYRTE),
Franck Pereira Dos Santos (SYRTE) | Limits to the sensitivity of a low noise compact atomic gravimeter | 30 pages, 14 figures | Applied Physics B: Lasers and Optics 92, 2 (2008) 133-144 | 10.1007/s00340-008-3088-1 | null | physics.atom-ph | null | A detailed analysis of the most relevant sources of phase noise in an atomic
interferometer is carried out, both theoretically and experimentally. Even a
short interrogation time of 100 ms allows our cold atom gravimeter to reach an
excellent short term sensitivity to acceleration of $1.4\times 10^{-8}$g at 1s.
This result relies on the combination of a low phase noise laser system,
efficient detection scheme and good shielding from vibrations. In particular,
we describe a simple and robust technique of vibration compensation, which is
based on correcting the interferometer signal by using the AC acceleration
signal measured by a low noise seismometer.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 16:26:51 GMT"
}
] | 2009-01-06T00:00:00 | [
[
"Gouët",
"J. Le",
"",
"SYRTE"
],
[
"Mehlstäubler",
"Tanja",
"",
"PTB"
],
[
"Kim",
"Jaewan",
"",
"SYRTE"
],
[
"Merlet",
"Sébastien",
"",
"SYRTE"
],
[
"Clairon",
"Andre",
"",
"SYRTE"
],
[
"Landragin",
"Arnaud",
"",
"SYRTE"
],
[
"Santos",
"Franck Pereira Dos",
"",
"SYRTE"
]
] | [
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] |
801.1271 | Lior Bary-Soroker | Lior Bary-Soroker and Eli Leher | On the remainder in the Taylor theorem | 2 pages, the proof was shortened | null | null | null | math.CA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We give a short straightforward proof for the bound of the reminder term in
the Taylor theorem. The proof uses only induction and the fact that $f'\geq 0$
implies the monotonicity of $f$, so it might be an attractive proof to give to
undergraduate students.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 16:31:41 GMT"
},
{
"version": "v2",
"created": "Wed, 24 Dec 2008 18:39:11 GMT"
}
] | 2008-12-24T00:00:00 | [
[
"Bary-Soroker",
"Lior",
""
],
[
"Leher",
"Eli",
""
]
] | [
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] |
801.1272 | Iv\'an Mart\'i-Vidal Mr. | I. Marti-Vidal and J.M. Marcaide | Spurious source generation in mapping from noisy phase-self-calibrated
data | 7 pages, 2 figures. Accepted in A&A on 12 December 2007 | null | 10.1051/0004-6361:20078690 | null | astro-ph | null | Phase self-calibration (or selfcal) is an algorithm often used in the
calibration of interferometric observations in astronomy. Although a powerful
tool, this algorithm presents strong limitations when applied to data with a
low signal-to-noise ratio. We analyze the artifacts that the phase selfcal
algorithm produces when applied to extremely noisy data. We show how the phase
selfcal may generate a spurious source in the sky from a distribution of
completely random visibilities. This spurious source is indistinguishable from
a real one. We numerically and analytically compute the relationship between
the maximum spurious flux density generated by selfcal from noise and the
particulars of the interferometric observations. Finally, we present two simple
tests that can be applied to interferometric data for checking whether a source
detection is real or whether the source is an artifact of the phase
self-calibration algorithm.
| [
{
"version": "v1",
"created": "Tue, 8 Jan 2008 16:40:14 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Marti-Vidal",
"I.",
""
],
[
"Marcaide",
"J. M.",
""
]
] | [
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