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712.3579 | Diana Worrall | D.M. Worrall, M. Birkinshaw, R.P. Kraft, G.R. Sivakoff, A. Jordan,
M.J. Hardcastle, N.J. Brassington, J.H. Croston, D.A. Evans, W.R. Forman,
W.E. Harris, C. Jones, A.M. Juett, S.S. Murray, P.E.J. Nulsen, S.
Raychaudhury, C.L. Sarazin, K.A. Woodley | Where Centaurus A gets its X-ray knottiness | Accepted for publication in ApJ (Letters) | null | 10.1086/528681 | null | astro-ph | null | We report an X-ray spectral study of the transverse structure of the
Centaurus A jet using new data from the Chandra Cen A Very Large Project. We
find that the spectrum steepens with increasing distance from the jet axis, and
that this steepening can be attributed to a change in the average spectrum of
the knotty emission. Such a trend is unexpected if the knots are predominantly
a surface feature residing in a shear layer between faster and slower flows. We
suggest that the spectral steepening of the knot emission as a function of
distance from the jet axis is due to knot migration, implying a component of
transverse motion of knots within the flow.
| [
{
"version": "v1",
"created": "Thu, 20 Dec 2007 21:20:11 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Worrall",
"D. M.",
""
],
[
"Birkinshaw",
"M.",
""
],
[
"Kraft",
"R. P.",
""
],
[
"Sivakoff",
"G. R.",
""
],
[
"Jordan",
"A.",
""
],
[
"Hardcastle",
"M. J.",
""
],
[
"Brassington",
"N. J.",
""
],
[
"Croston",
"J. H.",
""
],
[
"Evans",
"D. A.",
""
],
[
"Forman",
"W. R.",
""
],
[
"Harris",
"W. E.",
""
],
[
"Jones",
"C.",
""
],
[
"Juett",
"A. M.",
""
],
[
"Murray",
"S. S.",
""
],
[
"Nulsen",
"P. E. J.",
""
],
[
"Raychaudhury",
"S.",
""
],
[
"Sarazin",
"C. L.",
""
],
[
"Woodley",
"K. A.",
""
]
] | [
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712.358 | David Kalaj | David Kalaj | A priori estimate of gradient of a solution to certain differential
inequality and quasiconformal mappings | 24 pages | null | null | null | math.AP math.CV | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We will prove a global estimate for the gradient of the solution to the {\it
Poisson differential inequality} $|\Delta u(x)|\le a|\nabla u(x)|^2+b$, $x\in
B^{n}$, where $a,b<\infty$ and $u|_{S^{n-1}}\in C^{1,\alpha}(S^{n-1}, \Bbb
R^m)$. If $m=1$ and $a\le (n+1)/(|u|_\infty4n\sqrt n)$, then $|\nabla u| $ is a
priori bounded. This generalizes some similar results due to E. Heinz
(\cite{EH}) and Bernstein (\cite{BS}) for the plane. An application of these
results yields the theorem, which is the main result of the paper: A
quasiconformal mapping of the unit ball onto a domain with $C^2$ smooth
boundary, satisfying the Poisson differential inequality, is Lipschitz
continuous. This extends some results of the author, Mateljevi\'c and
Pavlovi\'c from the complex plane to the space.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 08:42:39 GMT"
},
{
"version": "v2",
"created": "Mon, 6 Oct 2008 20:01:52 GMT"
},
{
"version": "v3",
"created": "Sun, 13 Dec 2009 09:40:42 GMT"
}
] | 2009-12-14T00:00:00 | [
[
"Kalaj",
"David",
""
]
] | [
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712.3581 | Andrew Houck | J. A. Schreier, A. A. Houck, Jens Koch, D. I. Schuster, B. R. Johnson,
J. M. Chow, J. M. Gambetta, J. Majer, L. Frunzio, M. H. Devoret, S. M.
Girvin, and R. J. Schoelkopf | Suppressing Charge Noise Decoherence in Superconducting Charge Qubits | 4+ pages, 4 figures | Phys. Rev. B 77, 180502(R) (2008) | 10.1103/PhysRevB.77.180502 | null | cond-mat.mes-hall cond-mat.supr-con quant-ph | null | We present an experimental realization of the transmon qubit, an improved
superconducting charge qubit derived from the Cooper pair box. We
experimentally verify the predicted exponential suppression of sensitivity to
1/f charge noise [J. Koch et al., Phys. Rev. A 76, 042319 (2007)]. This removes
the leading source of dephasing in charge qubits, resulting in homogenously
broadened transitions with relaxation and dephasing times in the microsecond
range. Our systematic characterization of the qubit spectrum, anharmonicity,
and charge dispersion shows excellent agreement with theory, rendering the
transmon a promising qubit for future steps towards solid-state quantum
information processing.
| [
{
"version": "v1",
"created": "Thu, 20 Dec 2007 21:59:57 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Schreier",
"J. A.",
""
],
[
"Houck",
"A. A.",
""
],
[
"Koch",
"Jens",
""
],
[
"Schuster",
"D. I.",
""
],
[
"Johnson",
"B. R.",
""
],
[
"Chow",
"J. M.",
""
],
[
"Gambetta",
"J. M.",
""
],
[
"Majer",
"J.",
""
],
[
"Frunzio",
"L.",
""
],
[
"Devoret",
"M. H.",
""
],
[
"Girvin",
"S. M.",
""
],
[
"Schoelkopf",
"R. J.",
""
]
] | [
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] |
712.3582 | Nicola Brassington | N. J. Brassington (Harvard-Smithsonian Center for Astrophysics) | The LMXB Population of NGC 3379 | Conference proceedings from 'A Population Explosion: The Nature and
Evolution of X-ray Binaries in Diverse Environments', 28 Oct - 2 Nov, St.
Petersburg Beach, FL, 3 pages, 3 figures | null | null | null | astro-ph | null | Presented here are the highlights from the deep Chandra observation of the
elliptical galaxy NGC 3379. From the multi-epoch observation of this galaxy,
132 discrete X-ray sources have been detected within the region overlapped by
all observations, 98 of which lie within the D25 ellipse of the galaxy. Of
these 132 sources, 71 exhibit long-term variability, indicating that they are
accreting compact objects. 11 of these sources have been identified as
transient candidates, with a further 7 possible transients. In addition to
this, from the joint Hubble/Chandra field of view, nine globular clusters (GCs)
and 53 field low mass X-ray binaries (LMXBs) have been detected in the galaxy.
Comparisons of these two populations reveals that, at higher luminosities the
field LMXBs and GC-LMXBs are similar. However, a significant lack of GC-LMXBs
has been found at lower luminosities, indicating that not all LMXBs can form in
GCs.
| [
{
"version": "v1",
"created": "Thu, 20 Dec 2007 21:40:29 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Brassington",
"N. J.",
"",
"Harvard-Smithsonian Center for Astrophysics"
]
] | [
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] |
712.3583 | Peter Lunkenheimer | F. Schrettle, S. Krohns, P. Lunkenheimer, J. Hemberger, N. B\"uttgen,
H.-A. Krug von Nidda, A. V. Prokofiev, and A. Loidl | Switching the Ferroelectric Polarization by External Magnetic Fields in
the Spin = 1/2 Chain Cuprate LiCuVO4 | 6 pages, 5 figures | Phys. Rev. B 77, 144101 (2008) | 10.1103/PhysRevB.77.144101 | null | cond-mat.str-el | null | We present a detailed study of complex dielectric constant and ferroelectric
polarization in multiferroic LiCuVO4 as function of temperature and external
magnetic field. In zero external magnetic field, spiral spin order with an ab
helix and a propagation vector along the crystallographic b direction is
established, which induces ferroelectric order with spontaneous polarization
parallel to a. The direction of the helix can be reoriented by an external
magnetic field and allows switching of the spontaneous polarization. We find a
strong dependence of the absolute value of the polarization for different
orientations of the spiral plane. Above 7.5 T, LiCuVO4 reveals collinear spin
order and remains paraelectric for all field directions. Thus this system is
ideally suited to check the symmetry relations for spiral magnets as predicted
theoretically. The strong coupling of ferroelectric and magnetic order is
documented and the complex (B,T) phase diagram is fully explored.
| [
{
"version": "v1",
"created": "Thu, 20 Dec 2007 21:37:29 GMT"
}
] | 2008-04-15T00:00:00 | [
[
"Schrettle",
"F.",
""
],
[
"Krohns",
"S.",
""
],
[
"Lunkenheimer",
"P.",
""
],
[
"Hemberger",
"J.",
""
],
[
"Büttgen",
"N.",
""
],
[
"von Nidda",
"H. -A. Krug",
""
],
[
"Prokofiev",
"A. V.",
""
],
[
"Loidl",
"A.",
""
]
] | [
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] |
712.3584 | Jan de Gier | Jan de Gier, Pavel Pyatov and Paul Zinn-Justin | Punctured plane partitions and the q-deformed Knizhnik--Zamolodchikov
and Hirota equations | 27 pages, 29 eps figures, section rewritten and reference added | J. Combin. Theory A 116 (2009), 772--794 | 10.1016/j.jcta.2008.11.008 | null | math.CO math-ph math.MP math.RT | null | We consider partial sum rules for the homogeneous limit of the solution of
the q-deformed Knizhnik--Zamolodchikov equation with reflecting boundaries in
the Dyck path representation. We show that these partial sums arise in a
solution of the discrete Hirota equation, and prove that they are the
generating functions of $\tau^2$-weighted punctured cyclically symmetric
transpose complement plane partitions where $\tau=-(q+q^{-1})$. In the cases of
no or minimal punctures, we prove that these generating functions coincide with
$\tau^2$-enumerations of vertically symmetric alternating sign matrices and
modifications thereof.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 03:49:58 GMT"
},
{
"version": "v2",
"created": "Mon, 7 Jan 2008 09:26:32 GMT"
}
] | 2010-07-06T00:00:00 | [
[
"de Gier",
"Jan",
""
],
[
"Pyatov",
"Pavel",
""
],
[
"Zinn-Justin",
"Paul",
""
]
] | [
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] |
712.3585 | Eran O. Ofek | E. O. Ofek, M. Muno, R. Quimby, S. R. Kulkarni, H. Stiele, W. Pietsch,
E. Nakar, A. Gal-Yam, A. Rau, P. B. Cameron, S. B. Cenko, M. M. Kasliwal, D.
B. Fox, P. Chandra, A. K. H. Kong, R. Barnard | GRB 070201: A possible Soft Gamma Ray Repeater in M31 | 7 pages, submitted to ApJ (Fig. 2 resolution reduced) | Astrophys.J.681:1464-1469,2008 | 10.1086/587686 | null | astro-ph | null | The gamma-ray burst (GRB) 070201 was a bright short-duration hard-spectrum
GRB detected by the Inter-Planetary Network (IPN). Its error quadrilateral,
which has an area of 0.124 sq. deg, intersects some prominent spiral arms of
the nearby M31 (Andromeda) galaxy. Given the properties of this GRB, along with
the fact that LIGO data argues against a compact binary merger origin in M31,
this GRB is an excellent candidate for an extragalactic Soft Gamma-ray Repeater
(SGR) giant flare, with energy of 1.4x10^45 erg. Analysis of ROTSE-IIIb visible
light observations of M31, taken 10.6 hours after the burst and covering 42% of
the GRB error region, did not reveal any optical transient down to a limiting
magnitude of 17.1. We inspected archival and proprietary XMM-Newton X-ray
observations of the intersection of the GRB error quadrilateral and M31,
obtained about four weeks prior to the outburst, in order to look for periodic
variable X-ray sources. No SGR or Anomalous X-ray Pulsar (AXP) candidates
(periods in range 1 to 20 s) were detected. We discuss the possibility of
detecting extragalactic SGRs/AXPs by identifying their periodic X-ray light
curves. Our simulations suggest that the probability of detecting the periodic
X-ray signal of one of the known Galactic SGRs/AXPs, if placed in M31, is about
10% (50%), using 50 ks (2 Ms) XMM-Newton exposures.
| [
{
"version": "v1",
"created": "Thu, 20 Dec 2007 21:50:40 GMT"
}
] | 2011-05-18T00:00:00 | [
[
"Ofek",
"E. O.",
""
],
[
"Muno",
"M.",
""
],
[
"Quimby",
"R.",
""
],
[
"Kulkarni",
"S. R.",
""
],
[
"Stiele",
"H.",
""
],
[
"Pietsch",
"W.",
""
],
[
"Nakar",
"E.",
""
],
[
"Gal-Yam",
"A.",
""
],
[
"Rau",
"A.",
""
],
[
"Cameron",
"P. B.",
""
],
[
"Cenko",
"S. B.",
""
],
[
"Kasliwal",
"M. M.",
""
],
[
"Fox",
"D. B.",
""
],
[
"Chandra",
"P.",
""
],
[
"Kong",
"A. K. H.",
""
],
[
"Barnard",
"R.",
""
]
] | [
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712.3586 | Timo Aspelmeier | T. Aspelmeier | Free energy fluctuations and chaos in the Sherrington-Kirkpatrick model | 4.5 pages, no figures. This manuscript supersedes
arXiv:cond-mat/0610228 | Phys. Rev. Lett. 100:117205, 2008 | 10.1103/PhysRevLett.100.117205 | null | cond-mat.dis-nn | null | The sample-to-sample fluctuations Delta F_N of the free energy in the
Sherrington-Kirkpatrick model are shown rigorously to be related to bond chaos.
Via this connection, the fluctuations become analytically accessible by replica
methods. The replica calculation for bond chaos shows that the exponent mu
governing the growth of the fluctuations with system size N, i.e. Delta F_N
N^mu, is bounded by mu <= 1/4.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 09:39:37 GMT"
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] |
712.3587 | Po-Hsiang Lai | Po-Hsiang Lai and Joseph A. O'Sullivan | Pattern Recognition System Design with Linear Encoding for Discrete
Patterns | Submitted and accepted to ISIT 2007 | null | null | null | cs.IT cs.CV math.IT | null | In this paper, designs and analyses of compressive recognition systems are
discussed, and also a method of establishing a dual connection between designs
of good communication codes and designs of recognition systems is presented.
Pattern recognition systems based on compressed patterns and compressed sensor
measurements can be designed using low-density matrices. We examine truncation
encoding where a subset of the patterns and measurements are stored perfectly
while the rest is discarded. We also examine the use of LDPC parity check
matrices for compressing measurements and patterns. We show how more general
ensembles of good linear codes can be used as the basis for pattern recognition
system design, yielding system design strategies for more general noise models.
| [
{
"version": "v1",
"created": "Thu, 20 Dec 2007 22:46:29 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Lai",
"Po-Hsiang",
""
],
[
"O'Sullivan",
"Joseph A.",
""
]
] | [
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712.3588 | V\'ictor Rivero | Andreas E. Kyprianou and V\'i ctor Rivero | Special, conjugate and complete scale functions for spectrally negative
L\'evy processes | null | null | null | null | math.PR | null | Following from recent developments by Hubalek and Kyprianou, the objective of
this paper is to provide further methods for constructing new families of scale
functions for spectrally negative L\'evy processes which are completely
explicit. This is the result of an observation in the aforementioned paper
which permits feeding the theory of Bernstein functions directly into the
Wiener-Hopf factorization for spectrally negative L\'evy processes. Many new,
concrete examples of scale functions are offered although the methodology in
principle delivers still more explicit examples than those listed.
| [
{
"version": "v1",
"created": "Thu, 20 Dec 2007 22:35:48 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Kyprianou",
"Andreas E.",
""
],
[
"Rivero",
"Ví ctor",
""
]
] | [
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712.3589 | Mikhail Volkov | Julien Garaud and Mikhail S. Volkov | Stability Analysis of The Twisted Superconducting Semilocal Strings | 33 pages, 6 figures. to appear in Nuclear Physics B | Nucl.Phys.B799:430-455,2008 | 10.1016/j.nuclphysb.2008.01.022 | null | hep-th cond-mat.supr-con hep-ph | null | We study the stability properties of the twisted vortex solutions in the
semilocal Abelian Higgs model with a global $\mathbf{SU}(2)$ invariance. This
model can be viewed as the Weinberg-Salam theory in the limit where the
non-Abelian gauge field decouples, or as a two component Ginzburg-Landau
theory. The twisted vortices are characterized by a constant global current
${\cal I}$, and for ${\cal I}\to 0$ they reduce to the semilocal strings, that
is to the Abrikosov-Nielsen-Olesen vortices embedded into the semilocal model.
Solutions with ${\cal I}\neq 0$ are more complex and, in particular, they are
{\it less energetic} than the semilocal strings, which makes one hope that they
could have better stability properties. We consider the generic field
fluctuations around the twisted vortex within the linear perturbation theory
and apply the Jacobi criterion to test the existence of the negative modes in
the spectrum of the fluctuation operator. We find that twisted vortices do not
have the homogeneous instability known for the semilocal strings, neither do
they have inhomogeneous instabilities whose wavelength is less than a certain
critical value. This implies that short enough vortex pieces are perturbatively
stable and suggests that small vortex loops could perhaps be stable as well.
For longer wavelength perturbations there is exactly one negative mode in the
spectrum whose growth entails a segmentation of the uniform vortex into a
non-uniform, `sausage like' structure. This instability is qualitatively
similar to the hydrodynamical Plateau-Rayleigh instability of a water jet or to
the Gregory-Laflamme instability of black strings in the theory of gravity in
higher dimensions.
| [
{
"version": "v1",
"created": "Thu, 20 Dec 2007 22:55:35 GMT"
},
{
"version": "v2",
"created": "Sun, 23 Dec 2007 21:39:36 GMT"
},
{
"version": "v3",
"created": "Thu, 24 Jan 2008 22:15:04 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Garaud",
"Julien",
""
],
[
"Volkov",
"Mikhail S.",
""
]
] | [
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] |
712.359 | Tomasz Rusin dr | Tomasz M. Rusin and Wlodek Zawadzki | Zitterbewegung of electrons in graphene in a magnetic field | 9 pages, 8 figures | Phys. Rev. B 78, 125419 (2008) | 10.1103/PhysRevB.78.125419 | null | cond-mat.mes-hall cond-mat.mtrl-sci | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Electric current and spacial displacement due to trembling motion
[Zitterbewegung (ZB)] of electrons in graphene in the presence of an external
magnetic field are described. Contributions of both inequivalent $K$ points in
the Brillouin zone of graphene are considered. It is shown that, when the
electrons are prepared in the form of wave packets, the presence of a
quantizing magnetic field $B$ has very important effects on ZB. (1) For $B\neq
0$ the ZB oscillations are permanent, for B=0 they are transient. (2) For
$B\neq 0$ many ZB frequencies appear, for B=0 only one frequency is at work.
(3) For $B\neq 0$ both interband and intraband (cyclotron) frequencies
contribute to ZB, for B=0 there are no intraband frequencies. (4) Magnetic
field intensity changes not only the ZB frequencies but the entire character of
ZB spectrum. An emission of electromagnetic dipole radiation by the trembling
electrons is proposed and described. It is argued that graphene in a magnetic
field is a promising system for an experimental observation of Zitterbewegung.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 06:52:08 GMT"
},
{
"version": "v2",
"created": "Mon, 7 Jul 2008 19:27:50 GMT"
}
] | 2010-03-30T00:00:00 | [
[
"Rusin",
"Tomasz M.",
""
],
[
"Zawadzki",
"Wlodek",
""
]
] | [
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712.3591 | Michael Schindler | M. Schindler and A. Ajdari | Droplet traffic in microfluidic networks: A simple model for
understanding and designing | accepted for publication in PRL | Phys. Rev. Lett. 100, 044501 (2008) | 10.1103/PhysRevLett.100.044501 | null | physics.flu-dyn math.DS nlin.CD | null | We propose a simple model to analyze the traffic of droplets in microfluidic
``dual networks''. Such functional networks which consist of two types of
channels, namely those accessible or forbidden to droplets, often display a
complex behavior characteristic of dynamical systems. By focusing on three
recently proposed configurations, we offer an explanation for their remarkable
behavior. Additionally, the model allows us to predict the behavior in
different parameter regimes. A verification will clarify fundamental issues,
such as the network symmetry, the role of the driving conditions, and of the
occurrence of reversible behavior. The model lends itself to a fast numerical
implementation, thus can help designing devices, identifying parameter windows
where the behavior is sufficiently robust for a devices to be practically
useful, and exploring new functionalities.
| [
{
"version": "v1",
"created": "Thu, 20 Dec 2007 22:50:01 GMT"
}
] | 2008-01-30T00:00:00 | [
[
"Schindler",
"M.",
""
],
[
"Ajdari",
"A.",
""
]
] | [
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] |
712.3592 | Friederike Schmid | Jens Smiatek, Michael P. Allen, Friederike Schmid | Tunable-slip boundaries for coarse-grained simulations of fluid flow | submitted to Eur. Phys. J. E (accepted) | null | 10.1140/epje/i2007-10311-4 | null | physics.comp-ph physics.flu-dyn | null | On the micro- and nanoscale, classical hydrodynamic boundary conditions such
as the no-slip condition no longer apply. Instead, the flow profiles exhibit
``slip`` at the surface, which is characterized by a finite slip length
(partial slip). We present a new, systematic way of implementing partial-slip
boundary conditions with arbitrary slip length in coarse-grained computer
simulations. The main idea is to represent the complex microscopic interface
structure by a spatially varying effective viscous force. An analytical
equation for the resulting slip length can be derived for planar and for curved
surfaces. The comparison with computer simulations of a DPD (dissipative
particle dynamics) fluid shows that this expression is valid from full-slip to
no-slip.
| [
{
"version": "v1",
"created": "Thu, 20 Dec 2007 22:55:31 GMT"
},
{
"version": "v2",
"created": "Thu, 20 Mar 2008 10:29:21 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Smiatek",
"Jens",
""
],
[
"Allen",
"Michael P.",
""
],
[
"Schmid",
"Friederike",
""
]
] | [
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] |
712.3593 | Ferran Mazzanti | F.Mazzanti, G.E.Astrakharchik, J.Boronat, J.Casulleras | Off-diagonal Ground State Properties of a 1D Gas of Fermi Hard Rods | 5 figures | null | 10.1103/PhysRevA.77.043632 | null | cond-mat.stat-mech | null | A variational Monte Carlo calculation of the one-body density matrix and
momentum distribution of a system of Fermi hard rods (HR) is presented and
compared with the same quantities for its bosonic counterpart. The calculation
is exact within statistical errors since we sample the exact ground state wave
function, whose analytical expression is known. The numerical results are in
good agreement with known asymptotic expansions valid for Luttinger liquids. We
find that the difference between the absolute value of the bosonic and
fermionic density matrices becomes marginally small as the density increases.
In this same regime, the corresponding momentum distributions merge into a
common profile that is independent of the statistics. Non-analytical
contributions to the one--body density matrix are also discussed and found to
be less relevant with increasing density.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 14:17:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mazzanti",
"F.",
""
],
[
"Astrakharchik",
"G. E.",
""
],
[
"Boronat",
"J.",
""
],
[
"Casulleras",
"J.",
""
]
] | [
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] |
712.3594 | Xi Chen | Xi Chen, Edward L. Wright (UCLA) | Extragalactic Point Source Search in WMAP 61 and 94 GHz Data | 22 pages, 10 figures, submitted to ApJ; Typo corrected in the
uncertainty of kappa in the Discussion, and a correction to the description
of the smoothing function in Methodology | null | 10.1086/588249 | null | astro-ph | null | We report the results of an extragalactic point source search using the 61
and 94 GHz (V- and W-band) temperature maps from the Wilkinson Microwave
Anisotropy Probe (WMAP). Applying a method that cancels the ``noise'' due to
the CMB anisotropy signal, we find in the $|b| > 10\degr$ region 31 sources in
the first-year maps and 64 sources in the three-year co-added maps, at a
$5\sigma$ level. The 1$\sigma$ position uncertainties are 1.6' and 1.4' each.
The increased detections and improved positional accuracy are expected from the
higher signal-to-noise ratio of WMAP three-year data. All sources detected in
the first-year maps are repeatedly detected in the three-year maps, which is a
strong proof of the consistency and reliability of this method. Among all the
detections, 21 are new, i.e. not in the WMAP three-year point source catalog.
We associate all but two of them with known objects. The two unidentified
sources are likely to be variable or extended as observations through VLA,
CARMA and ATCA all show non-detection at the nominal locations. We derive the
source count distribution at WMAP V-band by combining our verified detections
with sources from the WMAP three-year catalog. Assuming the effect of source
clustering is negligible, the contribution to the power spectrum from faint
sources below 0.75 Jy is estimated to be $(2.4\pm0.8) \times 10^{-3} \mu K^2$
sr for V-band, which implies a source correction amplitude $A = 0.012\pm0.004
\mu K^2$ sr.
| [
{
"version": "v1",
"created": "Thu, 20 Dec 2007 23:16:16 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jan 2008 00:16:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Chen",
"Xi",
"",
"UCLA"
],
[
"Wright",
"Edward L.",
"",
"UCLA"
]
] | [
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] |
712.3595 | Kuang-Ta Chao | Ce Meng, Kuang-Ta Chao | Scalar Resonance Contributions to the Dipion Transition Rates of
$\Upsilon(4S,5S)$ in the re-scattering model | version to appear in Phys. Rev. D, discussions and references added | Phys.Rev.D77:074003,2008 | 10.1103/PhysRevD.77.074003 | null | hep-ph hep-ex | null | In order to explain the observed unusually large dipion transition rates of
$\Upsilon(10870)$, the scalar resonance contributions in the re-scattering
model to the dipion transitions of $\Upsilon(4S)$ and $\Upsilon(5S)$ are
studied. Since the imaginary part of the re-scattering amplitude is expected to
be dominant, the large ratios of the transition rates of $\Upsilon(10870)$,
which is identified with $\Upsilon(5S)$, to that of $\Upsilon(4S)$ can be
understood as mainly coming from the difference between the $p$-values in their
decays into open bottom channels, and the ratios are estimated numerically to
be about 200-600 with reasonable choices of parameters. The absolute and
relative rates of $\Upsilon(5S)\to\Upsilon(1S,2S,3S)\pi^+\pi^-$ and
$\Upsilon(5S)\to\Upsilon(1S)K^+K^-$ are roughly consistent with data. We
emphasize that the dipion transitions observed for some of the newly discovered
$Y$ states associated with charmonia may have similar features to the dipion
transitions of $\Upsilon(5S)$. Measurements on the dipion transitions of
$\Upsilon(6S)$ could provide further test for this mechanism.
| [
{
"version": "v1",
"created": "Thu, 20 Dec 2007 23:56:52 GMT"
},
{
"version": "v2",
"created": "Thu, 28 Feb 2008 13:58:33 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Meng",
"Ce",
""
],
[
"Chao",
"Kuang-Ta",
""
]
] | [
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] |
712.3596 | Anatoly Kolomeisky | Max N. Artyomov, Alexander Yu. Morozov and Anatoly B. Kolomeisky | Molecular Motors Interacting with Their Own Tracks | null | null | 10.1103/PhysRevE.77.040901 | null | cond-mat.soft cond-mat.stat-mech | null | Dynamics of molecular motors that move along linear lattices and interact
with them via reversible destruction of specific lattice bonds is investigated
theoretically by analyzing exactly solvable discrete-state ``burnt-bridge''
models. Molecular motors are viewed as diffusing particles that can
asymmetrically break or rebuild periodically distributed weak links when
passing over them. Our explicit calculations of dynamic properties show that
coupling the transport of the unbiased molecular motor with the bridge-burning
mechanism leads to a directed motion that lowers fluctuations and produces a
dynamic transition in the limit of low concentration of weak links. Interaction
between the backward biased molecular motor and the bridge-burning mechanism
yields a complex dynamic behavior. For the reversible dissociation the backward
motion of the molecular motor is slowed down. There is a change in the
direction of the molecular motor's motion for some range of parameters. The
molecular motor also experiences non-monotonic fluctuations due to the action
of two opposing mechanisms: the reduced activity after the burned sites and
locking of large fluctuations. Large spatial fluctuations are observed when two
mechanisms are comparable. The properties of the molecular motor are different
for the irreversible burning of bridges where the velocity and fluctuations are
suppressed for some concentration range, and the dynamic transition is also
observed. Dynamics of the system is discussed in terms of the effective driving
forces and transitions between different diffusional regimes.
| [
{
"version": "v1",
"created": "Thu, 20 Dec 2007 23:35:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Artyomov",
"Max N.",
""
],
[
"Morozov",
"Alexander Yu.",
""
],
[
"Kolomeisky",
"Anatoly B.",
""
]
] | [
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] |
712.3597 | Ryan Kalas | Ryan M. Kalas, D. Blume | Dilute Bose gases interacting via power-law potentials | 7 pages, 4 figures | null | 10.1103/PhysRevA.77.032703 | null | cond-mat.other | null | Neutral atoms interact through a van der Waals potential which asymptotically
falls off as r^{-6}. In ultracold gases, this interaction can be described to a
good approximation by the atom-atom scattering length. However, corrections
arise that depend on the characteristic length of the van der Waals potential.
We parameterize these corrections by analyzing the energies of two- and
few-atom systems under external harmonic confinement, obtained by numerically
and analytically solving the Schrodinger equation. We generalize our results to
particles interacting through a longer-ranged potential which asymptotically
falls off as r^{-4}.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 00:24:41 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kalas",
"Ryan M.",
""
],
[
"Blume",
"D.",
""
]
] | [
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] |
712.3598 | Radu A. Ionas | Radu A. Ionas | Elliptic constructions of hyperkaehler metrics I: The Atiyah-Hitchin
manifold | 40 pages, 1 figure | null | null | YITP-SB-07-39 | math.DG hep-th | null | This is the first in a series of papers in which we develop a twistor-based
method of constructing hyperkaehler metrics from holomorphic functions and
elliptic curves. As an application, we revisit the Atiyah-Hitchin manifold and
derive in an explicit holomorphic coordinate basis closed-form formulas for,
among other things, the metric, the holomorphic symplectic form and all three
Kaehler potentials.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 17:41:18 GMT"
}
] | 2008-01-05T00:00:00 | [
[
"Ionas",
"Radu A.",
""
]
] | [
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] |
712.3599 | Steve Zelditch | Jian Song and Steve Zelditch | Test configurations, large deviations and geodesic rays on toric
varieties | 42 pages, no figures | Advances in Mathematics 229 (2012) pp. 2338-2378 | null | null | math.DG math.CV | null | This article contains a detailed study, in the toric case, of the test
configuration geodesic rays defined by Phong-Sturm. We show that the `Bergman
approximations' of Phong-Sturm converge in C^1 to the geodesic ray and that the
geodesic ray itself is C^{1,1} and no better. The \kahler metrics associated to
the geodesic ray of potentials are discontinuous across certain hypersurfaces
and are degenerate on certain open sets. A novelty in the analysis is the
connection between Bergman metrics, Bergman kernels and the theory of large
deviations.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 00:29:23 GMT"
}
] | 2012-01-31T00:00:00 | [
[
"Song",
"Jian",
""
],
[
"Zelditch",
"Steve",
""
]
] | [
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] |
712.36 | Radu A. Ionas | Radu A. Ionas | Elliptic constructions of hyperkaehler metrics II: The quantum mechanics
of a Swann bundle | 25 pages, 3 figures | null | null | YITP-SB-07-40 | math.DG hep-th | null | The generalized Legendre transform method of Lindstrom and Rocek yields
hyperkaehler metrics from holomorphic functions. Its main ingredients are
sections of ${\cal O}(2j)$ bundles over the twistor space satisfying a reality
condition with respect to antipodal conjugation on the hyperkaehler sphere of
complex structures. Formally, the structure of the real ${\cal O}(2j)$ sections
is identical to that of quantum-mechanical wave functions describing the states
of a particle with spin $j$ in the spin coherent representation. We analyze
these sections and their SO(3) invariants and illustrate our findings with two
Swann bundle constructions.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 17:43:32 GMT"
}
] | 2008-01-05T00:00:00 | [
[
"Ionas",
"Radu A.",
""
]
] | [
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] |
712.3601 | Radu A. Ionas | Radu A. Ionas | Elliptic constructions of hyperkaehler metrics III: Gravitons and
Poncelet polygons | 26 pages, 7 figures | null | null | YITP-SB-07-41 | math.DG hep-th | null | In the generalized Legendre approach, the equation describing an
asymptotically locally Euclidean space of type $D_n$ is found to admit an
algebraic formulation in terms of the group law on a Weierstrass cubic. This
curve has the structure of a Cayley cubic for a pencil generated by two
transversal plane conics, that is, it takes the form $Y^2 = \det ({\cal
A}+X{\cal B})$, where ${\cal A}$ and ${\cal B}$ are the defining $3 \times 3$
matrices of the conics. In this light, the equation can be interpreted as the
closure condition for an elliptic billiard trajectory tangent to the conic
${\cal B}$ and bouncing into various conics of the pencil determined by the
positions of the monopoles. Poncelet's porism guarantees then that once a
trajectory closes to a star polygon, any trajectory will close, regardless of
the starting point and after the same number of steps.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 17:45:44 GMT"
}
] | 2008-01-05T00:00:00 | [
[
"Ionas",
"Radu A.",
""
]
] | [
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] |
712.3602 | Zong-Hong Zhu | Zong-Hong Zhu, Ming Hu, J. S. Alcaniz, Yu-Xing Liu | Testing power-law cosmology with galaxy clusters | 8 pages, 2 figures, 1 table, accepted for publication in A&A | Astro.Astrophys. 483 (2008) 15-18 | 10.1051/0004-6361:20077797 | null | astro-ph | null | Power-law cosmologies, in which the cosmological scale factor evolves as a
power law in the age, $a \propto t^{\alpha}$ with $\alpha \ga 1$, regardless of
the matter content or cosmological epoch, is comfortably concordant with a host
of cosmological observations.} {In this article, we use recent measurements of
the X-ray gas mass fractions in clusters of galaxies to constrain the $\alpha$
parameter with curvature $k = \pm1, 0$. We find that the best fit happens for
an open scenario with the power index $\alpha = 1.14 \pm 0.05$, though the flat
and closed model can not be rule out at very high confidence level.} {Our
results are in agreement with other recent analyses and show that the X-ray gas
mass fraction measurements in clusters of galaxies provide a complementary test
to the power law cosmology.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 00:44:30 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Zhu",
"Zong-Hong",
""
],
[
"Hu",
"Ming",
""
],
[
"Alcaniz",
"J. S.",
""
],
[
"Liu",
"Yu-Xing",
""
]
] | [
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] |
712.3603 | Zong-Hong Zhu | Xing Wu and Zong-Hong Zhu | Reconstructing f(R) theory according to holographic dark energy | 6 pages, 4 figures, accepted for publication in Physics Letters B | Phys.Lett.B660:293-298,2008 | 10.1016/j.physletb.2007.12.031 | null | astro-ph | null | In this paper a connection between the holographic dark energy model and the
$f(R)$ theory is established. We treat the $f(R)$ theory as an effective
description for the holographic dark energy and reconstruct the function $f(R)$
with the parameter $c>1$, $c=1$ and $c<1$, respectively. We show the
distinctive behavior of each cases realized in $f(R)$ theory, especially for
the future evolution.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 00:45:12 GMT"
},
{
"version": "v2",
"created": "Sun, 23 Dec 2007 05:55:42 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Wu",
"Xing",
""
],
[
"Zhu",
"Zong-Hong",
""
]
] | [
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] |
712.3604 | Zong-Hong Zhu | Xing Wu, Rong-Gen Cai, Zong-Hong Zhu | Dynamics of holographic vacuum energy in the DGP model | 11 pages, 18 figures, accepted for publication in Physical Review D | Phys.Rev.D77:043502,2008 | 10.1103/PhysRevD.77.043502 | null | astro-ph | null | We consider the evolution of the vacuum energy in the DGP model according to
the holographic principle under the assumption that the relation linking the IR
and UV cut-offs still holds in this scenario. The model is studied when the IR
cut-off is chosen to be the Hubble scale $H^{-1}$, the particle horizon $R_{\rm
ph}$ and the future event horizon $R_{\rm eh}$, respectively. And the two
branches of the DGP model are also taken into account. Through numerical
analysis, we find that in the cases of $H^{-1}$ in the (+) branch and $R_{\rm
eh}$ in both branches, the vacuum energy can play the role of dark energy.
Moreover, when considering the combination of the vacuum energy and the 5D
gravity effect in both branches, the equation of state of the effective dark
energy may cross -1, which may lead to the Big Rip singularity. Besides, we
constrain the model with the Type Ia supernovae and baryon oscillation data and
find that our model is consistent with current data within $1\sigma$, and that
the observations prefer either a pure holographic dark energy or a pure DGP
model
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 00:45:48 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Wu",
"Xing",
""
],
[
"Cai",
"Rong-Gen",
""
],
[
"Zhu",
"Zong-Hong",
""
]
] | [
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] |
712.3605 | Xin L\"u | Yajie Xu, Zhi Ma, Chunyuan Zhang, Xin L\"u | Logic Functions and Quantum Error Correcting Codes | 12 pages | null | null | null | quant-ph | null | In this paper, based on the relationship between logic functions and quantum
error correcting codes(QECCs), we unify the construction of QECCs via graphs,
projectors and logic functions. A construction of QECCs over a prime field
GF(p) is given, and one of the results given by Ref[8] can be viewed as a
corollary of one theorem in this paper. With the help of Boolean functions, we
give a clear proof of the existence of a graphical QECC in mathematical view,
and find that the existence of an [[n,k,d]] QECC over GF(p) requires similar
conditions with that depicted in Ref[9]. The result that under the
correspondence defined in Ref[17], every [[n,0,d]] QECC over GF(2)
corresponding to a simple undirected graph has a Boolean basis state, which is
closely related to the adjacency matrix of the graph, is given.
After a modification of the definition of operators, we find that some QECCs
constructed via projectors depicted in Ref[11] can have Boolean basis states. A
necessary condition for a Boolean function being used in the construction via
projectors is given. We also give some examples to illustrate our results.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 00:55:22 GMT"
},
{
"version": "v2",
"created": "Thu, 27 Dec 2007 14:31:18 GMT"
},
{
"version": "v3",
"created": "Wed, 2 Jan 2008 09:27:55 GMT"
},
{
"version": "v4",
"created": "Sun, 6 Jan 2008 08:53:20 GMT"
}
] | 2008-01-06T00:00:00 | [
[
"Xu",
"Yajie",
""
],
[
"Ma",
"Zhi",
""
],
[
"Zhang",
"Chunyuan",
""
],
[
"Lü",
"Xin",
""
]
] | [
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] |
712.3606 | Jiangyong Jia | Jiangyong Jia | Probe the QGP via dihadron correlations: Jet quenching and
Medium-response | Invited talk at International Symposium on Multiparticle Dynamics
(ISMD07), Berkeley, California, 4-9 Aug 2007. 5 pages 2 figures | Acta Phys.Polon.Supp.1:605-608,2008 | null | null | nucl-ex | null | We summarize the di-hadron correlation results from RHIC, focusing on the
high $p_T$ region and lower $p_T$ region for the away-side. The former is
consistent with fragmentation of jets that surviving the medium, while the
latter suggests the redistribution of the energy from the quenched jets. We
also discuss the role of the jet in the intermediate $p_T$.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 00:59:43 GMT"
}
] | 2009-01-16T00:00:00 | [
[
"Jia",
"Jiangyong",
""
]
] | [
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] |
712.3607 | Yuan Young | Yuan N. Young, Jerzy Blawzdziewicz, Vitorio Cristini, Roy Goodman | Hysteretic and chaotic dynamics of viscous drops in creeping flows with
rotation | 22 pages, 13 figures. submitted to Journal of Fluid Mechanics | null | 10.1017/S0022112008002036 | null | cond-mat.soft cond-mat.mtrl-sci | null | It has been shown in our previous publication
(Blawzdziewicz,Cristini,Loewenberg,2003) that high-viscosity drops in two
dimensional linear creeping flows with a nonzero vorticity component may have
two stable stationary states. One state corresponds to a nearly spherical,
compact drop stabilized primarily by rotation, and the other to an elongated
drop stabilized primarily by capillary forces. Here we explore consequences of
the drop bistability for the dynamics of highly viscous drops. Using both
boundary-integral simulations and small-deformation theory we show that a
quasi-static change of the flow vorticity gives rise to a hysteretic response
of the drop shape, with rapid changes between the compact and elongated
solutions at critical values of the vorticity. In flows with sinusoidal
temporal variation of the vorticity we find chaotic drop dynamics in response
to the periodic forcing. A cascade of period-doubling bifurcations is found to
be directly responsible for the transition to chaos. In random flows we obtain
a bimodal drop-length distribution. Some analogies with the dynamics of
macromolecules and vesicles are pointed out.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 01:02:19 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Young",
"Yuan N.",
""
],
[
"Blawzdziewicz",
"Jerzy",
""
],
[
"Cristini",
"Vitorio",
""
],
[
"Goodman",
"Roy",
""
]
] | [
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] |
712.3608 | M. Cristina Rabello-Soares | M.C. Rabello-Soares, S.G. Korzennik, J. Schou | Variations of the Solar Acoustic High-Degree Mode Frequencies over Solar
Cycle 23 | 7 figures. Advances in Space Research (2007) - in press | Adv.SpaceRes.41:861-867,2008 | 10.1016/j.asr.2007.03.014 | null | astro-ph | null | Using full-disk observations obtained with the Michelson Doppler Imager (MDI)
on board the Solar and Heliospheric Observatory (SOHO) spacecraft, we present
variations of the solar acoustic mode frequencies caused by the solar activity
cycle. High-degree (100 < l < 900) solar acoustic modes were analyzed using
global helioseismology analysis techniques over most of solar cycle 23. We
followed the methodology described in details in Korzennik, Rabello-Soares and
Schou (2004) to infer unbiased estimates of high-degree mode parameters (see
also Rabello-Soares, Korzennik and Schou, 2006). We have removed most of the
known instrumental and observational effects that affect specifically
high-degree modes. We show that the high-degree changes are in good agreement
with the medium-degree results, except for years when the instrument was highly
defocused. We analyzed and discuss the effect of defocusing on high degree
estimation. Our results for high-degree modes confirm that the frequency shift
scaled by the relative mode inertia is a function of frequency and it is
independent of degree.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 01:20:58 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Rabello-Soares",
"M. C.",
""
],
[
"Korzennik",
"S. G.",
""
],
[
"Schou",
"J.",
""
]
] | [
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712.3609 | Michael B. Mensky | Michael B. Mensky | Postcorrection and mathematical model of life in Extended Everett's
Concept | Comments: 24 pages, 1 figure, LaTeX, Journal URL:
http://www.neuroquantology.com | NeuroQuantology Vol 5, No 4, 363-376 (2007) | null | null | physics.gen-ph quant-ph | null | Extended Everett's Concept (EEC) recently developed by the author to explain
the phenomenon of consciousness is considered. A mathematical model is proposed
for the principal feature of consciousness assumed in EEC, namely its ability
(in the state of sleep, trance or meditation, when the explicit consciousness
is disabled) to obtain information from all alternative classical realities
(Everett's worlds) and select the favorable realities. To represent this
ability, a mathematical operation called postcorrection is introduced, which
corrects the present state to guarantee certain characteristics of the future
state. Evolution of living matter is thus determined by goals (first of all by
the goal of survival) as well as by causes. The resulting theory, in a way
symmetrical in time direction, follows from a sort of antropic principle.
Possible criteria for postcorrection and corresponding phenomena in the sphere
of life are classified. Both individual and collective criteria of survival are
considered as well as the criteria providing certain quality of life and those
which are irrelevant to the life quality. The phenomena of free will and direct
sighting of truth (e.g. scientific insight) are explained in these terms. The
problem of artificial intellect and the role of brain look differently in the
framework of this theory. Automats may perform intellectual operations, but not
postcorrection, therefore artificial intellect but not an artificial life can
be created. The brain serves as an interface between the body and
consciousness, but the most profound level of consciousness is not a function
of brain.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 14:18:21 GMT"
}
] | 2007-12-27T00:00:00 | [
[
"Mensky",
"Michael B.",
""
]
] | [
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] |
712.361 | Jindrich Kolorenc | Jindrich Kolorenc and Lubos Mitas | Quantum Monte Carlo calculations of structural properties of FeO under
pressure | 5 pages, 3 figures | Phys. Rev. Lett. 101, 185502 (2008) | 10.1103/PhysRevLett.101.185502 | null | cond-mat.mtrl-sci cond-mat.str-el | null | We determine the equation of state of stoichiometric FeO employing the
diffusion Monte Carlo method. The fermionic nodes are fixed to those of a wave
function having the form of a single Slater determinant. The calculated ambient
pressure properties (lattice constant, bulk modulus and cohesive energy) agree
very well with available experimental data. At approximately 65 GPa, the
lattice structure is found to change from rocksalt type (B1) to NiAs based
(inverse B8).
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 01:48:36 GMT"
}
] | 2008-10-29T00:00:00 | [
[
"Kolorenc",
"Jindrich",
""
],
[
"Mitas",
"Lubos",
""
]
] | [
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] |
712.3611 | Fran\c{c}ois Ghoulmi\'e Dr. | F. Ghoulmi\'e, M. Bartolozzi, C.P. Mellen, T. Di Matteo | Effects of diversification among assets in an agent-based market model | 12 pages, 5 figures, accepted for publication in the Proceedings of
the Complex Systems II Conference at the Australian National University, 4-7
December 2007, Canberra, ACT Australia | null | 10.1117/12.758912 | null | q-fin.TR physics.data-an physics.soc-ph | null | We extend to the multi-asset case the framework of a discrete time model of a
single asset financial market developed in Ghoulmie et al (2005). In
particular, we focus on adaptive agents with threshold behavior allocating
their resources among two assets. We explore numerically the effect of this
diversification as an additional source of complexity in the financial market
and we discuss its destabilizing role. We also point out the relevance of these
studies for financial decision making.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 02:05:20 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Ghoulmié",
"F.",
""
],
[
"Bartolozzi",
"M.",
""
],
[
"Mellen",
"C. P.",
""
],
[
"Di Matteo",
"T.",
""
]
] | [
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] |
712.3612 | Yasunori Mawatari | Yasunori Mawatari and Kazuhiro Kajikawa | Hysteretic ac loss of polygonally arranged superconducting strips
carrying ac transport current | 3 pages, 3 figures, to be published in Applied Physics Letters (2008) | null | 10.1063/1.2829793 | null | cond-mat.supr-con | null | The hysteretic ac loss of a current-carrying conductor in which multiple
superconducting strips are polygonally arranged around a cylindrical former is
theoretically investigated as a model of superconducting cables. Using the
critical state model, we analytically derive the ac loss $Q_n$ of a total of
$n$ strips. The normalized loss $Q_n/Q_1$ is determined by the number of strips
$n$ and the ratio of the strip width $2w$ to the diameter $2R$ of the
cylindrical former. When $n>> 1$ and $w/R<< 1$, the behavior of $Q_n$ is
similar to that of an infinite array of coplanar strips.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 02:19:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Mawatari",
"Yasunori",
""
],
[
"Kajikawa",
"Kazuhiro",
""
]
] | [
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] |
712.3613 | Stephen Serjeant | S. Serjeant, S. Dye, A. Mortier, J. Peacock, E. Egami, M. Cirasuolo,
G. Rieke, C. Borys, D. Clements, K. Coppin, J. Dunlop, S. Eales, D. Farrah,
M. Halpern, P. Mauskopf, A. Pope, M. Rowan-Robinson, D. Scott, I. Smail, M.
Vaccari | The SCUBA Half Degree Extragalactic Survey (SHADES) - IX: the
environment, mass and redshift dependence of star formation | Accepted by MNRAS. SMG environments analysis extended. 17 pages, 18
figures. Includes BoxedEPS | null | 10.1111/j.1365-2966.2008.13197.x | null | astro-ph | null | We present a comparison between the SCUBA Half Degree Extragalactic Survey
(SHADES) at 450 and 850 microns in the Lockman Hole East with a deep Spitzer
Space Telescope survey at 3.6-24 microns conducted in Guaranteed Time. Using
stacking analyses we demonstrate a striking correspondence between the galaxies
contributing the submm extragalactic background light, with those likely to
dominate the backgrounds at Spitzer wavelengths. Using a combination BRIzK plus
Spitzer photometric redshifts, we show that at least a third of the
Spitzer-identified submm galaxies at 1<z<1.5 appear to reside in overdensities
when the density field is smoothed at 0.5-2 Mpc comoving diameters, supporting
the high-redshift reversal of the local star formation - galaxy density
relation. We derive the dust-shrouded cosmic star formation history of galaxies
as a function of assembled stellar masses. For model stellar masses <10^11
Msun, this peaks at lower redshifts than the ostensible z~2.2 maximum for submm
point sources, adding to the growing consensus for ``downsizing'' in star
formation. Our surveys are also consistent with ``downsizing'' in mass
assembly. Both the mean star formation rates <dM/dt> and specific star
formation rates <(1/M)dM/dt> are in striking disagreement with some
semi-analytic predictions from the Millenium simulation. The discrepancy could
either be resolved with a top-heavy initial mass function, or a significant
component of the submm flux heated by the interstellar radiation field.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 14:29:20 GMT"
},
{
"version": "v2",
"created": "Wed, 5 Mar 2008 14:00:08 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Serjeant",
"S.",
""
],
[
"Dye",
"S.",
""
],
[
"Mortier",
"A.",
""
],
[
"Peacock",
"J.",
""
],
[
"Egami",
"E.",
""
],
[
"Cirasuolo",
"M.",
""
],
[
"Rieke",
"G.",
""
],
[
"Borys",
"C.",
""
],
[
"Clements",
"D.",
""
],
[
"Coppin",
"K.",
""
],
[
"Dunlop",
"J.",
""
],
[
"Eales",
"S.",
""
],
[
"Farrah",
"D.",
""
],
[
"Halpern",
"M.",
""
],
[
"Mauskopf",
"P.",
""
],
[
"Pope",
"A.",
""
],
[
"Rowan-Robinson",
"M.",
""
],
[
"Scott",
"D.",
""
],
[
"Smail",
"I.",
""
],
[
"Vaccari",
"M.",
""
]
] | [
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] |
712.3614 | Gregg Wade | G.A. Wade, J. Silvester, K. Bale, N. Johnson, J. Power, M. Auri\`ere,
F. Ligni\'eres, B. Dintrans, J.-F. Donati, A. Hui Bon Hoa, D. Mouillet, S.
Naseri, F. Paletou, P. Petit, F. Rincon, N. Toque, S. Bagnulo, C.P. Folsom,
J.D. Landstreet, M. Gruberbauer, T. Lueftinger, S. Jeffers, A. L\`ebre, S.
Marsden | Why are some A stars magnetic, while most are not? | 6 pages, 2 figures. Proceedings of Solar Polarisation Workshop #5 | null | null | null | astro-ph | null | A small fraction of intermediate-mass main sequence (A and B type) stars have
strong, organised magnetic fields. The large majority of such stars, however,
show no evidence for magnetic fields, even when observed with very high
precision. In this paper we describe a simple model, motivated by qualitatively
new observational results, that provides a natural physical explanation for the
small fraction of observed magnetic stars.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 02:27:36 GMT"
}
] | 2007-12-24T00:00:00 | [
[
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""
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"N.",
""
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[
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"J.",
""
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[
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"M.",
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[
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"F.",
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"B.",
""
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[
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"S.",
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] |
712.3615 | Kunihito Uzawa | Pierre Binetruy, Misao Sasaki, Kunihito Uzawa | Dynamical D4-D8 and D3-D7 branes in supergravity | 25 pages, no figure, typos corrected, references and discussions of
D3-D7 brane solutions added | Phys.Rev.D80:026001,2009 | 10.1103/PhysRevD.80.026001 | null | hep-th gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present a class of dynamical solutions for intersecting D4-D8 and D3-D7
brane systems in ten-dimensional type IIA and IIB supergravity. We discuss if
these solutions can be recovered in lower-dimensional effective theories for
the warped compactification of a general p-brane system. It is found that an
effective $p+1$-dimensional description is not possible in general due to the
entanglement of the transverse coordinates and the $p+1$-dimensional
coordinates in the metric components. For the D4-D8 brane system, the dynamical
solutions reduces to a static warped ${\rm AdS_6}\times {\rm S}^4$ geometry in
a certain spacetime region. For the D3-D7 brane system, we find a dynamical
solution whose metric form is similar to that of a D3-brane solution. The main
difference is the existence of a nontrivial dilaton configuration in the D3-D7
solution. Then we discuss cosmology of these solutions. We find that they
behave like a Kasner-type cosmological solution at $\tau\to\infty$, while it
reduces to a warped static solution at $\tau\to0$, where $\tau$ is the cosmic
time.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 02:53:30 GMT"
},
{
"version": "v2",
"created": "Tue, 7 Jul 2009 08:42:45 GMT"
}
] | 2009-09-29T00:00:00 | [
[
"Binetruy",
"Pierre",
""
],
[
"Sasaki",
"Misao",
""
],
[
"Uzawa",
"Kunihito",
""
]
] | [
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712.3616 | Ki-Myeong Lee | Jens Hoppe (KTH, Sweden) and Ki-Myeong Lee (KIAS, Korea) | New BPS Configurations of BMN Matrix Theory | 19 pages, No Figurers, JHEP stype | JHEP 0806:041,2008 | 10.1088/1126-6708/2008/06/041 | KIAS-P007075 | hep-th | null | We explore the 1/2 BPS configurations in BMN matrix theory with SO(3) angular
momentum of $SO(3)\times SO(6)$ symmetry. The fluctuation analysis of the BPS
configurations near the abelian solutions and also the fuzzy two sphere vacua
reveals how nonabelian BPS configurations emerge. Especially the irreducible
nonabelian configurations seem to have the maximal angular momentum of order
$N^3$, beyond which they collapse to abelian ones. We also find some new BPS
configurations explicitly.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 02:43:31 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Hoppe",
"Jens",
"",
"KTH, Sweden"
],
[
"Lee",
"Ki-Myeong",
"",
"KIAS, Korea"
]
] | [
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] |
712.3617 | Erhan Bayraktar | Erhan Bayraktar, Bo Yang | A Unified Framework for Pricing Credit and Equity Derivatives | Keywords: Credit Default Swap, Defaultable Bond, Defaultable Stock,
Equity Options, Stochastic Interest Rate, Implied Volatility, Multiscale
Perturbation Method | null | null | null | cs.CE | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We propose a model which can be jointly calibrated to the corporate bond term
structure and equity option volatility surface of the same company. Our purpose
is to obtain explicit bond and equity option pricing formulas that can be
calibrated to find a risk neutral model that matches a set of observed market
prices. This risk neutral model can then be used to price more exotic, illiquid
or over-the-counter derivatives. We observe that the model implied credit
default swap (CDS) spread matches the market CDS spread and that our model
produces a very desirable CDS spread term structure. This is observation is
worth noticing since without calibrating any parameter to the CDS spread data,
it is matched by the CDS spread that our model generates using the available
information from the equity options and corporate bond markets. We also observe
that our model matches the equity option implied volatility surface well since
we properly account for the default risk premium in the implied volatility
surface. We demonstrate the importance of accounting for the default risk and
stochastic interest rate in equity option pricing by comparing our results to
Fouque, Papanicolaou, Sircar and Solna (2003), which only accounts for
stochastic volatility.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 02:53:38 GMT"
},
{
"version": "v2",
"created": "Sat, 20 Sep 2008 21:44:00 GMT"
}
] | 2008-09-21T00:00:00 | [
[
"Bayraktar",
"Erhan",
""
],
[
"Yang",
"Bo",
""
]
] | [
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] |
712.3618 | Aiyou Chen | Aiyou Chen, Jin Cao, and Tian Bu | Network Tomography: Identifiability and Fourier Domain Estimation | 21 pages | IEEE INFOCOM 2007, p.1875-1883 | 10.1109/INFCOM.2007.218 | null | stat.ME math.ST stat.AP stat.CO stat.TH | null | The statistical problem for network tomography is to infer the distribution
of $\mathbf{X}$, with mutually independent components, from a measurement model
$\mathbf{Y}=A\mathbf{X}$, where $A$ is a given binary matrix representing the
routing topology of a network under consideration. The challenge is that the
dimension of $\mathbf{X}$ is much larger than that of $\mathbf{Y}$ and thus the
problem is often called ill-posed. This paper studies some statistical aspects
of network tomography. We first address the identifiability issue and prove
that the $\mathbf{X}$ distribution is identifiable up to a shift parameter
under mild conditions. We then use a mixture model of characteristic functions
to derive a fast algorithm for estimating the distribution of $\mathbf{X}$
based on the General method of Moments. Through extensive model simulation and
real Internet trace driven simulation, the proposed approach is shown to be
favorable comparing to previous methods using simple discretization for
inferring link delays in a heterogeneous network.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 03:47:28 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Chen",
"Aiyou",
""
],
[
"Cao",
"Jin",
""
],
[
"Bu",
"Tian",
""
]
] | [
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] |
712.3619 | Fuming Liu | Fu-Ming Liu, Klaus Werner | A Systematic Study on Direct Photon Production from Central Heavy Ion
Collisions | 13 pages 19 figures | J.Phys.G36:035101,2009 | 10.1088/0954-3899/36/3/035101 | null | hep-ph | null | We investigate the production of direct photons in central Au-Au collisions
at the relativistic Heavy-Ion Collider (RHIC) at 200 GeV per nucleon,
considering all possible sources. We treat thermal photons emitted from a
quark-gluon plasma and from a hadron gas, based on a realistic thermodynamic
expansion. Hard photons from elementary nucleon-nucleon scatterings are
included: primordial elementary scatterings are certainly dominant at large
transverse momenta, but also secondary photons from jet fragmentation and
jet-photon conversion cannot be ignored. In both cases we study the effect of
energy loss, and we also consider photons emitted from bremsstrahlung gluons
via fragmentation.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 04:05:50 GMT"
},
{
"version": "v2",
"created": "Sat, 29 Dec 2007 13:16:16 GMT"
}
] | 2009-02-02T00:00:00 | [
[
"Liu",
"Fu-Ming",
""
],
[
"Werner",
"Klaus",
""
]
] | [
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] |
712.362 | Joshua Combes | Joshua Combes and Howard M. Wiseman, Kurt Jacobs | Rapid Measurement of Quantum Systems using Feedback Control | 4 pages, 4 figures. V2: Minor corrections | Phys. Rev. Lett. 100, 160503 (2008) | 10.1103/PhysRevLett.100.160503 | null | quant-ph math.OC | null | We introduce a feedback control algorithm that increases the speed at which a
measurement extracts information about a $d$-dimensional system by a factor
that scales as $d^2$. Generalizing this algorithm, we apply it to a register of
$n$ qubits and show an improvement O(n). We derive analytical bounds on the
benefit provided by the feedback and perform simulations that confirm that this
speedup is achieved.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 06:52:33 GMT"
},
{
"version": "v2",
"created": "Tue, 29 Apr 2008 04:41:07 GMT"
}
] | 2009-08-15T00:00:00 | [
[
"Combes",
"Joshua",
""
],
[
"Wiseman",
"Howard M.",
""
],
[
"Jacobs",
"Kurt",
""
]
] | [
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] |
712.3621 | Vladimir Dzuba | V. A. Dzuba and V. V. Flambaum | Relativistic corrections to transition frequencies of Ag I, Dy I, Ho I,
Yb II, Yb III, Au I and Hg II and search for variation of the fine structure
constant | 6 pages, 5 tables | Phys. Rev. A, 77, 012515 (2008) | 10.1103/PhysRevA.77.012515 | null | physics.atom-ph | null | Dependence of transition frequencies on the fine structure constant
$\alpha=e^2/\hbar c$ is calculated for several many-electron systems which are
used or planned to be used in the laboratory search for the time variation of
the fine structure constant. In systems with a large number of electrons in
open shells (from 11 to 15) the relative effects of the variation may be
strongly enhanced. For the transitions which were considered before the results
are in good agreement with previous calculations.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 04:44:38 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dzuba",
"V. A.",
""
],
[
"Flambaum",
"V. V.",
""
]
] | [
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] |
712.3622 | Sungchul Kwon | Dong-Jin Lee, Sungchul Kwon, and Yup Kim | Conserved mass aggregation model with mass-dependent fragmentation | 4 pages, 2 figures, to be appeared in J. Korean Phys. Soc. (2008) | null | 10.3938/jkps.52.154 | null | cond-mat.stat-mech | null | We study a conserved mass aggregation model with mass-dependent fragmentation
in one dimension. In the model, the whole mass $m$ of a site isotropically
diffuse with unit rate. With rate $\omega$, a mass $m^{\lambda}$ is fragmented
from the site and moves to a randomly selected nearest neighbor site. Since the
fragmented mass is smaller than the whole mass $m$ of a site for $\lambda < 1$,
the on-site attractive interaction exists for the case. For $\lambda = 0$, the
model is known to undergo the condensation phase transitions from a fluid phase
into a condensed phase as the density of total masses ($\rho$) increases beyond
a critical density $\rho_c$. For $0< \lambda <1$, we numerically confirm for
several values of $\omega$ that $\rho_c$ diverges with the system size $L$.
Hence in thermodynamic limit, the condensed phase disappears and no transitions
take place in one dimension. We also explain that there are no transitions in
any dimensions.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 04:44:20 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Lee",
"Dong-Jin",
""
],
[
"Kwon",
"Sungchul",
""
],
[
"Kim",
"Yup",
""
]
] | [
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] |
712.3623 | Ping Zhang | Bo Sun, Ping Zhang, Xian-Geng Zhao | First-principles LDA+U and GGA+U study of plutonium oxides | To appear in J. Chem. Phys | null | null | null | cond-mat.mtrl-sci cond-mat.str-el | null | The electronic structure and properties of PuO$_{2}$ and Pu$_{2}$O$_{3}$ have
been studied from first principles by the all-electron projector-augmented-wave
(PAW) method. The local density approximation (LDA)+$U$ and the generalized
gradient approximation (GGA)+$U$ formalism have been used to account for the
strong on-site Coulomb repulsion among the localized Pu $5f$ electrons. We
discuss how the properties of PuO$_{2}$ and Pu$_{2}$O$_{3}$ are affected by the
choice of $U$ as well as the choice of exchange-correlation potential. Also,
oxidation reaction of Pu$_{2}$O$_{3}$, leading to formation of PuO$_{2}$, and
its dependence on $U$ and exchange-correlation potential have been studied. Our
results show that by choosing an appropriate $U$ it is promising to correctly
and consistently describe structural, electronic, and thermodynamic properties
of PuO$_{2}$ and Pu$_{2}$O$_{3}$, which enables it possible the modeling of
redox process involving Pu-based materials.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 05:24:41 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Sun",
"Bo",
""
],
[
"Zhang",
"Ping",
""
],
[
"Zhao",
"Xian-Geng",
""
]
] | [
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] |
712.3624 | U. Zuelicke | D. Csontos, U. Zuelicke (Massey University) | Tailoring hole spin splitting and polarization in nanowires | 3.1 pages, 4 figures, RevTex4, to appear in APL | Appl. Phys. Lett. 92, 023108 (2008) | 10.1063/1.2834702 | null | cond-mat.mes-hall | null | Spin splitting in p-type semiconductor nanowires is strongly affected by the
interplay between quantum confinement and spin-orbit coupling in the valence
band. The latter's particular importance is revealed in our systematic
theoretical study presented here, which has mapped the range of spin-orbit
coupling strengths realized in typical semiconductors. Large controllable
variations of the g-factor with associated characteristic spin polarization are
shown to exist for nanowire subband edges, which therefore turn out to be a
versatile laboratory for investigating the complex spin properties exhibited by
quantum-confined holes.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 05:45:57 GMT"
}
] | 2008-01-16T00:00:00 | [
[
"Csontos",
"D.",
"",
"Massey University"
],
[
"Zuelicke",
"U.",
"",
"Massey University"
]
] | [
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] |
712.3625 | K. Narayan | K. Narayan | On the internal structure of dyons in ${\cal N}=4$ super Yang-Mills
theories | Latex, 29 pgs, 5 eps figures; v2: typos fixed, minor clarifications
on internal faces | Phys.Rev.D77:046004,2008 | 10.1103/PhysRevD.77.046004 | null | hep-th | null | We use the low energy effective $U(1)^r$ action on the Coulomb branch of
${\cal N}=4$ super Yang-Mills theory to construct approximate field
configurations for solitonic dyons in these theories, building on the brane
prong description developed in hep-th/0101114. This dovetails closely with the
corresponding description of these dyons as string webs stretched between
D-branes in the transverse space. The resulting picture within these
approximations shows the internal structure of these dyons (for fixed
asymptotic charges) to be molecule-like, with multiple charge cores held
together at equilibrium separations, which grow large near lines of marginal
stability. Although these techniques do not yield a complete solution for the
spatial structure (i.e. all core sizes and separations) of large charge
multicenter dyons in high rank gauge theories, approximate configurations can
be found in specific regions of moduli space, which become increasingly
accurate near lines of marginal stability. We also discuss string webs with
internal faces from this point of view.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 07:46:39 GMT"
},
{
"version": "v2",
"created": "Fri, 28 Dec 2007 06:51:04 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Narayan",
"K.",
""
]
] | [
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] |
712.3626 | Jiang Qian | Jiang Qian, Pabitra N. Sen | Time dependent diffusion in a disordered medium with partially absorbing
walls: A perturbative approach | null | Journal of Chemical Physics, vol. 125, 194508, 2008 | 10.1063/1.2372497 | null | cond-mat.stat-mech cond-mat.dis-nn | null | We present an analytical study of the time dependent diffusion coefficient in
a dilute suspension of spheres with partially absorbing boundary condition.
Following Kirkpatrick (J. Chem. Phys. 76, 4255) we obtain a perturbative
expansion for the time dependent particle density using volume fraction $f$ of
spheres as an expansion parameter. The exact single particle $t$-operator for
partially absorbing boundary condition is used to obtain a closed form
time-dependent diffusion coefficient $D(t)$ accurate to first order in the
volume fraction $f$. Short and long time limits of $D(t)$ are checked against
the known short-time results for partially or fully absorbing boundary
conditions and long-time results for reflecting boundary conditions. For fully
absorbing boundary condition the long time diffusion coefficient is found to be
$D(t)=5 a^2/(12 f D_{0} t) +O((D_0t/a^2)^{-2})$, to the first order of
perturbation theory. Here $f$ is small but non-zero, $D_0$ the diffusion
coefficient in the absence of spheres, and $a$ the radius of the spheres. The
validity of this perturbative result is discussed.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 05:54:45 GMT"
}
] | 2012-10-29T00:00:00 | [
[
"Qian",
"Jiang",
""
],
[
"Sen",
"Pabitra N.",
""
]
] | [
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712.3627 | Ailin Zhang | Ailin Zhang | Exotica possibility of new observations by BES | 8 pages, talk given at XII International Conference on Hadron
Spectroscopy(Hadron 07), Frascati, Rome, 8-13 October, 2007 | null | null | null | hep-ph | null | The employment of interpolating currents of existed studies of four-quark
state and glueball with QCD sum rule approach is analyzed. In terms of suitable
currents, the masses of the lowest lying scalar and pseudo-scalar glueball were
determined. The masses of some tetraquark states and their first orbital
excitations were obtained through a combination of the sum rule with the
constituent quark model. Exotica possibility of the new observations by BES is
discussed.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 06:42:04 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Zhang",
"Ailin",
""
]
] | [
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] |
712.3628 | Andreas Winter | Toby Cubitt, Aram W. Harrow, Debbie Leung, Ashley Montanaro, Andreas
Winter | Counterexamples to additivity of minimum output p-Renyi entropy for p
close to 0 | 7 pages, revtex4; v2 added correct ref. [15]; v3 has more information
on the numerical violation as well as 1 figure (2 graphs) - note that the
explicit example was changed and the more conservative estimate of the bound
up to which violations occur, additionally some other small issues are
straightened out | Communications in Mathematical Physics, volume 284, p281-290
(2008) | 10.1007/s00220-008-0625-z | null | quant-ph | null | Complementing recent progress on the additivity conjecture of quantum
information theory, showing that the minimum output p-Renyi entropies of
channels are not generally additive for p>1, we demonstrate here by a careful
random selection argument that also at p=0, and consequently for sufficiently
small p, there exist counterexamples.
An explicit construction of two channels from 4 to 3 dimensions is given,
which have non-multiplicative minimum output rank; for this pair of channels,
numerics strongly suggest that the p-Renyi entropy is non-additive for all p <
0.11. We conjecture however that violations of additivity exist for all p<1.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 06:47:47 GMT"
},
{
"version": "v2",
"created": "Sat, 22 Dec 2007 05:06:11 GMT"
},
{
"version": "v3",
"created": "Thu, 14 Feb 2008 22:43:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Cubitt",
"Toby",
""
],
[
"Harrow",
"Aram W.",
""
],
[
"Leung",
"Debbie",
""
],
[
"Montanaro",
"Ashley",
""
],
[
"Winter",
"Andreas",
""
]
] | [
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] |
712.3629 | Masao Jinzenji | Masao Jinzenji (Hokkaido University) | Virtual Structure Constants as Intersection Numbers of Moduli Space of
Polynomial Maps with Two Marked Points | 10 pages, latex, a minor change in Section 4, English is refined,
Some typing errors in Section 3 are corrected | Letters in Mathematical Physics, Vol.86, No.2-3, 99-114 (2008) | 10.1007/s11005-008-0278-z | null | math.AG hep-th | null | In this paper, we derive the virtual structure constants used in mirror
computation of degree k hypersurface in CP^{N-1}, by using localization
computation applied to moduli space of polynomial maps from CP^{1} to CP^{N-1}
with two marked points. We also apply this technique to non-nef local geometry
O(1)+O(-3)->CP^{1} and realize mirror computation without using Birkhoff
factorization.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 06:55:49 GMT"
},
{
"version": "v2",
"created": "Wed, 16 Jan 2008 07:47:45 GMT"
},
{
"version": "v3",
"created": "Thu, 17 Jan 2008 06:35:40 GMT"
}
] | 2008-12-04T00:00:00 | [
[
"Jinzenji",
"Masao",
"",
"Hokkaido University"
]
] | [
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712.363 | Sven Heinemeyer | S. Heinemeyer, M. Mondragon, G. Zoupanos | Confronting Finite Unified Theories with Low-Energy Phenomenology | 25 pages, 8 figures. Discussion on models and on cold dark matter
constraint extended, references added. Version to appear in JHEP | JHEP 0807:135,2008 | 10.1088/1126-6708/2008/07/135 | null | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Finite Unified Theories (FUTs) are N=1 supersymmetric Grand Unified
Theories that can be made all-loop finite. The requirement of all-loop
finiteness leads to a severe reduction of the free parameters of the theory
and, in turn, to a large number of predictions. FUTs are investigated in the
context of low-energy phenomenology observables. We present a detailed scanning
of the all-loop finite SU(5) FUTs, where we include the theoretical
uncertainties at the unification scale and we apply several phenomenological
constraints. Taking into account the restrictions from the top and bottom quark
masses, we can discriminate between different models. Including further
low-energy constraints such as B physics observables, the bound on the lightest
Higgs boson mass and the cold dark matter density, we determine the predictions
of the allowed parameter space for the Higgs boson sector and the
supersymmetric particle spectrum of the selected model.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 07:37:58 GMT"
},
{
"version": "v2",
"created": "Tue, 29 Jul 2008 08:31:56 GMT"
}
] | 2009-01-06T00:00:00 | [
[
"Heinemeyer",
"S.",
""
],
[
"Mondragon",
"M.",
""
],
[
"Zoupanos",
"G.",
""
]
] | [
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712.3631 | Rabin Banerjee | Rabin Banerjee, Subir Ghosh and T. Shreecharan | Three dimensional noncommutative bosonization | LaTex, 9 pages, no figures | Phys.Lett.B662:231-236,2008 | 10.1016/j.physletb.2008.02.043 | null | hep-th | null | We consider the extension of the 2+1-dimensional bosonization process in
Non-Commutative (NC) spacetime. We show that the large mass limit of the
effective action obtained by integrating out the fermionic fields in NC
spacetime leads to the NC Chern-Simons action. The present result is valid to
all orders in the noncommutative parameter $\theta$. We also discuss how the NC
Yang-Mills action is induced in the next to leading order.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 07:45:40 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Banerjee",
"Rabin",
""
],
[
"Ghosh",
"Subir",
""
],
[
"Shreecharan",
"T.",
""
]
] | [
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712.3632 | P. F. Chen | P. F. Chen | Initiation and propagation of coronal mass ejections | 8 pages, 1 figure, an invited review, to appear in J. Astrophys.
Astron | null | 10.1007/s12036-008-0023-0 | null | astro-ph | null | This paper reviews recent progress in the research on the initiation and
propagation of CMEs. In the initiation part, several trigger mechanisms are
discussed; In the propagation part, the observations and modelings of EIT
waves/dimmings, as the EUV counterparts of CMEs, are described.
| [
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712.3633 | Hannes Jung | J. Bartels (Univ. Hamburg), K. Borras (DESY), M. Diehl (DESY) and H.
Jung (DESY), H. Abramowicz, J. Albacete, L. Alvarez-Gaume, J. Alvarez-Muniz,
R D. Ball, J. Bartels, K. Belov, J. Bluemer, J. Bluemlein, A. Bonato, M.
Braun, P. Brogueira, G. C Trinchero, R. Conceicao, J-R. Cudell, J Dainton, A.
De Roeck, M. Deile, J. Dias de Deus, R. Engel, M C. Espirito Santo, C. Ewerz,
R. Fabbri, V. Fadin, P. Falgari, L. Fan\`o, E. Ferreira, J Forshaw, S. Forte,
L. Frankfurt, H. G Dosch, C. Gomez, K. Golec-Biernat, S. Goloskokov, K.
Goulianos, G. Gustafson, A. Hamilton, C E. Hyde, M. Islam, D. Ivanov, R. J
Luddy, L. Jenkovsky, J. Kaspar, A. Kaidalov, O. Kepka, V. Khoze, M. Klein, B
Z. Kopeliovich, A. Kovner, H. Kowalski, M. Kozlov, J. Kretzschmar, K.
Kumericki, V. Kundrat, P. L Iafelice, P. Laycock, A. Lengyel, E. Levin, A.
Levy, L. Lipatov, M. Lokajicek, J. Londergan, A. Luszczak, V L. Lyuboshitz,
D. Mueller, A D. Martin, E. Martynov, S. Marzani, E. Meggiolaro, S. Munier,
O. Nachtmann, T. Namsoo, P. Newman, B. Nicolescu, J. Nystrand, K.
Passek-Kumericki, T. Pierog, A. Pilkington, M. Pimenta, B. Pire, B Povh, D.
Roehrich, C. Royon, M G. Ryskin, A. Sabio Vera, M. Salvadore, C. Sbarra, F.
Schuessler, R. Schicker, I. Schmidt, L. Schoeffel, F. Schwennsen, M. Segond,
O V. Selyugin, M. Seymour, A. Shoshi, A. Stasto, M. Strikman, B. Surrow, A P.
Szczepaniak, A. Szczurek, L. Szymanowski, M. Tasevsky, A. Tavanfar, M.
Togawa, A. Tricomi, R. Ulrich, M. Unger, V. V Lyuboshitz, M A. Vazquez-Mozo,
G P. Vacca, A. von Manteuffel, M I. Vyazovsky, S. Wallon, G. Watt, C. Weiss,
K. Werner, B W. Xiao | 12th International Conference on Elastic and Diffractive Scattering
(Blois Workshop) - Forward Physics and QCD | Proceedings of the 12th International Conference on Elastic and
Diffractive Scattering (Blois Workshop) - Forward Physics and QCD, 549 pages
replaced to include list of conveners | null | null | DESY-PROC-2007-02 | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Proceedings of the 12th International Conference on Elastic and Diffractive
Scattering (Blois Workshop) - Forward Physics and QCD
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] |
712.3634 | Simon Gustavsson | S. Gustavsson, I. Shorubalko, R. Leturcq, S. Sch\"on, K. Ensslin | Measuring current by counting electrons in a nanowire quantum dot | null | Appl. Phys. Lett. 92, 152101 (2008) | 10.1063/1.2892679 | null | cond-mat.mes-hall | null | We measure current by counting single electrons tunneling through an InAs
nanowire quantum dot. The charge detector is realized by fabricating a quantum
point contact in close vicinity to the nanowire. The results based on electron
counting compare well to a direct measurements of the quantum dot current, when
taking the finite bandwidth of the detector into account. The ability to detect
single electrons also opens up possibilities for manipulating and detecting
individual spins in nanowire quantum dots.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 07:51:37 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Gustavsson",
"S.",
""
],
[
"Shorubalko",
"I.",
""
],
[
"Leturcq",
"R.",
""
],
[
"Schön",
"S.",
""
],
[
"Ensslin",
"K.",
""
]
] | [
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712.3635 | Rainer Avikainen | Rainer Avikainen | Convergence Rates for Approximations of Functionals of SDEs | 30 pages | null | null | null | math.PR | null | We consider upper bounds for the approximation error E|g(X)-g(\hat X)|^p,
where X and \hat X are random variables such that \hat X is an approximation of
X in the L_p-norm, and the function g belongs to certain function classes,
which contain e.g. functions of bounded variation. We apply the results to the
approximations of a solution of a stochastic differential equation at time T by
the Euler and Milstein schemes. For the Euler scheme we provide also a lower
bound.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 07:51:40 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Avikainen",
"Rainer",
""
]
] | [
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] |
712.3636 | Francois Hild | Olivier Arnould (LMT), Fran\c{c}ois Hild (LMT) | On the measurement by EDX of diffusion profiles of Ni/Cu assemblies | null | Microscopy and Analysis European Edition (2000) 13-15 | null | null | physics.class-ph | null | To characterise (inter)diffusion in materials, concentration profiles can be
measured by EDX. It allows one to determine the chemical composition with a
very good accuracy if measurement artefacts are accounted for. Standard
phenomena (such as X-ray fluorescence) are usually corrected by commercial
software. However, the effect of the pear-shaped volume of X-ray emission on
the concentration profiles has to be considered. The paper describes the origin
of this artefact, its consequences on measurements and will provide a practical
solution (based on signal processing methods) to deconvolute the actual
concentration profiles (or the diffusion coefficient) from the raw
measurements.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 07:55:26 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Arnould",
"Olivier",
"",
"LMT"
],
[
"Hild",
"François",
"",
"LMT"
]
] | [
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] |
712.3637 | Toshiyuki Miyauchi | Norio Iwase, Kai Kikuchi and Toshiyuki Miyauchi | On Lusternik-Schnirelmann category of SO(10) | 28 pages, 4 figures | null | null | null | math.AT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Let $G$ be a compact connected Lie group and $p : E\to \Sigma A$ be a
principal G-bundle with a characteristic map $\alpha : A\to G$, where $A=\Sigma
A_{0}$ for some $A_{0}$. Let $\{K_{i}{\to} F_{i-1}{\hookrightarrow} F_{i} \,|\,
1{\le} i {\le} n,\, F_{0}{=} \{\ast\} \; F_{1}{=} \Sigma{K_{1}} \; \text{and}\;
F_{n}{\simeq} G \}$ be a cone-decomposition of $G$ of length $m$ and
$F'_{1}=\Sigma{K'_{1}} \subset F_{1}$ with $K'_{1} \subset K_{1}$ which satisfy
$F_{i}F'_{1} \subset F_{i+1}$ up to homotopy for any $i$. Our main result is as
follows: we have $\operatorname{cat}(X) \le m{+}1$, if firstly the
characteristic map $\alpha$ is compressible into $F'_{1}$, secondly the
Berstein-Hilton Hopf invariant $H_{1}(\alpha)$ vanishes in $[A, \Omega
F'_1{\ast}\Omega F'_1]$ and thirdly $K_{m}$ is a sphere. We apply this to the
principal bundle $\mathrm{SO}(9)\hookrightarrow\mathrm{SO}(10)\to S^{9}$ to
determine L-S category of $\mathrm{SO}(10)$.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 07:56:11 GMT"
},
{
"version": "v2",
"created": "Sun, 30 Dec 2012 13:13:38 GMT"
},
{
"version": "v3",
"created": "Wed, 30 Oct 2013 02:08:11 GMT"
}
] | 2015-03-13T00:00:00 | [
[
"Iwase",
"Norio",
""
],
[
"Kikuchi",
"Kai",
""
],
[
"Miyauchi",
"Toshiyuki",
""
]
] | [
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712.3638 | Jean-Baptiste Gouere | Jean-Baptiste Gou\'er\'e (MAPMO) | Subcritical regimes in some models of continuum percolation | Published in at http://dx.doi.org/10.1214/08-AAP575 the Annals of
Applied Probability (http://www.imstat.org/aap/) by the Institute of
Mathematical Statistics (http://www.imstat.org) | null | null | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider some continuum percolation models. We are mainly interested in
giving some sufficient conditions for absence of percolation. We give some
general conditions and then focuse on two examples. The first one is a
multiscale percolation model based on the Boolean model. It was introduced by
Meester and Roy and subsequently studied by Menshikov, Popov and Vachkovskaia.
The second one is based on the stable marriage of Poisson and Lebesgue
introduced by Hoffman, Holroyd and Peres and whose percolation properties have
been studied by Freire, Popov and Vachkovskaia.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 07:57:39 GMT"
},
{
"version": "v2",
"created": "Wed, 2 Apr 2008 16:55:43 GMT"
},
{
"version": "v3",
"created": "Mon, 28 Sep 2009 06:48:19 GMT"
}
] | 2009-09-28T00:00:00 | [
[
"Gouéré",
"Jean-Baptiste",
"",
"MAPMO"
]
] | [
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] |
712.3639 | Jean-Sebastien Lauret | G. Magadur (LPQM, PPSM), Jean-S\'ebastien Lauret (LPQM), V.
Alain-Rizzo (PPSM), C. Voisin (LPA), Ph. Roussignol (LPA), E. Deleporte
(LPQM), J.A. Delaire (PPSM) | Excitation transfer and luminescence in porphyrin-carbon nanotube
complexes | null | null | null | null | physics.optics | null | Functionalization of carbon nanotubes with hydrosoluble porphyrins (TPPS) is
achieved by "$\pi$-stacking". The porphyrin/nanotube interaction is studied by
means of optical absorption, photoluminescence and photoluminescence excitation
spectroscopies. The main absorption line of the porphyrins adsorbed on
nanotubes exhibits a 120 meV red shift, which we ascribe to a flattening of the
molecule in order to optimize $\pi-\pi$ interactions. The porphyrin-nanotube
complex shows a strong quenching of the TPPS emission while the
photoluminescence intensity of the nanotubes is enhanced when the excitation
laser is in resonance with the porphyrin absorption band. This reveals an
efficient excitation transfer from the TPPS to the carbon nanotube.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 08:02:46 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Magadur",
"G.",
"",
"LPQM, PPSM"
],
[
"Lauret",
"Jean-Sébastien",
"",
"LPQM"
],
[
"Alain-Rizzo",
"V.",
"",
"PPSM"
],
[
"Voisin",
"C.",
"",
"LPA"
],
[
"Roussignol",
"Ph.",
"",
"LPA"
],
[
"Deleporte",
"E.",
"",
"LPQM"
],
[
"Delaire",
"J. A.",
"",
"PPSM"
]
] | [
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] |
712.364 | Dmitriy Moskovkin | D.L. Moskovkin, V.M. Shabaev, and W. Quint | Zeeman effect of the hyperfine structure levels in lithiumlike ions | 25 pages, 5 figures | Phys. Rev. A 77, 063421 (2008) | 10.1103/PhysRevA.77.063421 | null | physics.atom-ph physics.optics | null | The fully relativistic theory of the Zeeman splitting of the $(1s)^2 2s$
hyperfine-structure levels in lithiumlike ions with $Z=6 - 32$ is considered
for the magnetic field magnitude in the range from 1 to 10 T. The second-order
corrections to the Breit -- Rabi formula are calculated and discussed including
the one-electron contributions as well as the interelectronic-interaction
effects of order 1/Z. The 1/Z corrections are evaluated within a rigorous QED
approach. These corrections are combined with other
interelectronic-interaction, QED, nuclear recoil, and nuclear size corrections
to obtain high-precision theoretical values for the Zeeman splitting in Li-like
ions with nonzero nuclear spin. The results can be used for a precise
determination of nuclear magnetic moments from $g$-factor experiments.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 08:13:19 GMT"
}
] | 2009-04-08T00:00:00 | [
[
"Moskovkin",
"D. L.",
""
],
[
"Shabaev",
"V. M.",
""
],
[
"Quint",
"W.",
""
]
] | [
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] |
712.3641 | Dawei Ding | Dawei Ding, Jie Zhu, Xiaoshu Luo, Yuliang Liu | Controlling Delay-induced Hopf bifurcation in Internet congestion
control system | 20 pages, 8 figures | null | null | null | cs.NI | null | This paper focuses on Hopf bifurcation control in a dual model of Internet
congestion control algorithms which is modeled as a delay differential equation
(DDE). By choosing communication delay as a bifurcation parameter, it has been
demonstrated that the system loses stability and a Hopf bifurcation occurs when
communication delay passes through a critical value. Therefore, a time-delayed
feedback control method is applied to the system for delaying the onset of
undesirable Hopf bifurcation. Theoretical analysis and numerical simulations
confirm that the delayed feedback controller is efficient in controlling Hopf
bifurcation in Internet congestion control system. Moreover, the direction of
the Hopf bifurcation and the stability of the bifurcating periodic solutions
are determinated by applying the center manifold theorem and the normal form
theory.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 08:30:23 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Ding",
"Dawei",
""
],
[
"Zhu",
"Jie",
""
],
[
"Luo",
"Xiaoshu",
""
],
[
"Liu",
"Yuliang",
""
]
] | [
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] |
712.3642 | Fang Xia | Fang Xia, Shulin Ren and Yanning Fu | The Empirical Mass-Luminosity Relation for Low Mass Stars | 8 pages, 2 figures. Accepted for publication in Astrophysics & Space
Science | Astrophys.SpaceSci.314:51-58,2008 | 10.1007/s10509-007-9729-8 | null | astro-ph | null | This work is devoted to improving empirical mass-luminosity relations and
mass-metallicity-luminosity relation for low mass stars. For these stars,
observational data in the mass-luminosity plane or the
mass-metallicity-luminosity space subject to non-negligible errors in all
coordinates with different dimensions. Thus a reasonable weight assigning
scheme is needed for obtaining more reliable results. Such a scheme is
developed, with which each data point can have its own due contribution.
Previous studies have shown that there exists a plateau feature in the
mass-luminosity relation. Taking into account the constraints from the
observational luminosity function, we find by fitting the observational data
using our weight assigning scheme that the plateau spans from 0.28 to 0.50
solar mass. Three-piecewise continuous improved mass-luminosity relations in K,
J, H and V bands, respectively, are obtained. The visual
mass-metallicity-luminosity relation is also improved based on our K band
mass-luminosity relation and the available observational metallicity data.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 08:48:34 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Xia",
"Fang",
""
],
[
"Ren",
"Shulin",
""
],
[
"Fu",
"Yanning",
""
]
] | [
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] |
712.3643 | Shih-Yuin Lin | B. L. Hu and Shih-Yuin Lin | Black Hole Information in a Detector (Atom) - Field Analog | 13 pages, 4 figures; Invited plenary talk at the workshop ``From
Quantum to Emergent Gravity: Theory and Phenomenology", Trieste, Italy, June
11-15, 2007 | PoS QG-Ph:019,2007 | null | null | gr-qc | null | This is a synopsis of our recent work on quantum entanglement, recoherence
and information flow between an uniformly accelerated detector and a massless
quantum scalar field. The availability of exact solutions to this model enables
us to explore the black hole information issue with some quantifiable results
and new insights. To the extent this model can be used as an analog to the
system of a black hole interacting with a quantum field, our result seems to
suggest in the prevalent non-Markovian regime, assuming unitarity for the
combined system, that black hole information is not lost but transferred to the
quantum field degrees of freedom. This combined system will evolve into a
highly entangled state between a remnant of large area (in Bekenstein's black
hole atom analog) without any information of its initial state, while the
quantum field is imbued with complex information content not-so-easily
retrievable by a local observer.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 09:09:46 GMT"
}
] | 2009-12-15T00:00:00 | [
[
"Hu",
"B. L.",
""
],
[
"Lin",
"Shih-Yuin",
""
]
] | [
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] |
712.3644 | Jerome Margueron | J. Margueron (IPNO), H. Sagawa, K. Hagino | Effective pairing interactions with isospin density dependence | null | Phys.Rev.C77:054309,2008 | 10.1103/PhysRevC.77.054309 | null | nucl-th | null | We perform Hartree-Fock-Bogoliubov (HFB) calculations for semi-magic Calcium,
Nickel, Tin and Lead isotopes and $N$=20, 28, 50 and 82 isotones using
density-dependent pairing interactions recently derived from a microscopic
nucleon-nucleon interaction. These interactions have an isovector component so
that the pairing gaps in symmetric and neutron matter are reproduced. Our
calculations well account for the experimental data for the neutron number
dependence of binding energy, two neutrons separation energy, and odd-even mass
staggering of these isotopes. This result suggests that by introducing the
isovector term in the pairing interaction, one can construct a global effective
pairing interaction which is applicable to nuclei in a wide range of the
nuclear chart. It is also shown with the local density approximation (LDA) that
the pairing field deduced from the pairing gaps in infinite matter reproduces
qualitatively well the pairing field for finite nuclei obtained with the HFB
method.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 09:12:03 GMT"
},
{
"version": "v2",
"created": "Sun, 23 Mar 2008 20:25:44 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Margueron",
"J.",
"",
"IPNO"
],
[
"Sagawa",
"H.",
""
],
[
"Hagino",
"K.",
""
]
] | [
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] |
712.3645 | Dmitry Nuzhnyy | S.Kamba, D.Nuzhnyy, R.Nechache, K.Zaveta, D.Niznansky, E.Santava,
C.Harnagea, A.Pignolet | Infrared and magnetic characterization of the multiferroic Bi2FeCrO6
thin films in a broad temperature range | subm. to PRB | Phys. Rev. B 77, 104111 (2008) | 10.1103/PhysRevB.77.104111 | null | cond-mat.mtrl-sci | null | Infrared reflectance spectra of an epitaxial Bi2FeCrO6 thin film prepared by
pulsed laser deposition on LaAlO3 substrate were recorded between 10 and 900 K.
No evidence for a phase transition to the paraelectric phase was observed, but
some phonon anomalies were revealed near 600 K. Most of the polar modes exhibit
only a gradual softening, which results in a continuous increase of the static
permittivity on heating. It indicates that the ferroelectric phase transition
should occur somewhere above 900 K. Magnetic measurements performed up to 1000
K, revealed a possible magnetic phase transition between 600 and 800 K, but the
exact critical temperature cannot be determined due to a strong diamagnetic
signal from the substrate. Nevertheless, our experimental data show that the
B-site ordered Bi2FeCrO6 is one of the rare high-temperature multiferroics.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 09:18:11 GMT"
}
] | 2009-01-06T00:00:00 | [
[
"Kamba",
"S.",
""
],
[
"Nuzhnyy",
"D.",
""
],
[
"Nechache",
"R.",
""
],
[
"Zaveta",
"K.",
""
],
[
"Niznansky",
"D.",
""
],
[
"Santava",
"E.",
""
],
[
"Harnagea",
"C.",
""
],
[
"Pignolet",
"A.",
""
]
] | [
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712.3646 | Ali Naji | Yevgeni Sh. Mamasakhlisov, Ali Naji, Rudolf Podgornik | Partially Annealed Disorder and Collapse of Like-Charged Macroions | 21 pages, 2 figures | J. Stat. Phys. 133, 659 (2008) | 10.1007/s10955-008-9635-7 | null | cond-mat.soft cond-mat.dis-nn | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Charged systems with partially annealed charge disorder are investigated
using field-theoretic and replica methods. Charge disorder is assumed to be
confined to macroion surfaces surrounded by a cloud of mobile neutralizing
counterions in an aqueous solvent. A general formalism is developed by assuming
that the disorder is partially annealed (with purely annealed and purely
quenched disorder included as special cases), i.e., we assume in general that
the disorder undergoes a slow dynamics relative to fast-relaxing counterions
making it possible thus to study the stationary-state properties of the system
using methods similar to those available in equilibrium statistical mechanics.
By focusing on the specific case of two planar surfaces of equal mean surface
charge and disorder variance, it is shown that partial annealing of the
quenched disorder leads to renormalization of the mean surface charge density
and thus a reduction of the inter-plate repulsion on the mean-field or
weak-coupling level. In the strong-coupling limit, charge disorder induces a
long-range attraction resulting in a continuous disorder-driven collapse
transition for the two surfaces as the disorder variance exceeds a threshold
value. Disorder annealing further enhances the attraction and, in the limit of
low screening, leads to a global attractive instability in the system.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 09:25:22 GMT"
},
{
"version": "v2",
"created": "Sat, 23 May 2009 22:21:45 GMT"
}
] | 2009-05-24T00:00:00 | [
[
"Mamasakhlisov",
"Yevgeni Sh.",
""
],
[
"Naji",
"Ali",
""
],
[
"Podgornik",
"Rudolf",
""
]
] | [
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] |
712.3647 | Nicola Visciglia | Scipio Cuccagna, Nicola Visciglia | Strichartz estimates for Schroedinger equations with periodic potential
in 1D | This paper has been withdrawn | null | null | null | math.AP | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | This paper has been withdrawn by the author due to a crucial error in the
Proof of Theorem 0.3
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 09:26:39 GMT"
},
{
"version": "v2",
"created": "Mon, 9 Jun 2008 11:48:37 GMT"
}
] | 2008-06-09T00:00:00 | [
[
"Cuccagna",
"Scipio",
""
],
[
"Visciglia",
"Nicola",
""
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] |
712.3648 | Nicola Visciglia | Luis Vega, Nicola Visciglia | Asymptotic Lower Bounds for a class of Schroedinger Equations | 24 pages. to appear on Comm. Math. Phys | null | 10.1007/s00220-008-0432-6 | null | math.AP | null | We shall study the following initial value problem: \begin{equation}{\bf
i}\partial_t u - \Delta u + V(x) u=0, \hbox{} (t, x) \in {\mathbf R} \times
{\mathbf R}^n, \end{equation} $$u(0)=f,$$ where $V(x)$ is a real short--range
potential, whose radial derivative satisfies some supplementary assumptions.
More precisely we shall present a family of identities satisfied by the
solutions to the previous Cauchy problem. As a by--product of these identities
we deduce some uniqueness results and a lower bound for the so called local
smoothing which becomes an identity in a precise asymptotic sense.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 09:35:00 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Vega",
"Luis",
""
],
[
"Visciglia",
"Nicola",
""
]
] | [
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] |
712.3649 | Gilles Schaeffer | Guillaume Chapuy, Michel Marcus and Gilles Schaeffer | A bijection for rooted maps on orientable surfaces | 27 pages ; We correct an inaccuracy in the proof of Lemma 8 | SIAM Journal on Discrete Mathematics, 23(3):1587-1611 (2009) | null | null | math.CO | null | The enumeration of maps and the study of uniform random maps have been
classical topics of combinatorics and statistical physics ever since the
seminal work of Tutte in the sixties. Following the bijective approach
initiated by Cori and Vauquelin in the eighties, we describe a bijection
between rooted maps, or rooted bipartite quadrangulations, on a surface of
genus g and some simpler objects that generalize plane trees. Thanks to a
rerooting argument, our bijection allows to compute the generating series of
rooted maps on a surface of genus g with respect to the number of edges, and to
recover the asymptotic numbers of such maps.
Our construction allows to keep track in a bipartite quadrangulation of the
distances of all vertices to a random basepoint. This is an analog for higher
genus surfaces of the basic result on which were built the recent advances in
the comprehension of the intrinsec geometry of large random planar maps,
hopefully opening the way to the study of a model of continuum random surfaces
of genus g.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 09:49:11 GMT"
},
{
"version": "v2",
"created": "Wed, 2 Apr 2008 16:55:06 GMT"
}
] | 2010-06-29T00:00:00 | [
[
"Chapuy",
"Guillaume",
""
],
[
"Marcus",
"Michel",
""
],
[
"Schaeffer",
"Gilles",
""
]
] | [
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] |
712.365 | Anne Fey-den Boer | Anne Fey, Remco van der Hofstad, Marten Klok | Large deviations for eigenvalues of sample covariance matrices, with
applications to mobile communication systems | corrected some typing errors, and extended Theorem 3.1 to Wishart
matrices; to appear in Advances of Applied Probability | Advances in Applied Probability 40 nr. 4 (2008), 1048-1071 | 10.1239/aap/1231340164 | null | math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We study sample covariance matrices of the form $W=\frac 1n C C^T$, where $C$
is a $k\times n$ matrix with i.i.d. mean zero entries. This is a generalization
of so-called Wishart matrices, where the entries of $C$ are independent and
identically distributed standard normal random variables. Such matrices arise
in statistics as sample covariance matrices, and the high-dimensional case,
when $k$ is large, arises in the analysis of DNA experiments.
We investigate the large deviation properties of the largest and smallest
eigenvalues of $W$ when either $k$ is fixed and $n\to \infty$, or $k_n\to
\infty$ with $k_n=o(n/\log\log{n})$, in the case where the squares of the
i.i.d. entries have finite exponential moments. Previous results, proving a.s.
limits of the eigenvalues, only require finite fourth moments.
Our most explicit results for $k$ large are for the case where the entries of
$C$ are $\pm1$ with equal probability. We relate the large deviation rate
functions of the smallest and largest eigenvalue to the rate functions for
independent and identically distributed standard normal entries of $C$. This
case is of particular interest, since it is related to the problem of the
decoding of a signal in a code division multiple access system arising in
mobile communication systems. In this example, $k$ plays the role of the number
of users in the system, and $n$ is the length of the coding sequence of each of
the users. Each user transmits at the same time and uses the same frequency,
and the codes are used to distinguish the signals of the separate users. The
results imply large deviation bounds for the probability of a bit error due to
the interference of the various users.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 09:40:49 GMT"
},
{
"version": "v2",
"created": "Fri, 14 Nov 2008 14:11:30 GMT"
}
] | 2009-01-29T00:00:00 | [
[
"Fey",
"Anne",
""
],
[
"van der Hofstad",
"Remco",
""
],
[
"Klok",
"Marten",
""
]
] | [
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] |
712.3651 | Xavier Moya | Lluis Manosa, Xavier Moya, Antoni Planes, Oliver Gutfleisch, Julia
Lyubina, Maria Barrio, Josep-Lluis Tamarit, Seda Aksoy, Thorsten Krenke,
Mehmet Acet | Effects of hydrostatic pressure on the magnetism and martensitic
transition of Ni-Mn-In magnetic superelastic alloys | 3 pages, 3 figures. Accepted for publication in Applied Physics
Letters | null | 10.1063/1.2830999 | null | cond-mat.mtrl-sci | null | We report magnetization and differential thermal analysis measurements as a
function of pressure accross the martensitic transition in magnetically
superelastic Ni-Mn-In alloys. It is found that the properties of the
martensitic transformation are significantly affected by the application of
pressure. All transition temperatures shift to higher values with increasing
pressure. The largest rate of temperature shift with pressure has been found
for Ni$_{50}$Mn$_{34}$In$_{16}$ as a consequence of its small entropy change at
the transition. Such a strong pressure dependence of the transition temperature
opens up the possibility of inducing the martensitic transition by applying
relatively low hydrostatic pressures.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 09:42:31 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Manosa",
"Lluis",
""
],
[
"Moya",
"Xavier",
""
],
[
"Planes",
"Antoni",
""
],
[
"Gutfleisch",
"Oliver",
""
],
[
"Lyubina",
"Julia",
""
],
[
"Barrio",
"Maria",
""
],
[
"Tamarit",
"Josep-Lluis",
""
],
[
"Aksoy",
"Seda",
""
],
[
"Krenke",
"Thorsten",
""
],
[
"Acet",
"Mehmet",
""
]
] | [
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] |
712.3652 | Simone Piccinin | Simone Piccinin, Catherine Stampfl, Matthias Scheffler | First-principles investigation of Ag-Cu alloy surfaces in an oxidizing
environment | 10 pages, 6 figures | null | 10.1103/PhysRevB.77.075426 | null | cond-mat.mtrl-sci | null | In this paper we investigate by means of first-principles density functional
theory calculations the (111) surface of the Ag-Cu alloy under varying
conditions of pressure of the surrounding oxygen atmosphere and temperature.
This alloy has been recently proposed as a catalyst with improved selectivity
for ethylene epoxidation with respect to pure silver, the catalyst commonly
used in industrial applications. Here we show that the presence of oxygen leads
to copper segregation to the surface. Considering the surface free energy as a
function of the surface composition, we construct the convex hull to
investigate the stability of various surface structures. By including the
dependence of the free surface energy on the oxygen chemical potential, we are
able compute the phase diagram of the alloy as a function of temperature,
pressure and surface composition. We find that, at temperature and pressure
typically used in ethylene epoxidation, a number of structures can be present
on the surface of the alloy, including clean Ag(111), thin layers of copper
oxide and thick oxide-like structures. These results are consistent with, and
help explain, recent experimental results.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 09:44:54 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Piccinin",
"Simone",
""
],
[
"Stampfl",
"Catherine",
""
],
[
"Scheffler",
"Matthias",
""
]
] | [
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] |
712.3653 | Naile Liu | Nai-Le Liu, Li Li, Sixia Yu, Zeng-Bing Chen | Duality relation and joint measurement in a Mach-Zehnder Interferometer | 6 pages, 2 figures, title changed, presentation improved, appendix
added, references updated, final version as published in PRA | Phys. Rev. A 79, 052108 (2009) | null | null | quant-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The Mach-Zehnder interferometric setup quantitatively characterizing the
wave-particle duality implements in fact a joint measurement of two unsharp
observables. We present a necessary and sufficient condition for such a pair of
unsharp observables to be jointly measurable. The condition is shown to be
equivalent to a duality inequality, which for the optimal strategy of
extracting the which-path information is more stringent than the
Jaeger-Shimony-Vaidman-Englert inequality.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 09:53:32 GMT"
},
{
"version": "v2",
"created": "Thu, 22 May 2008 15:45:28 GMT"
},
{
"version": "v3",
"created": "Tue, 12 May 2009 16:09:38 GMT"
}
] | 2009-05-12T00:00:00 | [
[
"Liu",
"Nai-Le",
""
],
[
"Li",
"Li",
""
],
[
"Yu",
"Sixia",
""
],
[
"Chen",
"Zeng-Bing",
""
]
] | [
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] |
712.3654 | Alejandro Chinea Manrique De Lara | Alejandro Chinea Manrique De Lara, Juan Manuel Moreno, Arostegui Jordi
Madrenas, Joan Cabestany | Improving the Performance of PieceWise Linear Separation Incremental
Algorithms for Practical Hardware Implementations | 10 pages, 1 figure, 3 tables | Biological and Artificial Computation: From Neuroscience to
Technology, J.Mira, R.Moreno-Diaz, J.Cabestany (eds.), pp. 607-616,
Springer-Verlag, 1997 | null | null | cs.NE cs.AI cs.LG | null | In this paper we shall review the common problems associated with Piecewise
Linear Separation incremental algorithms. This kind of neural models yield poor
performances when dealing with some classification problems, due to the
evolving schemes used to construct the resulting networks. So as to avoid this
undesirable behavior we shall propose a modification criterion. It is based
upon the definition of a function which will provide information about the
quality of the network growth process during the learning phase. This function
is evaluated periodically as the network structure evolves, and will permit, as
we shall show through exhaustive benchmarks, to considerably improve the
performance(measured in terms of network complexity and generalization
capabilities) offered by the networks generated by these incremental models.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 10:05:52 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"De Lara",
"Alejandro Chinea Manrique",
""
],
[
"Moreno",
"Juan Manuel",
""
],
[
"Madrenas",
"Arostegui Jordi",
""
],
[
"Cabestany",
"Joan",
""
]
] | [
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] |
712.3655 | Rejish Nath g r | R. Nath, P. Pedri and L. Santos | Stability of dark solitons in three dimensional dipolar Bose-Einstein
condensates | 4 pages, 3 eps figures | Phys. Rev. Lett. 101, 210402 (2008) | 10.1103/PhysRevLett.101.210402 | null | cond-mat.other | null | The dynamical stability of dark solitons in dipolar Bose-Einstein condensates
is studied. For standard short-range interacting condensates dark solitons are
unstable against transverse excitations in two and three dimensions. On the
contrary, due to its non local character, the dipolar interaction allows for
stable 3D stationary dark solitons, opening a qualitatively novel scenario in
nonlinear atom optics. We discuss in detail the conditions to achieve this
stability, which demand the use of an additional optical lattice, and the
stability regimes.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 20:52:18 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Nath",
"R.",
""
],
[
"Pedri",
"P.",
""
],
[
"Santos",
"L.",
""
]
] | [
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-0.0206488743,
-0.043156147,
-0.0328575224,
-0.0359806642,
-0.0230105892,
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] |
712.3656 | Anders Szepessy | Anders Szepessy | Langevin molecular dynamics derived from Ehrenfest dynamics | 39 pages: modeling and analysis in separate sections. Formulation of
initial data simplified | null | null | null | math-ph math.MP math.PR | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Stochastic Langevin molecular dynamics for nuclei is derived from the
Ehrenfest Hamiltonian system (also called quantum classical molecular dynamics)
in a Kac-Zwanzig setting, with the initial data for the electrons
stochastically perturbed from the ground state and the ratio, $M$, of nuclei
and electron mass tending to infinity. The Ehrenfest nuclei dynamics is
approximated by the Langevin dynamics with accuracy $o(M^{-1/2})$ on bounded
time intervals and by $o(1)$ on unbounded time intervals, which makes the small
$\mathcal{O}(M^{-1/2})$ friction and $o(M^{-1/2})$ diffusion terms visible. The
initial electron probability distribution is a Gibbs density at low temperture,
derived by a stability and consistency argument: starting with any equilibrium
measure of the Ehrenfest Hamiltonian system, the initial electron distribution
is sampled from the equilibrium measure conditioned on the nuclei positions,
which after long time leads to the nuclei positions in a Gibbs distribution
(i.e. asymptotic stability); by consistency the original equilibrium measure is
then a Gibbs measure.The diffusion and friction coefficients in the Langevin
equation satisfy the Einstein's fluctuation-dissipation relation.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 10:11:42 GMT"
},
{
"version": "v2",
"created": "Sun, 5 Apr 2009 08:54:36 GMT"
},
{
"version": "v3",
"created": "Sun, 2 Aug 2009 15:11:16 GMT"
},
{
"version": "v4",
"created": "Mon, 6 Sep 2010 11:53:19 GMT"
},
{
"version": "v5",
"created": "Wed, 30 Mar 2011 10:52:53 GMT"
}
] | 2011-03-31T00:00:00 | [
[
"Szepessy",
"Anders",
""
]
] | [
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712.3657 | Giovanni Alessandrini | Giovanni Alessandrini, Edi Rosset | Symmetry of singular solutions of degenerate quasilinear elliptic
equations | 8 pages, to appear on Rendiconti dell'Istituto di Matematica
dell'Universita' di Trieste | Rend. Istit. Mat. Univ. Trieste 39 (2007) | null | null | math.AP | null | We prove radial symmetry of singular solutions to an overdetermined boundary
value problem for a class of degenerate quasilinear elliptic equations.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 10:18:38 GMT"
}
] | 2010-11-09T00:00:00 | [
[
"Alessandrini",
"Giovanni",
""
],
[
"Rosset",
"Edi",
""
]
] | [
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] |
712.3658 | Sebastiano Pennisi | M.C. Carrisi, M.A. Mele, S. Pennisi | On a non approximated approach to Extended Thermodynamics for dense
gases and macromolecular fluids | null | null | null | null | math-ph math.MP | null | Recently the 14 moments model of Extended Thermodynamics for dense gases and
macromolecular fluids has been considered and an exact solution, of the
restrictions imposed by the entropy principle and that of Galilean relativity,
has been obtained through a non relativistic limit. Here we prove uniqueness of
the above solution and exploit other pertinent conditions such us the convexity
of the function $h'$ related to the entropy density, the problem of subsystems
and the fact that the flux in the conservation law of mass must be the moment
of order 1 in the conservation law of momentum. Also the solution of this last
condition is here obtained without using expansions around equilibrium. The
results present interesting aspects which were not suspected when only
approximated solutions of this problem were known.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 10:19:25 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Carrisi",
"M. C.",
""
],
[
"Mele",
"M. A.",
""
],
[
"Pennisi",
"S.",
""
]
] | [
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] |
712.3659 | Krzysztof Sacha | Jakub S. Prauzner-Bechcicki, Krzysztof Sacha, Bruno Eckhardt, and
Jakub Zakrzewski | Quantum model for double ionization of atoms in strong laser fields | 14 pages, 16 figures, version accepted for publication in Phys. Rev.
A | Phys. Rev. A 78, 013419 (2008) | 10.1103/PhysRevA.78.013419 | null | physics.atom-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We discuss double ionization of atoms in strong laser pulses using a reduced
dimensionality model. Following the insights obtained from an analysis of the
classical mechanics of the process, we confine each electron to move along the
lines that point towards the two-particle Stark saddle in the presence of a
field. The resulting effective two dimensional model is similar to the aligned
electron model, but it enables correlated escape of electrons with equal
momenta, as observed experimentally. The time-dependent solution of the
Schr\"odinger equation allows us to discuss in detail the time dynamics of the
ionization process, the formation of electronic wave packets and the
development of the momentum distribution of the outgoing electrons. In
particular, we are able to identify the rescattering process, simultaneous
direct double ionization during the same field cycle, as well as other double
ionization processes. We also use the model to study the phase dependence of
the ionization process.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 10:28:25 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Apr 2008 11:40:09 GMT"
},
{
"version": "v3",
"created": "Thu, 10 Jul 2008 12:21:39 GMT"
}
] | 2008-08-06T00:00:00 | [
[
"Prauzner-Bechcicki",
"Jakub S.",
""
],
[
"Sacha",
"Krzysztof",
""
],
[
"Eckhardt",
"Bruno",
""
],
[
"Zakrzewski",
"Jakub",
""
]
] | [
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] |
712.366 | Matej Pavsic | Matej Pavsic | Towards a New Paradigm: Relativity in Configuration Space | 15 pages; Presented at "Time and Matter 2007", 26-31 August 2007,
Bled, Slovenia | null | null | null | gr-qc | null | We consider the possibility that the basic space of physics is not spacetime,
but configuration space. We illustrate this on the example with a system of
gravitationally interacting point particles. It turns out that such system can
be described by the minimal length action in a multidimensional configuration
space C with a block diagonal metric. Allowing for more general metrics and
curvatures of C, we step beyond the ordinary general relativity in spacetime.
The latter theory is then an approximation to the general relativity in C.
Other sorts of configuration spaces can also be considered, for instance those
associated with extended objects, such as strings and branes. This enables a
deeper understanding of the geometric principle behind string theory, and an
insight on the occurrence of Yang-Mills and gravitational fields at the
`fundamental level'.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 12:54:18 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Pavsic",
"Matej",
""
]
] | [
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] |
712.3661 | R\'emi Huguet | R. Huguet, J.C. Caillon and J. Labarsouque | A nuclear matter description based on quark structure of the nucleon and
pion exchange | Revised Version, 30 pages, 9 figures, 4 tables, Accepted for
publication in Nuclear Physics A | Nucl.Phys.A809:189-210,2008 | 10.1016/j.nuclphysa.2008.06.002 | null | nucl-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We investigate the possibility to describe nuclear matter in an approach
constrained by the prominent features of quantum chromodynamics. We mapped the
in-medium nucleon self-energies of a point coupling relativistic mean-field
model on self-energies obtained in effective theories of QCD. More precisely,
the contributions to the nucleon self-energy have been separated into the short
range part, driven principally by the quark structure of the nucleon described
in a quark-diquark picture, and the long range part, dictated by pion dynamics
and determined using in-medium chiral perturbation theory. A saturation point,
although unrealistic, is obtained without any free parameter. A realistic
description of nuclear matter saturation properties has been obtained with the
inclusion of a small phenomenological correction term to the short range part
of the self-energy.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 10:35:38 GMT"
},
{
"version": "v2",
"created": "Mon, 25 Feb 2008 10:52:40 GMT"
},
{
"version": "v3",
"created": "Mon, 9 Jun 2008 12:50:35 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Huguet",
"R.",
""
],
[
"Caillon",
"J. C.",
""
],
[
"Labarsouque",
"J.",
""
]
] | [
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] |
712.3662 | Nicolas Jacon | C\'edric Bonnaf\'e (LM-Besan\c{c}on), Nicolas Jacon (LM-Besan\c{c}on) | Cellular structures on Hecke algebras of type B | null | null | null | null | math.RT math.CO | null | The aim of this paper is to gather and (try to) unify several approaches for
the modular representation theory of Hecke algebras of type $B$. We attempt to
explain the connections between Geck's cellular structures (coming from
Kazhdan-Lusztig theory with unequal parameters) and Ariki's Theorem on the
canonical basis of the Fock spaces.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 10:39:08 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Apr 2008 09:39:25 GMT"
},
{
"version": "v3",
"created": "Wed, 14 May 2008 07:45:01 GMT"
}
] | 2008-05-14T00:00:00 | [
[
"Bonnafé",
"Cédric",
"",
"LM-Besançon"
],
[
"Jacon",
"Nicolas",
"",
"LM-Besançon"
]
] | [
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] |
712.3663 | Hujeirat | A. Hujeirat, F.-K. Thielemann, J. Dusek, A. Nusser | Compressed low Mach number flows in astrophysics: a nonlinear Newtonian
numerical solver | 12 pages, 4 figures | null | null | null | astro-ph | null | Internal flows inside gravitationally stable astrophysical objects, such as
the Sun, stars and compact stars are compressed and extremely subsonic. Such
low Mach number flows are usually encountered when studying for example dynamo
action in stars, planets, the hydro-thermodynamics of X-ray bursts on neutron
stars and dwarf novae. Treating such flows is numerically complicated and
challenging task. We aim to present a robust numerical tool that enables
modeling the time-evolution or quasi-stationary of stratified low Mach number
flows under astrophysical conditions. It is argued that astrophysical low Mach
number flows cannot be considered as an asymptotic limit of incompressible
flows, but rather as highly compressed flows with extremely stiff pressure
terms. Unlike the pseudo-pressure in incompressible fluids, a Possion-like
treatment for the pressure would smooth unnecessarily the physically induced
acoustic perturbations, thereby violating the conservation character of the
compressible equations. Moreover, classical dimensional splitting techniques,
such as ADI or Line-Gauss-Seidel methods are found to be unsuited for modeling
compressible flows with low Mach numbers. In this paper we present a nonlinear
Newton-type solver that is based on the defect-correction iteration procedure
and in which the Approximate Factorization Method (AFM) is used as a
preconditioner. This solver is found to be sufficiently robust and is capable
of capturing stationary solutions for viscous rotating flows with Mach number
as small as $\mcal{M} \approx 10^{-3},$ i.e., near the incompressibility limit.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 10:52:56 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Hujeirat",
"A.",
""
],
[
"Thielemann",
"F. -K.",
""
],
[
"Dusek",
"J.",
""
],
[
"Nusser",
"A.",
""
]
] | [
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] |
712.3664 | Kazimierz St{\ke}pie\'n | L. Lipski and K. Stepien | Effective temperatures of magnetic CP stars from full spectral energy
distributions | 13 pages, 5 figures, accepted to MNRAS | Mon.Not.Roy.Astron.Soc.385:481,2008 | 10.1111/j.1365-2966.2008.12856.x | null | astro-ph | null | New determinations of effective temperatures of 23 magnetic, chemically
peculiar (mCP) stars were obtained from a fit of metal enhanced model
atmospheres to the observed spectral energy distributions (SED) from UV to red.
The root-mean-square (RMS) method was used to fit the theoretical SED to the
observations corrected for reddening if necessary, with metallicity and
effective temperature as the fitting parameters. Gravity was assumed to be
equal to log g = 4 for main sequence stars and to log g = 3 for two giants in
the considered sample. Equal weights were given to the UV part and visual part
of SED. Independently of the formal quality of fit resulting from the RMS
method applied to the whole SED, the quality of fit was additionally checked
for each star by determination of the temperature from the best fitting model
atmosphere to the UV part and the visual part of SED separately. Both
temperatures should be close to one another if the global best fitting model
satisfactorily describes the full observed SED. This is the case for about a
half of the investigated stars but the difference exceeds 750 K for the
remaining stars with the extreme values above 2000 K. Possible reasons for such
discrepancies are discussed. New, revised calibrations of effective temperature
and bolometric corrections of mCP stars in terms of reddening free Stromgren
indices are given.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:00:28 GMT"
}
] | 2008-11-07T00:00:00 | [
[
"Lipski",
"L.",
""
],
[
"Stepien",
"K.",
""
]
] | [
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] |
712.3665 | Paul M. Terwilliger | Kazumasa Nomura and Paul Terwilliger | Sharp tridiagonal pairs | 24 pages | null | null | null | math.RA math.CO | null | Let $K$ denote a field and let $V$ denote a vector space over $K$ with finite
positive dimension. We consider a pair of $K$-linear transformations $A:V \to
V$ and $A^*:V \to V$ that satisfies the following conditions:
(i) each of $A,A^*$ is diagonalizable;
(ii) there exists an ordering ${V_i}_{i=0}^d$ of the eigenspaces of $A$ such
that $A^* V_i \subseteq V_{i-1} + V_{i} + V_{i+1}$ for $0 \leq i \leq d$, where
$V_{-1}=0$ and $V_{d+1}=0$;
(iii) there exists an ordering ${V^*_i}_{i=0}^\delta$ of the eigenspaces of
$A^*$ such that $A V^*_i \subseteq V^*_{i-1} + V^*_{i} + V^*_{i+1}$ for $0 \leq
i \leq \delta$, where $V^*_{-1}=0$ and $V^*_{\delta+1}=0$;
(iv) there is no subspace $W$ of $V$ such that $AW \subseteq W$, $A^* W
\subseteq W$, $W \neq 0$, $W \neq V$.
We call such a pair a {\em tridiagonal pair} on $V$. It is known that
$d=\delta$ and for $0 \leq i \leq d$ the dimensions of $V_i$, $V_{d-i}$,
$V^*_i$, $V^*_{d-i}$ coincide. We say the pair $A,A^*$ is {\em sharp} whenever
$\dim V_0=1$. A conjecture of Tatsuro Ito and the second author states that if
$K$ is algebraically closed then $A,A^*$ is sharp. In order to better
understand and eventually prove the conjecture, in this paper we begin a
systematic study of the sharp tridiagonal pairs.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:01:08 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Nomura",
"Kazumasa",
""
],
[
"Terwilliger",
"Paul",
""
]
] | [
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712.3666 | Yuchun Wu | Yu-Chun Wu, Piotr Badziag, Marcin Wie\'sniak and Marek \.Zukowski | Extending Bell inequalities to more parties | 8 pages, no figure | Phys. Rev. A 77 032105, 2008 | 10.1103/PhysRevA.77.032105 | null | quant-ph | null | We describe a method of extending Bell inequalities from $n$ to $n+1$ parties
and formulate sufficient conditions for our method to produce tight
inequalities from tight inequalities. The method is non trivial in the sense
that the inequalities produced by it, when applied to entangled quantum states
may be violated stronger than the original inequalities. In other words, the
method is capable of generating inequalities which are more powerfull
indicators of non-classical correlations than the original inequalities.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:04:31 GMT"
},
{
"version": "v2",
"created": "Tue, 6 May 2008 20:22:53 GMT"
}
] | 2008-05-06T00:00:00 | [
[
"Wu",
"Yu-Chun",
""
],
[
"Badziag",
"Piotr",
""
],
[
"Wieśniak",
"Marcin",
""
],
[
"Żukowski",
"Marek",
""
]
] | [
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] |
712.3667 | Marta Morigi Ms | Gustavo Fernandez Alcob\'er and Marta Morigi | Generalizing a theorem of P. Hall on finite-by-nilpotent groups | null | null | null | null | math.GR | null | Let $\gamma_i(G)$ and $Z_i(G)$ denote the $i$-th terms of the lower and upper
central series of a group $G$, respectively. P. Hall showed that if
$\gamma_{i+1}(G)$ is finite then the index $|G:Z_{2i}(G)|$ is finite. We prove
that the same result holds under the weaker hypothesis that
$|\gamma_{i+1}(G):\gamma_{i+1}(G)\cap Z_i(G)|$ is finite.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:08:12 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Alcobér",
"Gustavo Fernandez",
""
],
[
"Morigi",
"Marta",
""
]
] | [
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712.3668 | Janusz Kaluzny | J. Kaluzny, I.B. Thompson | Variability Study of EHB Stars in the Globular Cluster NGC 6752 | 4 pages, 4 figures, to appear in "Hot Subdwarf Stars and Related
Objects", ASP Conf. Ser | null | null | null | astro-ph | null | We present the results of a search for variable stars in the central part of
the globular cluster NGC 6752. The monitored sample included 160 BHB and 107
EHB stars, respectively. A total of 17 variables were detected of which 14 are
new identifications. Five variables are BHB/EHB stars. We report also on
identification of a detached eclipsing binary being likely a member of the
cluster. Moreover, we detected an outburst of a dwarf nova located in the
cluster core.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:23:29 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Kaluzny",
"J.",
""
],
[
"Thompson",
"I. B.",
""
]
] | [
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] |
712.3669 | Marco Ruggieri | L. Campanelli and M. Ruggieri | Supersymmetric Q-balls: A Numerical Study | 6 pages, 2 columns, 6 figures. To appear on Phys. Rev. D | Phys.Rev.D77:043504,2008 | 10.1103/PhysRevD.77.043504 | null | hep-th hep-ph | null | We study numerically a class of non-topological solitons, the Q-balls,
arising in supersymmetric extension of the Standard Model with low-energy,
gauge-mediated symmetry breaking. % Taking into account the exact form of the
supersymmetric potential giving rise to Q-balls, we find that there is a lower
limit on the value of the charge $Q$ in order to make them classically stable:
$Q \gtrsim 5 \times 10^2 Q_{\rm cr}$, where $Q_{\rm cr}$ is constant depending
on the parameters defining the potential and can be in the range $1 \lesssim
Q_{\rm cr} \lesssim 10^{8 \div 16}$.If $Q$ is the baryon number, stability with
respect to the decay into protons requires $Q \gtrsim 10^{17} Q_{\rm cr}$,
while if the gravitino mass is greater then $m_{3/2} \gtrsim 61 \MeV$, no
stable gauge-mediation supersymmetric Q-balls exist. Finally, we find that
energy and radius of Q-balls can be parameterized as $E \sim \xi_E Q^{3/4}$ and
$R \sim \xi_R Q^{1/4}$, where $\xi_E$ and $\xi_R$ are slowly varying functions
of the charge.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:24:11 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Campanelli",
"L.",
""
],
[
"Ruggieri",
"M.",
""
]
] | [
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] |
712.367 | Vadim Schechtman | Vassily Gorbounov and Vadim Schechtman | Homological Algebra and Divergent Series | null | SIGMA 5 (2009), 034, 31 pages | 10.3842/SIGMA.2009.034 | null | math.AG | http://creativecommons.org/licenses/by-nc-sa/3.0/ | We study some features of infinite resolutions of Koszul algebras motivated
by the developments in the string theory initiated by Berkovits.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:56:32 GMT"
},
{
"version": "v2",
"created": "Wed, 8 Oct 2008 16:45:36 GMT"
},
{
"version": "v3",
"created": "Tue, 24 Mar 2009 06:03:26 GMT"
}
] | 2009-03-24T00:00:00 | [
[
"Gorbounov",
"Vassily",
""
],
[
"Schechtman",
"Vadim",
""
]
] | [
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] |
712.3671 | Nedzad Limic | Nedzad Limi\'c and Mladen Rogina | Monotone Numerical Schemes for a Dirichlet Problem for Elliptic
Operators in Divergence Form | 22 pages, 1 figure | null | null | null | math.AP math.NA | null | We consider a second order differential operator $A(\msx) = -\:\sum_{i,j=1}^d
\partial_i a_{ij}(\msx) \partial_j \:+\: \sum_{j=1}^d \partial_j \big(b_j(\msx)
\cdot \big)\:+\: c(\msx)$ on ${\bbR}^d$, on a bounded domain $D$ with Dirichlet
boundary conditions on $\partial D$, under mild assumptions on the coefficients
of the diffusion tensor $a_{ij}$. The object is to construct monotone numerical
schemes to approximate the solution to the problem $A(\msx) u(\msx) \: = \:
\mu(\msx), \quad \msx \in D$, where $\mu$ is a positive Radon measure. We start
by briefly mentioning questions of existence and uniqueness, introducing
function spaces needed to prove convergence results. Then, we define
non-standard stencils on grid-knots that lead to extended discretization
schemes by matrices possesing compartmental structure. We proceed to
discretization of elliptic operators, starting with constant diffusion tensor
and ending with operators in divergence form. Finally, we discuss
$W_2^1$-convergence in detail, and mention convergence in $C$ and $L_1$ spaces.
We conclude by a numerical example illustarting the schemes and convergence
results.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:36:31 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Limić",
"Nedzad",
""
],
[
"Rogina",
"Mladen",
""
]
] | [
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712.3672 | Prasanta K. Panigrahi | Priyam Das, T. Solomon Raju, Utpal Roy and Prasanta K. Panigrahi | Sinusoidal Excitations in Two Component Bose-Einstein Condensates | 6 pages, 1 figure | PHYSICAL REVIEW A 79, 015601 (2009) | 10.1103/PhysRevA.79.015601 | null | cond-mat.other | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | The non-linear coupled Gross-Pitaevskii equation governing the dynamics of
the two component Bose-Einstein condensate (TBEC) is shown to admit pure
sinusoidal, propagating wave solutions in quasi one dimensional geometry. These
solutions, which exist for a wide parameter range, are then investigated in the
presence of a harmonic oscillator trap with time dependent scattering length.
This illustrates the procedure for coherent control of these modes through
temporal modulation of the parameters, like scattering length and oscillator
frequency. We subsequently analyzed this system in an optical lattice, where
the occurrence of an irreversible phase transition from superfluid to insulator
phase is seen.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:43:08 GMT"
},
{
"version": "v2",
"created": "Mon, 23 Nov 2009 10:35:41 GMT"
}
] | 2009-11-23T00:00:00 | [
[
"Das",
"Priyam",
""
],
[
"Raju",
"T. Solomon",
""
],
[
"Roy",
"Utpal",
""
],
[
"Panigrahi",
"Prasanta K.",
""
]
] | [
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] |
712.3673 | Jan Wiersig | Jan Wiersig, J\"org Main | Fractal Weyl law for chaotic microcavities: Fresnel's laws imply
multifractal scattering | 8 pages, 12 figures | null | 10.1103/PhysRevE.77.036205 | null | nlin.CD physics.optics | null | We demonstrate that the harmonic inversion technique is a powerful tool to
analyze the spectral properties of optical microcavities. As an interesting
example we study the statistical properties of complex frequencies of the fully
chaotic microstadium. We show that the conjectured fractal Weyl law for open
chaotic systems [W. T. Lu, S. Sridhar, and M. Zworski, Phys. Rev. Lett. 91,
154101 (2003)] is valid for dielectric microcavities only if the concept of the
chaotic repeller is extended to a multifractal by incorporating Fresnel's laws.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:49:27 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Wiersig",
"Jan",
""
],
[
"Main",
"Jörg",
""
]
] | [
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712.3674 | Hujeirat | A. Hujeirat, B.W. Keil and F. Heitsch | Advanced numerical methods in astrophysical fluid dynamics | 25 pages, 11 figures, | null | null | null | astro-ph | null | Computational gas dynamics has become a prominent research field both in
astrophysics and cosmology. In the first part of this review we intend to
briefly describe several of the numerical methods used in this field, discuss
their range of application and present strategies for converting
conditionally-stable numerical methods into unconditionally-stable solution
procedures. The underlying aim of the conversion is to enhance the robustness
and unification of numerical methods and subsequently enlarge their range of
applications considerably. In the second part Fabian Heitsch presents and
discusses the implementation of a time-explicit MHD Boltzmann solver.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:55:05 GMT"
}
] | 2007-12-24T00:00:00 | [
[
"Hujeirat",
"A.",
""
],
[
"Keil",
"B. W.",
""
],
[
"Heitsch",
"F.",
""
]
] | [
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] |
712.3675 | Mario Ziman | Mario Ziman, Teiko Heinosaari | Discrimination of quantum observables using limited resources | 8 pages, no figures | Phys. Rev. A 77, 042321 (2008) | 10.1103/PhysRevA.77.042321 | null | quant-ph | null | We address the problem of unambiguous discrimination and identification among
quantum observables. We set a general framework and investigate in details the
case of qubit observables. In particular, we show that perfect discrimination
with two shots is possible only for sharp qubit observables (e.g. Stern-Gerlach
apparatuses) associated with mutually orthogonal directions. We also show that
for sharp qubit observables associated to nonorthogonal directions unambiguous
discrimination with an inconclusive result is always possible.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:55:23 GMT"
},
{
"version": "v2",
"created": "Mon, 18 Feb 2008 15:35:02 GMT"
}
] | 2008-07-15T00:00:00 | [
[
"Ziman",
"Mario",
""
],
[
"Heinosaari",
"Teiko",
""
]
] | [
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] |
712.3676 | Florian Marty | Florian Marty | Relative Zariski Open Objects | 19 pages. A more general main theorem has been proved. The
organisation has been modified | null | null | null | math.AG math.CT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In [TV], Bertrand To\"en and Michel Vaqui\'e define a scheme theory for a
closed monoidal category $(\mathcal{C},\otimes,1)$. One of the key ingredients
of this theory is the definition of a Zariski topology on the category of
commutative monoids in $\mathcal{C}$. The purpose of this article is to prove
that under some hypotheses, Zariski open subobjects of affine schemes can be
classified almost as in the usual case of rings $(Z-mod,\otimes,Z)$. The main
result states that for any commutative monoid $A$, the locale of Zariski open
subobjects of the affine scheme $Spec(A)$ is associated to a topological space
whose points are prime ideals of $A$ and open subsets are defined by the same
formula as in rings. As a consequence, we compare the notions of scheme over
$\mathbb{F}_{1}$ of [D] and [TV].
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:55:28 GMT"
},
{
"version": "v2",
"created": "Thu, 6 Nov 2008 16:19:10 GMT"
},
{
"version": "v3",
"created": "Tue, 12 May 2009 08:36:21 GMT"
}
] | 2009-05-12T00:00:00 | [
[
"Marty",
"Florian",
""
]
] | [
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712.3677 | N. W. Evans | P.E. Verrier (Cambridge), N.W. Evans (Cambridge) | A New Superintegrable Hamiltonian | 11 pages, 4 figures, submitted to The Journal of Mathematical Physics | null | 10.1063/1.2840465 | null | nlin.SI astro-ph | null | We identify a new superintegrable Hamiltonian in 3 degrees of freedom,
obtained as a reduction of pure Keplerian motion in 6 dimensions. The new
Hamiltonian is a generalization of the Keplerian one, and has the familiar 1/r
potential with three barrier terms preventing the particle crossing the
principal planes. In 3 degrees of freedom, there are 5 functionally independent
integrals of motion, and all bound, classical trajectories are closed and
strictly periodic. The generalisation of the Laplace-Runge-Lenz vector is
identified and shown to provide functionally independent isolating integrals.
They are quartic in the momenta and do not arise from separability of the
Hamilton-Jacobi equation. A formulation of the system in action-angle variables
is presented.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:58:54 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Verrier",
"P. E.",
"",
"Cambridge"
],
[
"Evans",
"N. W.",
"",
"Cambridge"
]
] | [
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] |
712.3678 | Nedzad Limic | Nedzad Limi\'c and Mladen Rogina | Numerical approach to $L_1$-problems with the second order elliptic
operators | 33 pages | null | null | null | math.AP math.NA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | For a second order differential operator $A(\msx) =-\nabla a(\msx)\nabla +
b'(\msx)\nabla+ \nabla \big(\msb''(\msx) \cdot\big)$ on a bounded domain $D$
with the Dirichlet boundary conditions on $\partial D$ there exists the inverse
$T(\lambda, A)= (\lambda I+A)^{-1}$ in $L_1(D)$. If $\mu$ is a Radon
(probability) measure on Borel algebra of subsets of $D$, then $T(\lambda,
A)\mu \in L_p(D), p \in [1, d/(d-1))$. We construct the numerical
approximations to $u =T(\lambda, A)\mu$ in two steps. In the first one we
construct grid-solutions ${\bf u}_n$ and in the second step we embed
grid-solutions into the linear space of hat functions $u(n) \in
\dot{W}_p^1(D)$. The strong convergence to the original solutions $u$ is
established in $L_p(D)$ and the weak convergence in $\dot{W}_p^1(D)$.
| [
{
"version": "v1",
"created": "Fri, 21 Dec 2007 11:59:42 GMT"
},
{
"version": "v2",
"created": "Thu, 28 Aug 2008 13:08:37 GMT"
}
] | 2008-08-28T00:00:00 | [
[
"Limić",
"Nedzad",
""
],
[
"Rogina",
"Mladen",
""
]
] | [
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