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801.1673 | Andrea Cattaneo | A. Cattaneo, A. Dekel, S.M. Faber, B. Guiderdoni | Downsizing by Shutdown in Red Galaxies | 21 pages, 13 figures, submitted to MNRAS | null | 10.1111/j.1365-2966.2008.13562.x | null | astro-ph | null | We address the origin of the `downsizing' of elliptical galaxies, according
to which the stars in more massive galaxies formed earlier and over a shorter
period than those in less massive galaxies. We show that this could be the
natural result of a shutdown of star formation in dark matter haloes above a
critical mass of 10^12MSun. This is demonstrated using a semianalytic
simulation of galaxy formation within the standard hierarchical scenario of
structure formation. The assumed threshold mass is motivated by the prediction
of stable shock heating above this mass and the finding that such a shutdown
reproduces the observed distribution of galaxies in luminosity and colour.The
shutdown at a critical halo mass introduces a characteristic stellar mass for
the transition of galaxies into the `red sequence' of the galaxy
colour-magnitude diagram. Central galaxies of haloes that are more massive
today have reached this mass earlier and can therefore grow further along the
red sequence by dry mergers, ending up more massive and containing older stars.
Small galaxies formed in haloes below the critical mass can shutdown late, when
they fall into haloes above the critical mass and become satellites. While our
semianalytic simulation that incorporates an explicit shutdown reproduces
downsizing as inferred from the stellar ages of ellipticals, we explain why it
is much harder to detect downsizing using the mass functions of different
galaxy types.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 21:04:23 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Cattaneo",
"A.",
""
],
[
"Dekel",
"A.",
""
],
[
"Faber",
"S. M.",
""
],
[
"Guiderdoni",
"B.",
""
]
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801.1674 | Ivan Kazachkov | Ivan Kazachkov | A combined space discrete algorithm with a Taylor series by time for CFD | 17 pages | null | null | null | math.NA math-ph math.MP | null | The first order by time partial differential equations are used as models in
applications such as fluid flow, heat transfer, solid deformation,
electromagnetic waves, and others. In this paper we propose the new numerical
method to solve a class of initial-boundary value problems for the PDEs using
one of the known space discrete numerical schemes and a Taylor series expansion
by time. Normally a second order discretization by space is applied while a
first order by time is satisfactory. Nevertheless, in a number of different
problems, discretization both by temporal and by spatial variables is needed of
highest orders, which complicates numerical solution, in some cases
dramatically. Therefore it is difficult to apply the same numerical methods for
the solution of some PDE arrays if their parameters are varying in a wide range
so that in some of them different numerical schemes by time fit the best for
precise numerical solution. The Taylor series based solution strategy for the
non-stationary PDEs in CFD simulations has been proposed here that attempts to
optimise the computation time and fidelity of the numerical solution.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 16:50:37 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Kazachkov",
"Ivan",
""
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801.1675 | Danilo Marchesini | Danilo Marchesini, Pieter van Dokkum (Yale University) | Assessing the Predictive Power of Galaxy Formation Models with the
Rest-Frame Optical Luminosity Functions at 2.0<z<3.3 | 6 pages, 2 figures. To appear in the proceedings of `A Century of
Cosmology', S. Servolo, August 2007, to be published in Il Nuovo Cimento | Nuovo Cim.B122:1121-1126,2007 | 10.1393/ncb/i2008-10452-7 | null | astro-ph | null | We compare recently measured rest-frame V-band luminosity functions (LFs) of
galaxies at redshifts 2.0<z<3.3 to predictions of semianalytic models by De
Lucia & Blaizot and Bower et al. and hydrodynamic simulations by Dave et al.
The models succeed for some luminosity and redshift ranges and fail for others.
A notable success is that the Bower et al. model provides a good match to the
observed LF at z~3. However, all models predict an increase with time of the
rest-frame V-band luminosity density, whereas the observations show a decrease.
The models also have difficulty matching the observed rest-frame colors of
galaxies. In all models the luminosity density of red galaxies increases
sharply from z~3 to z~2.2, whereas it is approximately constant in the
observations. Conversely, in the models the luminosity density of blue galaxies
is approximately constant, whereas it decreases in the observations. These
discrepancies cannot be entirely remedied by changing the treatment of dust and
suggest that current models do not yet provide an adequate description of
galaxy formation and evolution since z~3.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 21:06:40 GMT"
}
] | 2010-11-11T00:00:00 | [
[
"Marchesini",
"Danilo",
"",
"Yale University"
],
[
"van Dokkum",
"Pieter",
"",
"Yale University"
]
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] |
801.1676 | Juan Gerardo Alcazar Arribas | Juan Gerardo Alcazar | Analyzing the Topology Types arising in a Family of Algebraic Curves
Depending On Two Parameters | 8 pages, 4 figures | null | null | null | cs.SC | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Given the implicit equation $F(x,y,t,s)$ of a family of algebraic plane
curves depending on the parameters $t,s$, we provide an algorithm for studying
the topology types arising in the family. For this purpose, the algorithm
computes a finite partition of the parameter space so that the topology type of
the family stays invariant over each element of the partition. The ideas
contained in the paper can be seen as a generalization of the ideas in
\cite{JGRS}, where the problem is solved for families of algebraic curves
depending on one parameter, to the two-parameters case.
| [
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{
"version": "v2",
"created": "Tue, 2 Sep 2008 15:44:23 GMT"
}
] | 2008-09-02T00:00:00 | [
[
"Alcazar",
"Juan Gerardo",
""
]
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801.1677 | Avi Loeb | Abraham Loeb (Harvard), Stuart Wyithe (Melbourne) | Possibility of Precise Measurement of the Cosmological Power Spectrum
With a Dedicated 21cm Survey After Reionization | 4 pages, 3 figures, Accepted for publication in Physical Review
Letters | Phys.Rev.Lett.100:161301,2008 | 10.1103/PhysRevLett.100.161301 | null | astro-ph hep-ph | null | Measurements of the 21cm line emission by residual cosmic hydrogen after
reionization can be used to trace the power spectrum of density perturbations
through a significant fraction of the observable volume of the Universe. We
show that a dedicated 21cm observatory coule probe a number of independent
modes that is two orders of magnitude larger than currently available, and
enable a cosmic-variance limited detection of the signature of a neutrino mass
~0.05eV. The evolution of the linear growth factor with redshift could also
constrain exotic theories of gravity or dark energy to an unprecedented
precision.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 21:09:04 GMT"
},
{
"version": "v2",
"created": "Fri, 21 Mar 2008 22:43:07 GMT"
}
] | 2009-06-23T00:00:00 | [
[
"Loeb",
"Abraham",
"",
"Harvard"
],
[
"Wyithe",
"Stuart",
"",
"Melbourne"
]
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801.1678 | Jarle Brinchmann | Jarle Brinchmann (1,4), Max Pettini (2), Stephane Charlot (3) ((1)
CAUP Porto, (2) IoA Cambridge, (3) IAP, (4) Leiden) | New insights into the stellar content and physical conditions of
star-forming galaxies at z = 2-3 from spectral modelling | 14pages, Accepted for MNRAS | null | 10.1111/j.1365-2966.2008.12914.x | null | astro-ph | null | We have used extensive libraries of model and empirical galaxy spectra
(assembled respectively from the population synthesis code of Bruzual and
Charlot and the fourth data release of the Sloan Digital Sky Survey) to
interpret some puzzling features seen in the spectra of high redshift
star-forming galaxies. We show that a stellar He II 1640 emission line,
produced in the expanding atmospheres of Of and Wolf-Rayet stars, should be
detectable with an equivalent width of 0.5-1.5AA in the integrated spectra of
star-forming galaxies, provided the metallicity is greater than about half
solar. Our models reproduce the strength of the He II 1640 line measured in the
spectra of Lyman break galaxies for established values of their metallicities.
With better empirical calibrations in local galaxies, this spectral feature has
the potential of becoming a useful diagnostic of massive star winds at high, as
well as low, redshifts.
We also uncover a relationship in SDSS galaxies between their location in the
[O III]/Hb vs. [N II]/Ha diagnostic diagram (the BPT diagram) and their excess
specific star formation rate relative to galaxies of similar mass. We infer
that an elevated ionisation parameter U is at the root of this effect, and
propose that this is also the cause of the offset of high redshift star-forming
galaxies in the BPT diagram compared to local ones. We further speculate that
higher electron densities and escape fractions of hydrogen ionising photons may
be the factors responsible for the systematically higher values of U in the H
II regions of high redshift galaxies. The impact of such differences on
abundance determinations from strong nebular lines are considered and found to
be relatively minor.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 21:11:54 GMT"
}
] | 2009-10-08T00:00:00 | [
[
"Brinchmann",
"Jarle",
""
],
[
"Pettini",
"Max",
""
],
[
"Charlot",
"Stephane",
""
]
] | [
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] |
801.1679 | Geraldine Servant | Roberto Contino and Geraldine Servant | Discovering the top partners at the LHC using same-sign dilepton final
states | 23 pages, 10 figures. v2: typos corrected, a few comments added,
conclusions unchanged | JHEP 0806:026,2008 | 10.1088/1126-6708/2008/06/026 | CERN-PH-TH/2007-233, SACLAY-T07/149 | hep-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | A natural, non-supersymmetric solution to the hierarchy problem generically
requires fermionic partners of the top quark with masses not much heavier than
500 GeV. We study the pair production and detection at the LHC of the top
partners with electric charge Q=5/3 (T_{5/3}) and Q=-1/3 (B), that are
predicted in models where the Higgs is a pseudo-Goldstone boson. The exotic
T_{5/3} fermion, in particular, is the distinct prediction of a LR custodial
parity invariance of the electroweak symmetry breaking sector. Both kinds of
new fermions decay to Wt, leading to a t\bar{t}WW final state. We focus on the
golden channel with two same-sign leptons, and show that a discovery could come
with less than 100 pb^{-1} (less than 20 fb^{-1}) of integrated luminosity for
masses M=500 GeV (M=1TeV). In the case of the T_{5/3}, we present a simple
strategy for its reconstruction in the fully hadronic decay chain. Although no
full mass reconstruction is possible for the B, we still find that the
same-sign dilepton channel offers the best chances of discovery compared to
other previous searches that used final states with one or two opposite-sign
leptons, and hence suffered from the large t\bar{t} background. Our analysis
also directly applies to the search of 4th generation b' quarks.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 15:53:53 GMT"
},
{
"version": "v2",
"created": "Wed, 3 Mar 2010 16:46:20 GMT"
}
] | 2010-03-03T00:00:00 | [
[
"Contino",
"Roberto",
""
],
[
"Servant",
"Geraldine",
""
]
] | [
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] |
801.168 | Patrick Tisserand | P.Tisserand, J.B.Marquette, P.R.Wood, E.Lesquoy, J.P.Beaulieu,
A.Milsztajn, C.Hamadache, C.Afonso, J.N.Albert, J.Andersen, R.Ansari,
E.Aubourg, P.Bareyre, X.Charlot, C.Coutures, R.Ferlet, P.Fouqu\'e,
J.F.Glicenstein, B.Goldman, A.Gould, M.Gros, J.Haissinski, J.de Kat, L.Le
Guillou, C.Loup, C.Magneville, E.Maurice, A.Maury, M.Moniez,
N.Palanque-Delabrouille, O.Perdereau, Y.Rahal, J.Rich, M.Spiro,
A.Vidal-Madjar and S.Zylberajch | R Coronae Borealis stars in the Galactic Bulge discovered by EROS-2 | 20 pages, 26 figures, Accepted in A&A | null | 10.1051/0004-6361:20078814 | null | astro-ph | null | Rare types of variable star may give unique insight into short-lived stages
of stellar evolution. The systematic monitoring of millions of stars and
advanced light curve analysis techniques of microlensing surveys make them
ideal for discovering also such rare variable stars. One example is the R
Coronae Borealis (RCB) stars, a rare type of evolved carbon-rich supergiant. We
have conducted a systematic search of the EROS-2 database for the Galactic
catalogue Bulge and spiral arms to find Galactic RCB stars. The light curves of
$\sim$100 million stars, monitored for 6.7 years (from July 1996 to February
2003), have been analysed to search for the main signature of RCB stars, large
and rapid drops in luminosity. Follow-up spectroscopy has been used to confirm
the photometric candidates. We have discovered 14 new RCB stars, all in the
direction of the Galactic Bulge, bringing the total number of confirmed
Galactic RCB stars to about 51. After reddening correction, the colours and
absolute magnitudes of at least 9 of the stars are similar to those of
Magellanic RCB stars. This suggests that these stars are in fact located in the
Galactic Bulge, making them the first RCB stars discovered in the Bulge. The
localisation of the 5 remaining RCBs is more uncertain: 4 are either located
behind the Bulge at an estimated maximum distance of 14 kpc or have an unusual
thick circumstellar shell; the other is a DY Per RCB which may be located in
the Bulge, even if it is fainter than the known Magellanic DY Per. From the
small scale height found using the 9 new Bulge RCBs, $61<h^{RCB}_{Bulge}<246$
pc (95% C.L.), we conclude that the RCB stars follow a disk-like distribution
inside the Bulge.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 01:20:59 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Tisserand",
"P.",
""
],
[
"Marquette",
"J. B.",
""
],
[
"Wood",
"P. R.",
""
],
[
"Lesquoy",
"E.",
""
],
[
"Beaulieu",
"J. P.",
""
],
[
"Milsztajn",
"A.",
""
],
[
"Hamadache",
"C.",
""
],
[
"Afonso",
"C.",
""
],
[
"Albert",
"J. N.",
""
],
[
"Andersen",
"J.",
""
],
[
"Ansari",
"R.",
""
],
[
"Aubourg",
"E.",
""
],
[
"Bareyre",
"P.",
""
],
[
"Charlot",
"X.",
""
],
[
"Coutures",
"C.",
""
],
[
"Ferlet",
"R.",
""
],
[
"Fouqué",
"P.",
""
],
[
"Glicenstein",
"J. F.",
""
],
[
"Goldman",
"B.",
""
],
[
"Gould",
"A.",
""
],
[
"Gros",
"M.",
""
],
[
"Haissinski",
"J.",
""
],
[
"de Kat",
"J.",
""
],
[
"Guillou",
"L. Le",
""
],
[
"Loup",
"C.",
""
],
[
"Magneville",
"C.",
""
],
[
"Maurice",
"E.",
""
],
[
"Maury",
"A.",
""
],
[
"Moniez",
"M.",
""
],
[
"Palanque-Delabrouille",
"N.",
""
],
[
"Perdereau",
"O.",
""
],
[
"Rahal",
"Y.",
""
],
[
"Rich",
"J.",
""
],
[
"Spiro",
"M.",
""
],
[
"Vidal-Madjar",
"A.",
""
],
[
"Zylberajch",
"S.",
""
]
] | [
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0.0361772217,
-0.0093512731,
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0.0824169815,
0.0201101042,
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] |
801.1681 | Artur Rutkowski | A. Olech, A. Rutkowski, A. Schwarzenberg-Czerny | Curious Variables Experiment (CURVE). Three Periodicities of BF Ara | To appear in Acta Astronomica | null | null | null | astro-ph | null | We report CCD photometry of the dwarf nova BF Ara throughout fifteen
consecutive nights in quiescence. Light curve in this interval is dominated by
a large amplitude around 0.8 mag modulation consisting two periods. Higher
amplitude signal is characterized by period of 0.082159(4) days, which was
increasing at the rate of dotP/Psh = 3.8(3)* 10^{-5}. Weaker and stable signal
has period of 0.084176(21) days. Knowing the superhump period of BF Ara
determined by Kato et al. (2003) and equal to 0.08797(1) days, the first
modulation is interpreted as quiescent negative superhump arising from
retrograde precesion of titled accretion disk and the latter one as an orbital
period of the binary. The respective period excess and defect are epsilon_+ =
4.51% +/- 0.03% and epsilon_- = -2.44% +/- 0.02%. Thus BF Ara is yet another
in-the-gap nova with mass ratio q of around 0.21.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 21:19:40 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Olech",
"A.",
""
],
[
"Rutkowski",
"A.",
""
],
[
"Schwarzenberg-Czerny",
"A.",
""
]
] | [
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] |
801.1682 | Rongwei Hu | Rongwei Hu, K. Lauritch-Kullas, J. O Brian, V. F. Mitrovic and C.
Petrovic | Anisotropy of Electrical Transport and Superconductivity in Metal Chains
of Nb2Se3 | 5 pages, 5 figures | Phys. Rev. B 75, 064517 (2007) | 10.1103/PhysRevB.75.064517 | null | cond-mat.supr-con cond-mat.mtrl-sci | null | In this work we have shown bulk superconductivity and studied the anisotropy
in both the normal and superconducting states in quasi-1D conductor Nb2Se3.
Electron - electron Umklapp scattering dominates electronic transport along the
direction of Nb metal chains as well as perpendicular to it. The
superconducting state is rather anisotropic with possible multi - band
features.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 03:23:24 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hu",
"Rongwei",
""
],
[
"Lauritch-Kullas",
"K.",
""
],
[
"Brian",
"J. O",
""
],
[
"Mitrovic",
"V. F.",
""
],
[
"Petrovic",
"C.",
""
]
] | [
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] |
801.1683 | Igor Pisnichenko | F. I. Pisnichenko, I. A. Pisnichenko, J. M. Martinez, S. A. Santos | Continuing dynamic assimilation of the inner region data in
hydrodynamics modelling: Optimization approach | Paper contents 14 pages and 12 figures. Some results of this work was
presented on the sixth international conference on optimization,
OPTIMIZATION2007, Porto, Portugal, July 22-25,2007 | null | null | null | physics.ao-ph physics.comp-ph | null | In meteorological and oceanological studies the classical approach for
finding the numerical solution of the regional model consists in formulating
and solving the Cauchy-Dirichlet problem. The related boundary conditions are
obtained by linear interpolation of data available on a coarse grid (global
data), to the boundary of regional model. Errors, in boundary conditions,
appearing owing to linear interpolation may lead to increasing errors in
numerical solution during integration. The methods developed to reduce these
errors deal with continuous dynamic assimilation of known global data available
inside the regional domain. Essentially, this assimilation procedure performs a
nudging of large-scale component of regional model solution to large-scale
global data component by introducing the relaxation forcing terms into the
regional model equations. As a result, the obtained solution is not a valid
numerical solution of the original regional model. In this work we propose the
optimization approach which is free from the above-mentioned shortcoming. The
formulation of the joint problem of finding the regional model solution and
data assimilation, as a PDE-constrained optimization problem, gives the
possibility to obtain the exact numerical solution of the regional model. Three
simple model examples (ODE Burgers equation, Rossby-Oboukhov equation,
Korteweg-de Vries equation) were considered in this paper. The result of
performed numerical experiments indicates that the optimization approach can
significantly improve the precision of the sought numerical solution, even in
the cases in which the solution of Cauchy-Dirichlet problem is very sensitive
to the errors in the boundary condition.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 22:04:57 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Pisnichenko",
"F. I.",
""
],
[
"Pisnichenko",
"I. A.",
""
],
[
"Martinez",
"J. M.",
""
],
[
"Santos",
"S. A.",
""
]
] | [
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] |
801.1684 | Benjamin Brown | Benjamin P. Brown (1), Matthew K. Browning (2), Allan Sacha Brun (1
and 3), Mark S. Miesch (4), Nicholas J. Nelson (1) and Juri Toomre (1) ((1)
JILA and Dept. of Astrophysical and Planetary Sciences, University of
Colorado, Boulder, (2) Dept. of Astronomy, University of California,
Berkeley, (3) DSM/DAPNIA/SAp, CEA Saclay, Gif sur Yvette, France, (4) High
Altitude Observatory, NCAR, Boulder) | Strong Dynamo Action in Rapidly Rotating Suns | 8 pages, 4 figs. Published in conference proceedings "Unsolved
Problems in Stellar Physics", held July 2-6 2007 Cambridge, England | AIP Conf.Proc.948:271-278,2007 | 10.1063/1.2818981 | null | astro-ph | null | Stellar dynamos are driven by complex couplings between rotation and
turbulent convection, which drive global-scale flows and build and rebuild
stellar magnetic fields. When stars like our sun are young, they rotate much
more rapidly than the current solar rate. Observations generally indicate that
more rapid rotation is correlated with stronger magnetic activity and perhaps
more effective dynamo action. Here we examine the effects of more rapid
rotation on dynamo action in a star like our sun. We find that vigorous dynamo
action is realized, with magnetic field generated throughout the bulk of the
convection zone. These simulations do not possess a penetrative tachocline of
shear where global-scale fields are thought to be organized in our sun, but
despite this we find strikingly ordered fields, much like sea-snakes of
toroidal field, which are organized on global scales. We believe this to be a
novel finding.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 21:29:44 GMT"
}
] | 2009-06-25T00:00:00 | [
[
"Brown",
"Benjamin P.",
"",
"1\n and 3"
],
[
"Browning",
"Matthew K.",
"",
"1\n and 3"
],
[
"Brun",
"Allan Sacha",
"",
"1\n and 3"
],
[
"Miesch",
"Mark S.",
""
],
[
"Nelson",
"Nicholas J.",
""
],
[
"Toomre",
"Juri",
""
]
] | [
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] |
801.1685 | David Anderson | D. R. Anderson, M. Gillon, C. Hellier, P. F. L. Maxted, F. Pepe, D.
Queloz, D. M. Wilson, A. Collier Cameron, B. Smalley, T. A. Lister, S. J.
Bentley, A. Blecha, D. J. Christian, B. Enoch, L. Hebb, K. Horne, J. Irwin,
Y. C. Joshi, S. R. Kane, M. Marmier, M. Mayor, N. R. Parley, D. L. Pollacco,
F. Pont, R. Ryans, D. S\'egransan, I. Skillen, R. A. Street, S. Udry, R. G.
West, P. J. Wheatley | WASP-5b: a dense, very-hot Jupiter transiting a 12th-mag
Southern-hemisphere star | 4 pages, 4 figures, 4 tables, submitted to MNRAS Letters. Corrected
vsini value and therefore age estimate. Added reference. Corrected error bars
in Fig 4. Changed some wording | null | 10.1111/j.1745-3933.2008.00465.x | null | astro-ph | null | We report the discovery of WASP-5b, a Jupiter-mass planet orbiting a 12th-mag
G-type star in the Southern hemisphere. The 1.6-d orbital period places WASP-5b
in the class of very-hot Jupiters and leads to a predicted equilibrium
temperature of 1750 K. WASP-5b is the densest of any known Jovian-mass planet,
being a factor seven denser than TrES-4, which is subject to similar stellar
insolation, and a factor three denser than WASP-4b, which has a similar orbital
period. We present transit photometry and radial-velocity measurements of
WASP-5 (= USNO-B1 0487-0799749), from which we derive the mass, radius and
density of the planet: M_P = 1.58 +0.13 -0.08 M_J, R_P = 1.090 +0.094 -0.058
R_J and Rho_P = 1.22 +0.19 -0.24 Rho_J. The orbital period is P = 1.6284296
+0.0000048 -0.0000037 d and the mid-transit epoch is T_C (HJD) = 2454375.62466
+0.00026 -0.00025.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 22:00:19 GMT"
},
{
"version": "v2",
"created": "Fri, 22 Feb 2008 01:31:34 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Anderson",
"D. R.",
""
],
[
"Gillon",
"M.",
""
],
[
"Hellier",
"C.",
""
],
[
"Maxted",
"P. F. L.",
""
],
[
"Pepe",
"F.",
""
],
[
"Queloz",
"D.",
""
],
[
"Wilson",
"D. M.",
""
],
[
"Cameron",
"A. Collier",
""
],
[
"Smalley",
"B.",
""
],
[
"Lister",
"T. A.",
""
],
[
"Bentley",
"S. J.",
""
],
[
"Blecha",
"A.",
""
],
[
"Christian",
"D. J.",
""
],
[
"Enoch",
"B.",
""
],
[
"Hebb",
"L.",
""
],
[
"Horne",
"K.",
""
],
[
"Irwin",
"J.",
""
],
[
"Joshi",
"Y. C.",
""
],
[
"Kane",
"S. R.",
""
],
[
"Marmier",
"M.",
""
],
[
"Mayor",
"M.",
""
],
[
"Parley",
"N. R.",
""
],
[
"Pollacco",
"D. L.",
""
],
[
"Pont",
"F.",
""
],
[
"Ryans",
"R.",
""
],
[
"Ségransan",
"D.",
""
],
[
"Skillen",
"I.",
""
],
[
"Street",
"R. A.",
""
],
[
"Udry",
"S.",
""
],
[
"West",
"R. G.",
""
],
[
"Wheatley",
"P. J.",
""
]
] | [
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801.1686 | Arturo Avelino Huerta | Arturo Avelino, U. Nucamendi and F. S. Guzm\'an (Instituto de F\'isica
y Matem\'aticas, Universidad Michoacana de San Nicol\'as de Hidalgo, Morelia,
Michoac\'an, M\'exico) | Constraining a bulk viscous matter-dominated cosmological model using
SNe Ia, CMB and LSS | 4 pages, 1 figure. Work presented in the XI Mexican Workshop on
Particles and Fields, Tuxtla Gutierrez, Mexico, nov 7-12, 2007. Submitted to
AIP Conference Proceedings of this conference | AIP Conf.Proc.1026:300-302,2008 | 10.1063/1.2965067 | null | gr-qc astro-ph | null | We present and constrain a cosmological model which component is a
pressureless fluid with bulk viscosity as an explanation for the present
accelerated expansion of the universe. We study the particular model of a
constant bulk viscosity coefficient \zeta_m. The possible values of \zeta_m are
constrained using the cosmological tests of SNe Ia Gold 2006 sample, the CMB
shift parameter R from the three-year WMAP observations, the Baryon Acoustic
Oscillation (BAO) peak A from the Sloan Digital Sky Survey (SDSS) and the
Second Law of Thermodynamics (SLT). It was found that this model is in
agreement with the SLT using only the SNe Ia test. However when the model is
submitted to the three cosmological tests together (SNe+CMB+BAO) the results
are: 1.- the model violates the SLT, 2.- predicts a value of H_0 \approx 53 km
sec^{-1} Mpc^{-1} for the Hubble constant, and 3.- we obtain a bad fit to data
with a \chi^2_{min} \approx 400 (\chi^2_{d.o.f.} \approx 2.2). These results
indicate that this model is ruled out by the observations.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 21:26:07 GMT"
}
] | 2009-03-24T00:00:00 | [
[
"Avelino",
"Arturo",
"",
"Instituto de Física\n y Matemáticas, Universidad Michoacana de San Nicolás de Hidalgo, Morelia,\n Michoacán, México"
],
[
"Nucamendi",
"U.",
"",
"Instituto de Física\n y Matemáticas, Universidad Michoacana de San Nicolás de Hidalgo, Morelia,\n Michoacán, México"
],
[
"Guzmán",
"F. S.",
"",
"Instituto de Física\n y Matemáticas, Universidad Michoacana de San Nicolás de Hidalgo, Morelia,\n Michoacán, México"
]
] | [
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] |
801.1687 | Jad Saklawi | Paul C. Attie | Synthesis of Large Dynamic Concurrent Programs from Dynamic
Specifications | 46 pages | null | null | null | cs.LO | null | We present a tractable method for synthesizing arbitrarily large concurrent
programs, for a shared memory model with common hardware-available primitives
such as atomic registers, compare-and-swap, load-linked/store conditional, etc.
The programs we synthesize are dynamic: new processes can be created and added
at run-time, and so our programs are not finite-state, in general.
Nevertheless, we successfully exploit automatic synthesis and model-checking
methods based on propositional temporal logic. Our method is algorithmically
efficient, with complexity polynomial in the number of component processes (of
the program) that are ``alive'' at any time. Our method does not explicitly
construct the automata-theoretic product of all processes that are alive,
thereby avoiding \intr{state explosion}. Instead, for each pair of processes
which interact, our method constructs an automata-theoretic product
(\intr{pair-machine}) which embodies all the possible interactions of these two
processes. From each pair-machine, we can synthesize a correct
\intr{pair-program} which coordinates the two involved processes as needed. We
allow such pair-programs to be added dynamically at run-time. They are then
``composed conjunctively'' with the currently alive pair-programs to
re-synthesize the program as it results after addition of the new pair-program.
We are thus able to add new behaviors, which result in new properties being
satisfied, at run-time. We establish a ``large model'' theorem which shows that
the synthesized large program inherits correctness properties from the
pair-programs.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 21:27:42 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Attie",
"Paul C.",
""
]
] | [
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] |
801.1688 | Rongwei Hu | Rongwei Hu, R. P. Hermann, F. Grandjean, Y. Lee, J. B. Warren, V. F.
Mitrovic and C. Petrovic | Weak Ferromagnetism in Fe1-xCoxSb2 | 6 pages, 7 figures | Phys. Rev. B 76, 224422 (2007) | 10.1103/PhysRevB.76.224422 | null | cond-mat.str-el cond-mat.mtrl-sci | null | Weak ferromagnetism in Fe1-xCoxSb2 is studied by magnetization and Mossbauer
measurements. A small spontaneous magnetic moment of the order of 10^-3 uB
appears along the b-axis for 0.2<= x <= 0.4. Based on the structural analysis,
we argue against extrinsic sources of weak ferromagnetism. We discuss our
results in the framework of the nearly magnetic electronic structure of the
parent compound FeSb2.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 03:26:48 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Hu",
"Rongwei",
""
],
[
"Hermann",
"R. P.",
""
],
[
"Grandjean",
"F.",
""
],
[
"Lee",
"Y.",
""
],
[
"Warren",
"J. B.",
""
],
[
"Mitrovic",
"V. F.",
""
],
[
"Petrovic",
"C.",
""
]
] | [
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801.1689 | Tomasz Kami\'nski | T. Kami\'nski | Extended CO emission in the field of the light echo of V838 Mon | 6 pages, 2 figures (+2 figures in an appendix), submitted to A&A.
High resolution version of Fig. 1 at
http://www.ncac.torun.pl/~tomkam/AAII/Fig1.eps | null | 10.1051/0004-6361:20079189 | null | astro-ph | null | V838 Mon erupted at the beginning of 2002 becoming an extremely luminous star
with L=10^6 L_sun. The outburst was followed by the spectacular light echo that
revealed that the star is immersed in a diffuse and dusty medium, plausibly
interstellar in nature. Low angular resolution observations in the lowest CO
rotational transitions revealed a molecular emission from the direction of V838
Mon. The origin of this CO emission has not been established. In this paper we
investigate the idea that the molecular emission originates in the material
responsible for the optical light echo. We report on observations of 13
positions within the light echo in the two lowest rotational transitions of CO
using the IRAM 30 m telescope. Emission in CO J=1-0 and J=2-1 was detected in
three positions. In three other positions only weak J=1-0 lines were found. We
conclude that the molecular emission from the direction of V838 Mon is extended
and has a complex distribution. We identify the emission as arising from
diffuse interstellar clouds and suggest that the CO-bearing gas and the echoing
dust are collocated in the same interstellar cloud.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 22:16:29 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kamiński",
"T.",
""
]
] | [
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801.169 | Kwok Sau Fa | Kwok Sau Fa | Nonlocal description of a falling body through the air | 14 pages and 3 figures | null | null | null | physics.gen-ph physics.class-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In this present work we consider a falling body through the air under the
influence of gravity. In particular, we consider the experimental data based
upon the free fall of six men in the atmosphere of the earth. In order to
describe this process we employ a nonlocal dissipative force. We show that our
description, by using an exponential memory kernel, can fit the experimental
data as well as that of a local dissipative force.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 21:54:26 GMT"
},
{
"version": "v2",
"created": "Thu, 2 Oct 2008 22:22:51 GMT"
}
] | 2008-10-03T00:00:00 | [
[
"Fa",
"Kwok Sau",
""
]
] | [
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801.1691 | James M. Borger | James Borger | The basic geometry of Witt vectors, I: The affine case | Final version | Algebra & Number Theory 5 (2011), no. 2, pp 231-285 | null | null | math.AG math.CT math.NT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We give a concrete description of the category of etale algebras over the
ring of Witt vectors of a given finite length with entries in an arbitrary
ring. We do this not only for the classical p-typical and big Witt vector
functors but also for variants of these functors which are in a certain sense
their analogues over arbitrary local and global fields. The basic theory of
these generalized Witt vectors is developed from the point of view of commuting
Frobenius lifts and their universal properties, which is a new approach even
for the classical Witt vectors. The larger purpose of this paper is to provide
the affine foundations for the algebraic geometry of generalized Witt schemes
and arithmetic jet spaces. So the basics here are developed somewhat fully,
with an eye toward future applications.
| [
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"created": "Mon, 14 Dec 2015 02:02:42 GMT"
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] | 2015-12-15T00:00:00 | [
[
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"James",
""
]
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] |
801.1692 | Michael Eracleous | Toru Misawa, Michael Eracleous, George Chartas, Jane C. Charlton (Penn
State) | Exploratory Study of the X-Ray Properties of Quasars With Intrinsic
Narrow Absorption Lines | Accepted by the Astrophysical Journal | null | 10.1086/529426 | null | astro-ph | null | We have used archival Chandra and XMM-Newton observations of quasars hosting
intrinsic narrow UV absorption lines (intrinsic NALs) to carry out an
exploratory survey of their X-ray properties. Our sample consists of three
intrinsic-NAL quasars and one "mini-BAL" quasar, plus four quasars without
intrinsic absorption lines for comparison. These were drawn in a systematic
manner from an optical/UV-selected sample. The X-ray properties of
intrinsic-NAL quasars are indistinguishable from those of "normal" quasars. We
do not find any excess absorption in quasars with intrinsic NALs, with upper
limits of a few times 10^22 cm^-2. We compare the X-ray and UV properties of
our sample quasars by plotting the equivalent width and blueshift velocity of
the intrinsic NALs and the X-ray spectral index against the "optical-to-X-ray"
slope, alpha-ox. When BAL quasars and other AGNs with intrinsic NALs are
included, the plots suggest that intrinsic-NAL quasars form an extension of the
BAL sequences and tend to bridge the gap between BAL and "normal" quasars.
Observations of larger samples of intrinsic-NAL quasars are needed to verify
these conclusions. We also test two competing scenarios for the location of the
NAL gas in an accretion-disk wind. Our results strongly support a location of
the NAL gas at high latitudes above the disk, closer to the disk axis than the
dense BAL wind. We detect excess X-ray absorption only in Q0014+8118, which
does not host intrinsic NALs. The absorbing medium very likely corresponds to
an intervening system at z=1.1, which also produces strong absorption lines in
the rest-frame UV spectrum of this quasar. In the appendix we discuss the
connection between UV and X-ray attenuation and its effect on alpha-ox.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 22:22:33 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Misawa",
"Toru",
"",
"Penn\n State"
],
[
"Eracleous",
"Michael",
"",
"Penn\n State"
],
[
"Chartas",
"George",
"",
"Penn\n State"
],
[
"Charlton",
"Jane C.",
"",
"Penn\n State"
]
] | [
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] |
801.1693 | Christopher Herzog | Sean A. Hartnoll and Christopher P. Herzog | Impure AdS/CFT | 26 pages, 11 figures; v2 ref added | Phys.Rev.D77:106009,2008 | 10.1103/PhysRevD.77.106009 | null | hep-th cond-mat.str-el | null | We study momentum relaxation due to dilute, weak impurities in a strongly
coupled CFT, a truncation of the M2 brane theory. Using the AdS/CFT
correspondence, we compute the relaxation time scale as a function of the
background magnetic field B and charge density \rho. The theory admits two
different types of impurities. We find that for magnetic impurities, momentum
relaxation due to the impurity is suppressed by a background B or \rho. For
electric impurities, due to an underlying instability in the theory towards an
ordered phase, the inverse relaxation time scale increases dramatically near
\sqrt{B^2 + \rho^2/\sigma^2_0} \sim 21 T^2. We compute the Nernst response for
the impure theory, and comment on similarities with recent measurements in
superconductors.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 16:35:31 GMT"
},
{
"version": "v2",
"created": "Thu, 14 Feb 2008 22:40:49 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Hartnoll",
"Sean A.",
""
],
[
"Herzog",
"Christopher P.",
""
]
] | [
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] |
801.1694 | Alexander Bolonkin | Alexander Bolonkin | Cheap Method for Shielding a City from Rocket and Nuclear Warhead
Impacts | 31 pages, 11 figures, 4 tables | null | null | null | physics.gen-ph physics.soc-ph | null | The author suggests a cheap closed AB-Dome which protects the densely
populated cities from nuclear, chemical, biological weapon (bombs) delivered by
warheads, strategic missiles, rockets, and various incarnations of aviation
technology. The offered AB-Dome is also very useful in peacetime because it
shields a city from exterior weather and creates a fine climate within the
AB-Dome. The hemispherical AB-Dome is the inflatable, thin transparent film,
located at altitude up to as much as 15 km, which converts the city into a
closed-loop system. The film may be armored the stones which destroy the
rockets and nuclear warhead. AB-Dome protects the city in case the World
nuclear war and total poisoning the Earth atmosphere by radioactive fallout
(gases and dust). Construction of the AB-Dome is easy; the enclosure film is
spread upon the ground, the air pump is turned on, and the cover rises to its
planned altitude and supported by a small air over-pressure. The offered method
is cheaper by thousand times than protection of city by current anti-rocket
systems. The AB-Dome may be also used (height up to 15 and more kilometers) for
TV, communication, telescope, long distance location, tourism, high placed
windmills (energy), illumination and entertainments. The author developed
theory of AB-Dome, made estimation, computation and computed a typical project.
Discussion and results are in the end of article.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 23:23:53 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Bolonkin",
"Alexander",
""
]
] | [
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] |
801.1695 | Haitao Xu | Alice M. Crawford, Nicolas Mordant, Haitao Xu, and Eberhard
Bodenschatz | Fluid Acceleration in the Bulk Turbulence of Dilute Polymer Solutions | 5 pages, 4 figures | null | 10.1088/1367-2630/10/12/123015 | null | physics.flu-dyn | null | We report experimental measurements of Lagrangian accelerations in the bulk
of intense turbulent flows of dilute polymer solutions by following tracer
particles with a high-speed optical tracking system. We observed a significant
decrease in the acceleration variance in dilute polymer solutions. The shape of
the normalized acceleration probability density functions, however, remain the
same as in Newtonian water flows. We also observed an increase in the turbulent
Lagrangian acceleration autocorrelation time in these dilute polymer solutions.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 23:41:40 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Crawford",
"Alice M.",
""
],
[
"Mordant",
"Nicolas",
""
],
[
"Xu",
"Haitao",
""
],
[
"Bodenschatz",
"Eberhard",
""
]
] | [
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] |
801.1696 | Flemming Videb{\ae}k | F.Videbaek (for the BRAHMS collaboration) | Results from pp at 62.4 GeV and 200 GeV with the BRAHMS experiment | 8 pages with 5 figures. Proceedings for the 23winter workshop on
nuclear dynamics. Big Sky Montana,USA 11-18, 2007 | null | null | null | nucl-ex | null | Measurements of elementary pp collisions are an integral component to
understand heavy ion collisions. Results for pp collisions at 200 and 62.4 GeV
are presented. At both energies NLO pQCD describes pion production well. The
measured pion transverse single spin asymmetries are very large at 62.4 GeV and
are reasonably well described by models relying on pQCD at transverse momenta
larger than 1 GeV/c.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 23:46:48 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Videbaek",
"F.",
"",
"for the BRAHMS collaboration"
]
] | [
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] |
801.1697 | Scott Bergeson | S. D. Bergeson, J. B. Peatross, N. J. Eyring, J. F. Fralick, D. N.
Stevenson, and S. B. Ferguson | Resonance Raman measurements of carotenoids using light emitting diodes | Accepted for publication by the Journal of Biomedical Optics | null | 10.1117/1.2952075 | null | physics.med-ph physics.optics | null | We report on the development of a compact commercial instrument for measuring
carotenoids in skin tissue. The instrument uses two light emitting diodes
(LEDs) for dual-wavelength excitation and four photomultiplier tubes for
multichannel detection. Bandpass filters are used to select the excitation and
detection wavelengths. The f/1.3 optical system has high optical throughput and
single photon sensitivity, both of which are crucial in LED-based Raman
measurements. We employ a signal processing technique that compensates for
detector drift and error. The sensitivity and reproducibility of the LED Raman
instrument compares favorably to laser-based Raman spectrometers. This compact,
portable instrument is used for non-invasive measurement of carotenoid
molecules in human skin with a repeatability better than 10%.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 23:51:52 GMT"
},
{
"version": "v2",
"created": "Fri, 15 Feb 2008 19:54:04 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Bergeson",
"S. D.",
""
],
[
"Peatross",
"J. B.",
""
],
[
"Eyring",
"N. J.",
""
],
[
"Fralick",
"J. F.",
""
],
[
"Stevenson",
"D. N.",
""
],
[
"Ferguson",
"S. B.",
""
]
] | [
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] |
801.1698 | Tim Austin | Tim Austin | On exchangeable random variables and the statistics of large graphs and
hypergraphs | Published in at http://dx.doi.org/10.1214/08-PS124 the Probability
Surveys (http://www.i-journals.org/ps/) by the Institute of Mathematical
Statistics (http://www.imstat.org) | Probability Surveys 2008, Vol. 5, 80-145 | 10.1214/08-PS124 | IMS-PS-PS_2008_124 | math.PR math.CO | null | De Finetti's classical result of [18] identifying the law of an exchangeable
family of random variables as a mixture of i.i.d. laws was extended to
structure theorems for more complex notions of exchangeability by Aldous
[1,2,3], Hoover [41,42], Kallenberg [44] and Kingman [47]. On the other hand,
such exchangeable laws were first related to questions from combinatorics in an
independent analysis by Fremlin and Talagrand [29], and again more recently in
Tao [62], where they appear as a natural proxy for the `leading order
statistics' of colourings of large graphs or hypergraphs. Moreover, this
relation appears implicitly in the study of various more bespoke formalisms for
handling `limit objects' of sequences of dense graphs or hypergraphs in a
number of recent works, including Lov\'{a}sz and Szegedy [52], Borgs, Chayes,
Lov\'{a}sz, S\'{o}s, Szegedy and Vesztergombi [17], Elek and Szegedy [24] and
Razborov [54,55]. However, the connection between these works and the earlier
probabilistic structural results seems to have gone largely unappreciated. In
this survey we recall the basic results of the theory of exchangeable laws, and
then explain the probabilistic versions of various interesting questions from
graph and hypergraph theory that their connection motivates (particularly
extremal questions on the testability of properties for graphs and
hypergraphs). We also locate the notions of exchangeability of interest to us
in the context of other classes of probability measures subject to various
symmetries, in particular contrasting the methods employed to analyze
exchangeable laws with related structural results in ergodic theory, particular
the Furstenberg-Zimmer structure theorem for probability-preserving $\mathbb
{Z}$-systems, which underpins Furstenberg's ergodic-theoretic proof of
Szemer\'{e}di's Theorem. The forthcoming paper [10]--hereditarytest will make a
much more elaborate appeal to the link between exchangeable laws and dense
(directed) hypergraphs to establish various results in property testing.
| [
{
"version": "v1",
"created": "Thu, 10 Jan 2008 23:54:17 GMT"
},
{
"version": "v2",
"created": "Tue, 29 Apr 2008 02:14:54 GMT"
},
{
"version": "v3",
"created": "Mon, 26 May 2008 06:08:46 GMT"
}
] | 2008-05-26T00:00:00 | [
[
"Austin",
"Tim",
""
]
] | [
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] |
801.1699 | Augusto Alcalde | C. L. Romano, G. E. Marques, L. Sanz, A. M. Alcalde | Phonon modulation of the spin-orbit interaction as a spin relaxation
mechanism in quantum dots | null | null | 10.1103/PhysRevB.77.033301 | null | cond-mat.mes-hall | null | We calculate the spin relaxation rates in a parabolic InSb quantum dots due
to the spin interaction with acoustical phonons. We considered the deformation
potential mechanism as the dominant electron-phonon coupling in the
Pavlov-Firsov spin-phonon Hamiltonian. By studying suitable choices of magnetic
field and lateral dot size, we determine regions where the spin relaxation
rates can be practically suppressed. We analyze the behavior of the spin
relaxation rates as a function of an external magnetic field and mean quantum
dot radius. Effects of the spin admixture due to Dresselhaus contribution to
spin-orbit interaction are also discussed.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 00:20:06 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Romano",
"C. L.",
""
],
[
"Marques",
"G. E.",
""
],
[
"Sanz",
"L.",
""
],
[
"Alcalde",
"A. M.",
""
]
] | [
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] |
801.17 | C. W. Engelbracht | C. W. Engelbracht, G. H. Rieke, K. D. Gordon, J.-D. T. Smith, M. W.
Werner, J. Moustakas, C. N. A. Willmer, and L. Vanzi | Metallicity Effects on Dust Properties in Starbursting Galaxies | 34 pages, 11 figures, accepted to ApJ | Astrophys.J.678:804-827,2008 | 10.1086/529513 | null | astro-ph | null | We present infrared observations of 66 starburst galaxies over a wide range
of oxygen abundances, to measure how metallicity affects their dust properties.
The data include imaging and spectroscopy from the Spitzer Space Telescope,
supplemented by groundbased near-infrared imaging. We confirm a strong
correlation of aromatic emission with metallicity, with a threshold at a
metallicity [12+log(O/H)]~8. The large scatter in both the metallicity and
radiation hardness dependence of this behavior implies that it is not due to a
single effect, but to some combination. We show that the far-infrared color
temperature of the large dust grains increases towards lower metallicity,
peaking at a metallicity of 8 before turning over. We compute dust masses and
compare them to HI masses from the literature to derive the gas to dust ratio,
which increases by nearly 3 orders of magnitude between solar metallicity and a
metallicity of 8, below which it flattens out. The abrupt change in aromatic
emission at mid-infrared wavelengths thus appears to be reflected in the
far-infrared properties, indicating that metallicity changes affect the
composition of the full range of dust grain sizes that dominate the infrared
emission. In addition, we find that the ratio L(8 micron)/L(TIR), important for
calibrating 24 micron measurements of high redshift galaxies, increases
slightly as the metallicity decreases from ~solar to ~50% of solar, and then
decreases by an order of magnitude with further decreases in metallicity.
Although the great majority of galaxies show similar patterns of behavior as
described above, there are three exceptions, SBS 0335-052E, Haro 11, and SHOC
391. Their infrared SEDs are dominated energetically by the mid-IR near 24
micron rather than by the 60 - 200 micron region. (Abridged)
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 00:24:18 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Engelbracht",
"C. W.",
""
],
[
"Rieke",
"G. H.",
""
],
[
"Gordon",
"K. D.",
""
],
[
"Smith",
"J. -D. T.",
""
],
[
"Werner",
"M. W.",
""
],
[
"Moustakas",
"J.",
""
],
[
"Willmer",
"C. N. A.",
""
],
[
"Vanzi",
"L.",
""
]
] | [
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] |
801.1701 | Guozhen Lu | Yongsheng Han and Guozhen Lu | Discrete Littlewood-Paley-Stein theory and multi-parameter Hardy spaces
associated with flag singular integrals | 50 pages | null | null | null | math.CA | null | The main purpose of this paper is to develop a unified approach of
multi-parameter Hardy space theory using the discrete Littlewood-Paley-Stein
analysis in the setting of implicit multi-parameter structure. It is motivated
by the goal to establish and develop the Hardy space theory for the flag
singular integral operators studied by Muller-Ricci-Stein and
Nagel-Ricci-Stein. This approach enables us to avoid the use of transference
method of Coifman-Weiss as often used in the $L^p$ theory for $p>1$ and
establish the Hardy spaces $H^p_F$ and its dual spaces associated with the flag
singular integral operators for all $0<p\leq 1$. We also prove the boundedness
of flag singular integral operators on $BMO_F$ and $H^p_F$, and from $H^p_F$ to
$L^p$ for all $0<p\le 1$ without using the deep atomic decomposition. As a
result, it bypasses the use of Journe's type covering lemma in this implicit
multi-parameter structure. The method used here provides alternate approaches
of those developed by Chang, R. Fefferman, Journe and Pipher in the pure
product setting. A Calderon-Zygmund decomposition and interpolation theorem are
also proved for the implicit multi-parameter Hardy spaces.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 00:54:50 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Han",
"Yongsheng",
""
],
[
"Lu",
"Guozhen",
""
]
] | [
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] |
801.1702 | Noriaki Kitazawa | Noriaki Kitazawa | Tadpole Resummations in String Theory | 14 pages | Phys.Lett.B660:415-421,2008 | 10.1016/j.physletb.2008.01.028 | null | hep-th | null | While R-R tadpoles should be canceled for consistency, string models with
broken supersymmetry generally have uncanceled NS-NS tadpoles. Their presence
signals that the background does not solve the field equations, so that these
models are in "wrong" vacua. In this letter we investigate, with reference to
some prototype examples, whether the true values of physical quantities can be
recovered resumming the NS-NS tadpoles, hence by an approach that is related to
the analysis based on String Field Theory by open-closed duality. We show that,
indeed, the positive classical vacuum energy of a Dp-brane of the bosonic
string is exactly canceled by the negative contribution arising from tree-level
tadpole resummation, in complete agreement with Sen's conjecture on open-string
tachyon condensation and with the consequent analysis based on String Field
Theory. We also show that the vanishing classical vacuum energy of the SO(8192)
unoriented bosonic open-string theory does not receive any tree-level
corrections from the tadpole resummation. This result is consistent with the
fact that this (unstable) configuration is free from tadpoles of massless
closed-string modes, although there is a tadpole of the closed string tachyon.
The application of this method to superstring models with broken supersymmetry
is also discussed.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 01:08:03 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Kitazawa",
"Noriaki",
""
]
] | [
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] |
801.1703 | Milan Derpich | Milan S. Derpich, Jan Ostergaard and Graham C. Goodwin | The Quadratic Gaussian Rate-Distortion Function for Source Uncorrelated
Distortions | Revised version, to be presented at the Data Compression Conference
2008 | null | null | null | cs.IT math.IT | null | We characterize the rate-distortion function for zero-mean stationary
Gaussian sources under the MSE fidelity criterion and subject to the additional
constraint that the distortion is uncorrelated to the input. The solution is
given by two equations coupled through a single scalar parameter. This has a
structure similar to the well known water-filling solution obtained without the
uncorrelated distortion restriction. Our results fully characterize the unique
statistics of the optimal distortion. We also show that, for all positive
distortions, the minimum achievable rate subject to the uncorrelation
constraint is strictly larger than that given by the un-constrained
rate-distortion function. This gap increases with the distortion and tends to
infinity and zero, respectively, as the distortion tends to zero and infinity.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 01:37:56 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Derpich",
"Milan S.",
""
],
[
"Ostergaard",
"Jan",
""
],
[
"Goodwin",
"Graham C.",
""
]
] | [
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] |
801.1704 | Shao-Ming Fei | Zu-Huan Yu, Xian-Qing Li-Jost and Shao-Ming Fei | Representation Class and Geometrical Invariants of Quantum States under
Local Unitary Transformations | 11 pages | Int. J. Quant. Inform. 5(2007)795-803 | 10.1142/S0219749907003262 | null | quant-ph | null | We investigate the equivalence of bipartite quantum mixed states under local
unitary transformations by introducing representation classes from a
geometrical approach. It is shown that two bipartite mixed states are
equivalent under local unitary transformations if and only if they have the
same representation class. Detailed examples are given on calculating
representation classes.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 01:27:08 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Yu",
"Zu-Huan",
""
],
[
"Li-Jost",
"Xian-Qing",
""
],
[
"Fei",
"Shao-Ming",
""
]
] | [
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] |
801.1705 | Ping Wang | Zhe Chang, Ping Wang, and Ying-Hong Zheng | Ashkin-Teller formalism for elastic response of DNA molecule to external
force and torque | 5 pages, 7 figures | null | 10.1088/0253-6102/49/2/57 | null | physics.bio-ph cond-mat.soft | null | We propose an Ashkin-Teller like model for elastic response of DNA molecule
to external force and torque. The base-stacking interaction is described in a
simple and uniform way. We obtain the phase diagram of dsDNA, and in
particular, the transition from B form to the S state induced by stretching and
twisting. The elastic response of the ssDNA is presented also in a unified
formalism. The close relation of dsDNA molecule structure with elastic response
is shown clearly. The calculated folding angle of the dsDNA molecule is
$59.2^o$.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 01:35:08 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Chang",
"Zhe",
""
],
[
"Wang",
"Ping",
""
],
[
"Zheng",
"Ying-Hong",
""
]
] | [
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] |
801.1706 | Shao-Ming Fei | Xiao-Hong Wang, Shao-Ming Fei and Ke Wu | A Complete Set of Local Invariants for a Family of Multipartite Mixed
States | 10 pages | J. Phys. A 41, Math. Theor. (2008) 025305 | 10.1088/1751-8113/41/2/025305 | null | quant-ph | null | We study the equivalence of quantum states under local unitary
transformations by using the singular value decomposition. A complete set of
invariants under local unitary transformations is presented for several classes
of tripartite mixed states in KxMxN composite systems. Two density matrices in
the same class are equivalent under local unitary transformations if and only
if all these invariants have equal values for these density matrices.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 01:50:16 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Wang",
"Xiao-Hong",
""
],
[
"Fei",
"Shao-Ming",
""
],
[
"Wu",
"Ke",
""
]
] | [
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] |
801.1707 | Fabio Governato | F.Governato (UW), L.Mayer (U. of Zurich & ETH), C.Brook (UW) | The Formation of Galaxy Disks | To appear in proceedings of "Formation and Evolution of Galaxy
Disks", Rome, October 2007, Eds. J.G. Funes, S.J. and E.M. Corsini. Bigger
figures than in printed version | null | null | null | astro-ph | null | We present a new set of multi-million particle SPH simulations of the
formation of disk dominated galaxies in a cosmological context. Some of these
galaxies are higher resolution versions of the models already described in
Governato et al (2007). To correctly compare simulations with observations we
create artificial images of our simulations and from them measure photometric
Bulge to Disk (B/D) ratios and disk scale lengths. We show how feedback and
high force and mass resolution are necessary ingredients to form galaxies that
have flatter rotation curves, larger I band disk scale lengths and smaller B/D
ratios. A new simulated disk galaxy has an I-band disk scale length of 9.2 kpc
and a B/D flux ratio of 0.64 (face on, dust reddened).
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 02:04:53 GMT"
},
{
"version": "v2",
"created": "Mon, 14 Jan 2008 17:07:12 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Governato",
"F.",
"",
"UW"
],
[
"Mayer",
"L.",
"",
"U. of Zurich & ETH"
],
[
"Brook",
"C.",
"",
"UW"
]
] | [
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] |
801.1708 | Matthew Wood | M. Wood, G. Blaylock, S. M. Bradbury, J. H. Buckley, K. L. Byrum, Y.
C. K. Chow, W. Cui, I. de la Calle Perez, A. D. Falcone, S. J. Fegan, J. P.
Finley, J. Grube, J. Hall, D. Hanna, J. Holder, D. Horan, T. B. Humensky, D.
B. Kieda, J. Kildea, A. Konopelko, H. Krawczynski, F. Krennrich, M. J. Lang,
S. LeBohec, T. Nagai, R. A. Ong, J. S. Perkins, M. Pohl, J. Quinn, H. J.
Rose, G. H. Sembroski, V. V. Vassiliev, R. G. Wagner, S. P. Wakely, T. C.
Weekes, A. Weinstein | A Search for Dark Matter Annihilation with the Whipple 10m Telescope | 33 pages, 12 figures, accepted for publication in the Astrophysical
Journal | null | 10.1086/529421 | null | astro-ph | null | We present observations of the dwarf galaxies Draco and Ursa Minor, the local
group galaxies M32 and M33, and the globular cluster M15 conducted with the
Whipple 10m gamma-ray telescope to search for the gamma-ray signature of
self-annihilating weakly interacting massive particles (WIMPs) which may
constitute astrophysical dark matter (DM). We review the motivations for
selecting these sources based on their unique astrophysical environments and
report the results of the data analysis which produced upper limits on excess
rate of gamma rays for each source. We consider models for the DM distribution
in each source based on the available observational constraints and discuss
possible scenarios for the enhancement of the gamma-ray luminosity. Limits on
the thermally averaged product of the total self-annihilation cross section and
velocity of the WIMP, <\sigma v>, are derived using conservative estimates for
the magnitude of the astrophysical contribution to the gamma-ray flux. Although
these limits do not constrain predictions from the currently favored
theoretical models of supersymmetry (SUSY), future observations with VERITAS
will probe a larger region of the WIMP parameter phase space, <\sigma v> and
WIMP particle mass (m_\chi).
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 02:05:51 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Wood",
"M.",
""
],
[
"Blaylock",
"G.",
""
],
[
"Bradbury",
"S. M.",
""
],
[
"Buckley",
"J. H.",
""
],
[
"Byrum",
"K. L.",
""
],
[
"Chow",
"Y. C. K.",
""
],
[
"Cui",
"W.",
""
],
[
"Perez",
"I. de la Calle",
""
],
[
"Falcone",
"A. D.",
""
],
[
"Fegan",
"S. J.",
""
],
[
"Finley",
"J. P.",
""
],
[
"Grube",
"J.",
""
],
[
"Hall",
"J.",
""
],
[
"Hanna",
"D.",
""
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[
"Holder",
"J.",
""
],
[
"Horan",
"D.",
""
],
[
"Humensky",
"T. B.",
""
],
[
"Kieda",
"D. B.",
""
],
[
"Kildea",
"J.",
""
],
[
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"A.",
""
],
[
"Krawczynski",
"H.",
""
],
[
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"F.",
""
],
[
"Lang",
"M. J.",
""
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[
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"S.",
""
],
[
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"T.",
""
],
[
"Ong",
"R. A.",
""
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[
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"J. S.",
""
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[
"Pohl",
"M.",
""
],
[
"Quinn",
"J.",
""
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[
"Rose",
"H. J.",
""
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[
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"G. H.",
""
],
[
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"V. V.",
""
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[
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"R. G.",
""
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[
"Wakely",
"S. P.",
""
],
[
"Weekes",
"T. C.",
""
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[
"Weinstein",
"A.",
""
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] | [
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] |
801.1709 | Igor Rodnianski | S. Klainerman, I. Rodnianski | On the breakdown criterion in General Relativity | null | null | null | null | math.AP gr-qc | null | We give a geometric criterion for the breakdown of an Einstein vacuum
space-time foliated by a constant mean curvature, or maximal, foliation. More
precisely we show that the foliated space-time can be extended as long as the
the second fundamental form and the first derivatives of the logarithm of the
lapse of the foliation remain uniformly bounded. No restrictions on the size of
the initial data are made.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 02:10:10 GMT"
}
] | 2008-01-28T00:00:00 | [
[
"Klainerman",
"S.",
""
],
[
"Rodnianski",
"I.",
""
]
] | [
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] |
801.171 | Zhi-Qiang Jiang | Zhi-Qiang Jiang, Wei-Xing Zhou (ECUST) | Multifractal analysis of Chinese stock volatilities based on partition
function approach | 14 elsart pages including 4 eps figures | Physica A 387 (19), 4881-4888 (2008) | 10.1016/j.physa.2008.04.028 | null | q-fin.ST physics.soc-ph | null | We have performed detailed multifractal analysis on the minutely volatility
of two indexes and 1139 stocks in the Chinese stock markets based on the
partition function approach. The partition function $\chi_q(s)$ scales as a
power law with respect to box size $s$. The scaling exponents $\tau(q)$ form a
nonlinear function of $q$. Statistical tests based on bootstrapping show that
the extracted multifractal nature is significant at the 1% significance level.
The individual securities can be well modeled by the $p$-model in turbulence
with $p = 0.40 \pm 0.02$. Based on the idea of ensemble averaging (including
quenched and annealed average), we treat each stock exchange as a whole and
confirm the existence of multifractal nature in the Chinese stock markets.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 02:28:41 GMT"
},
{
"version": "v2",
"created": "Mon, 18 Feb 2008 01:32:37 GMT"
}
] | 2008-12-02T00:00:00 | [
[
"Jiang",
"Zhi-Qiang",
"",
"ECUST"
],
[
"Zhou",
"Wei-Xing",
"",
"ECUST"
]
] | [
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] |
801.1711 | Robert Bluhm | Robert Bluhm | Nambu-Goldstone and Massive Modes in Gravitational Theories with
Spontaneous Lorentz Breaking | Talk presented at the Fourth Meeting on CPT and Lorentz Symmetry,
Bloomington, IN, August, 2007; 7 pages. Typos corrected | null | 10.1142/9789812779519_0020 | null | gr-qc | null | Spontaneous breaking of local Lorentz symmetry is of interest as a possible
mechanism originating from physics at the Planck scale. If such breaking
occurs, however, it raises the questions of what the fate of the
Nambu-Goldstone modes is, whether a Higgs mechanism can occur, and whether
additional massive modes (analogous to the Higgs particle) can appear. A
summary of some recent work looking at these questions is presented here.
| [
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{
"version": "v2",
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] | 2016-11-09T00:00:00 | [
[
"Bluhm",
"Robert",
""
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801.1712 | Steven Morrison | Steven K. Morrison and Yuri S. Kivshar | Observation of Enhanced Beaming from Photonic Crystal Waveguides | 4 pages, 6 figures | null | 10.1007/s00340-008-3305-y | null | physics.optics physics.gen-ph | null | We report on the experimental observation of the beaming effect in photonic
crystals enhanced via surface modes. We experimentally map the spatial field
distribution of energy emitted from a subwavelength photonic crystal waveguide
into free-space, rendering with crisp clarity the diffractionless beaming of
energy. Our experimental data agree well with our numerical studies of the
beaming enhancement in photonic crystals with modulated surfaces. Without loss
of generality, we study the beaming effect in a photonic crystal scaled to
microwave frequencies and demonstrate the technological capacity to deliver
long-range, wavelength-scaled beaming of energy.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 02:43:01 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Morrison",
"Steven K.",
""
],
[
"Kivshar",
"Yuri S.",
""
]
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801.1713 | Satoru Morita | Satoru Morita | Extended Pair Approximation of Evolutionary Game on Complex Networks | to be published in Progress of Theoretical Physics | Progress of Theoretical Physics 119, 29-38 (2008) | 10.1143/PTP.119.29 | null | physics.soc-ph physics.comp-ph | null | We investigate how network structure influences evolutionary games on
networks. We extend the pair approximation to study the effects of degree
fluctuation and clustering of the network. We find that a larger fluctuation of
the degree is equivalent to a larger mobility of the players. In addition, a
larger clustering coefficient is equivalent to a smaller number of neighbors.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 02:50:55 GMT"
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] | 2015-11-12T00:00:00 | [
[
"Morita",
"Satoru",
""
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] |
801.1714 | Christoph Freysoldt | Christoph Freysoldt, Philipp Eggert, Patrick Rinke, Arno Schindlmayr,
Matthias Scheffler | Screening in 2D: GW calculations for surfaces and thin films using the
repeated-slab approach | 11 pages, 10 figures, PRB accepted | Phys. Rev. B 77, 235428 (2008) | 10.1103/PhysRevB.77.235428 | null | cond-mat.mtrl-sci | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | In the context of photoelectron spectroscopy, the $GW$ approach has developed
into the method of choice for computing excitation spectra of weakly correlated
bulk systems and their surfaces. To employ the established computational
schemes that have been developed for three-dimensional crystals,
two-dimensional systems are typically treated in the repeated-slab approach. In
this work we critically examine this approach and identify three important
aspects for which the treatment of long-range screening in two dimensions
differs from the bulk: (1) anisotropy of the macroscopic screening (2) $\mathbf
k$-point sampling parallel to the surface (3) periodic repetition and slab-slab
interaction. For prototypical semiconductor (silicon) and ionic (NaCl) thin
films we quantify the individual contributions of points (1) to (3) and develop
robust and efficient correction schemes derived from the classic theory of
dielectric screening.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 15:21:42 GMT"
},
{
"version": "v2",
"created": "Wed, 11 Jun 2008 21:47:45 GMT"
}
] | 2008-06-20T00:00:00 | [
[
"Freysoldt",
"Christoph",
""
],
[
"Eggert",
"Philipp",
""
],
[
"Rinke",
"Patrick",
""
],
[
"Schindlmayr",
"Arno",
""
],
[
"Scheffler",
"Matthias",
""
]
] | [
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] |
801.1715 | Srivatsava Ranjit Ganta | Srivatsava Ranjit Ganta, Raj Acharya | On Breaching Enterprise Data Privacy Through Adversarial Information
Fusion | null | null | null | null | cs.DB cs.CR cs.OH | null | Data privacy is one of the key challenges faced by enterprises today.
Anonymization techniques address this problem by sanitizing sensitive data such
that individual privacy is preserved while allowing enterprises to maintain and
share sensitive data. However, existing work on this problem make inherent
assumptions about the data that are impractical in day-to-day enterprise data
management scenarios. Further, application of existing anonymization schemes on
enterprise data could lead to adversarial attacks in which an intruder could
use information fusion techniques to inflict a privacy breach. In this paper,
we shed light on the shortcomings of current anonymization schemes in the
context of enterprise data. We define and experimentally demonstrate Web-based
Information- Fusion Attack on anonymized enterprise data. We formulate the
problem of Fusion Resilient Enterprise Data Anonymization and propose a
prototype solution to address this problem.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 03:21:49 GMT"
},
{
"version": "v2",
"created": "Fri, 8 Feb 2008 21:58:35 GMT"
}
] | 2008-02-08T00:00:00 | [
[
"Ganta",
"Srivatsava Ranjit",
""
],
[
"Acharya",
"Raj",
""
]
] | [
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-0.087822631,
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0.1212671474,
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-0.0890540257,
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0.0293316767,
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] |
801.1716 | Oscar Iglesias | Oscar Iglesias, Xavier Batlle and Amilcar Labarta | Particle size and cooling field dependence of exchange bias in
core/shell magnetic nanoparticles | Submitted to J. Phys. D (10 pages, 10 figures) | J. Phys. D 41, 134010 (2008) | 10.1088/0022-3727/41/13/134010 | null | cond-mat.mtrl-sci | null | We present a numerical simulation study of the exchange bias (EB) effect in
nanoparticles with core/shell structure aimed to unveil the microscopic origin
of some of the experimental phenomenology associated to this effect. In
particular, we have focused our study on the particle size and field cooling
dependence of the hysteresis loop shifts. To this end, hysteresis loops after a
field cooling process have been computed by means of Monte Carlo simulations
based on a model that takes into account the peculiar properties of the core,
shell and interfacial regions of the particle and the EB and coercive fields
have been extracted from them. The results show that, as a general trend, the
EB field $h_{EB}$ decreases with increasing particle size, in agreement with
some experimental observations. However, closer inspection reveals notable
oscillations of $h_{EB}$ as a function of the particle radius which we show to
be closely related to the net magnetization established after field cooling at
the interfacial shell spins. For a particle with ferromagnetic interface
coupling, we show that the magnitude and sign of $h_{EB}$ can be varied with
the magnetic field applied during the cooling process.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 15:09:02 GMT"
}
] | 2008-06-20T00:00:00 | [
[
"Iglesias",
"Oscar",
""
],
[
"Batlle",
"Xavier",
""
],
[
"Labarta",
"Amilcar",
""
]
] | [
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] |
801.1717 | Vesko Valov | S. Nedev, J. Pelant and V. Valov | A non-separable Christensen's theorem and set tri-quotient maps | 11 pages | null | null | null | math.GN | null | For every space $X$ let $\mathcal K(X)$ be the set of all compact subsets of
$X$. Christensen \cite{c:74} proved that if $X, Y$ are separable metrizable
spaces and $F\colon\mathcal{K}(X)\to\mathcal{K}(Y)$ is a monotone map such that
any $L\in\mathcal{K}(Y)$ is covered by $F(K)$ for some $K\in\mathcal{K}(X)$,
then $Y$ is complete provided $X$ is complete. It is well known \cite{bgp} that
this result is not true for non-separable spaces. In this paper we discuss some
additional properties of $F$ which guarantee the validity of Christensen's
result for more general spaces.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 04:06:39 GMT"
},
{
"version": "v2",
"created": "Sat, 19 Jan 2008 06:44:13 GMT"
}
] | 2008-01-21T00:00:00 | [
[
"Nedev",
"S.",
""
],
[
"Pelant",
"J.",
""
],
[
"Valov",
"V.",
""
]
] | [
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] |
801.1718 | Milan Derpich | Milan S. Derpich, Jan Ostergaard and Daniel E. Quevedo | Achieving the Quadratic Gaussian Rate-Distortion Function for Source
Uncorrelated Distortions | Technical report, January 2008. Other papers available from
http://msderpich.no-ip.org | null | null | null | cs.IT math.IT | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove achievability of the recently characterized quadratic Gaussian
rate-distortion function (RDF) subject to the constraint that the distortion is
uncorrelated to the source. This result is based on shaped dithered lattice
quantization in the limit as the lattice dimension tends to infinity and holds
for all positive distortions. It turns out that this uncorrelated distortion
RDF can be realized causally. This feature, which stands in contrast to
Shannon's RDF, is illustrated by causal transform coding. Moreover, we prove
that by using feedback noise shaping the uncorrelated distortion RDF can be
achieved causally and with memoryless entropy coding. Whilst achievability
relies upon infinite dimensional quantizers, we prove that the rate loss
incurred in the finite dimensional case can be upper-bounded by the space
filling loss of the quantizer and, thus, is at most 0.254 bit/dimension.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 04:08:07 GMT"
},
{
"version": "v2",
"created": "Sun, 13 Jan 2008 04:48:14 GMT"
},
{
"version": "v3",
"created": "Thu, 24 Jul 2008 10:02:42 GMT"
}
] | 2008-07-24T00:00:00 | [
[
"Derpich",
"Milan S.",
""
],
[
"Ostergaard",
"Jan",
""
],
[
"Quevedo",
"Daniel E.",
""
]
] | [
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] |
801.1719 | Geoff Willmott | Geoff Willmott | Dynamics of a sphere with inhomogeneous slip boundary conditions in
Stokes flow | 13 Pages, 2 figures | null | 10.1103/PhysRevE.77.055302 | null | physics.flu-dyn | null | The dynamic resistance of a sphere with a general inhomogeneous slip boundary
condition is analysed in Newtonian unbounded uniform flow at low Reynolds
number. The boundary condition is treated as a perturbation to a homogeneous
sphere, assuming that the slip length magnitude b is much smaller than the
sphere radius a. To first order, the effect of inhomogeneous slip is the same
as that of a radial deformity of magnitude b. Full resistance tensors are
presented and the dynamics of a hemispherical inhomogeneous sphere, such as a
Janus particle, are explicitly calculated.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 04:10:48 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Willmott",
"Geoff",
""
]
] | [
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] |
801.172 | Brudnyi Alexander | Alexander Brudnyi | Extension of Matrices with Entries in H^{\infty} on Coverings of Riemann
Surfaces of Finite Type | 12 pages | null | null | null | math.CV math.FA | null | In the present paper continuing our previous work we prove an extension
theorem for matrices with entries in the algebra of bounded holomorphic
functions defined on an unbranched covering of a Caratheodory hyperbolic
Riemann surface of finite type.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 04:19:22 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Brudnyi",
"Alexander",
""
]
] | [
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801.1721 | Vesko Valov | V. Valov | Probability measures and Milyutin maps between metric spaces | 14 pages | null | null | null | math.GN math.FA | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We prove that the functor $\Hat{P}$ of Radon probability measures transforms
any open map between completely metrizable spaces into a soft map. This result
is applied to establish some properties of Milyutin maps between completely
metrizable spaces.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 04:48:47 GMT"
},
{
"version": "v2",
"created": "Wed, 23 Jul 2008 21:18:18 GMT"
}
] | 2008-07-24T00:00:00 | [
[
"Valov",
"V.",
""
]
] | [
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801.1722 | Seong Chan Park | Seong Chan Park and Satoshi Yamaguchi | Inflation by non-minimal coupling | 9 pages, 1 figure | JCAP0808:009,2008 | 10.1088/1475-7516/2008/08/009 | SNUTP 07-016 | hep-ph astro-ph gr-qc hep-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Inflationary scenarios based on simple non-minimal coupling and its
generalizations are studied. Generalizing the form of non-minimal coupling to
"K(phi)R" with an arbitrary function K(phi), we show that the flat potential
still is obtainable when V(phi)/K^2(phi) is asymptotically constant. Very
interestingly, if the ratio of the dimensionless self-coupling constant of the
inflaton field and the non-minimal coupling constant is small the cosmological
observables for general monomial cases are in good agreement with recent
observational data.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 05:41:38 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Jan 2008 00:46:16 GMT"
},
{
"version": "v3",
"created": "Fri, 21 Mar 2008 07:56:25 GMT"
},
{
"version": "v4",
"created": "Fri, 8 Aug 2008 01:37:04 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Park",
"Seong Chan",
""
],
[
"Yamaguchi",
"Satoshi",
""
]
] | [
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] |
801.1723 | Ozgur Cakir | Ozgur Cakir and Toshihide Takagahara | Quantum dynamics in electron-nuclei coupled spin system in quantum dots:
Bunching, revival, and quantum correlation in electron-spin measurements | 21 pages, to be published in Phys. Rev. B | Phys. Rev. B 77, 115304(2008) | 10.1103/PhysRevB.77.115304 | null | cond-mat.mes-hall | null | We investigate quantum dynamics in the electron-nuclei coupled spin system in
quantum dots and clarify the fundamental features of quantum correlation
induced via successive electron spin measurements. This quantum correlation
leads to interesting phenomena such as the bunching of outcomes in the electron
spin measurements and the revival of an arbitrary initial electron spin state.
The nuclear spin system is also affected by the quantum correlation and is in
fact squeezed via conditional measurements or postselection. This squeezing is
confirmed by calculating the increase in the purity of the nuclear spin system.
Thus the successive electron spin measurements provide a probabilistic method
to squeeze the nuclear spin system. These new features are predicted not only
for the case of a double quantum dots occupied by a pair of electrons but also
for the case of a single quantum dot occupied by a single electron or a pair of
electrons.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 06:32:46 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Cakir",
"Ozgur",
""
],
[
"Takagahara",
"Toshihide",
""
]
] | [
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] |
801.1724 | M. Khalilian | S. Alimoradi, M. Khalilian | Bilinear Mixed Effects Models For Relations Between Universities | Submitted to the Electronic Journal of Statistics
(http://www.i-journals.org/ejs/) by the Institute of Mathematical Statistics
(http://www.imstat.org) | null | null | IMS-EJS-EJS_2008_167 | stat.AP | null | this article illustrates the use of linear and bilinear random effects models
to represent statistical dependencies that often characterize dyadic data such
as international relations. In particular, we show how to estimate models for
dyadic data that simultaneously take into account: regressor variables and
third-order dependencies, such as transitivity, clustering, and balance. We
apply this new approach to the relations among ph.d. of university in Iran over
the period from 1991-2005, illustrating the presence and strength of second and
third-order statistical dependencies in these data.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 06:54:47 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Alimoradi",
"S.",
""
],
[
"Khalilian",
"M.",
""
]
] | [
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] |
801.1725 | Peter Moran | E.-M. Ilgenfritz, D. Leinweber, P. Moran, K. Koller, G. Schierholz, V.
Weinberg | Vacuum structure revealed by over-improved stout-link smearing compared
with the overlap analysis for quenched QCD | 19 pages, 18 figures | Phys.Rev.D77:074502,2008; Erratum-ibid.D77:099902,2008 | 10.1103/PhysRevD.77.074502 10.1103/PhysRevD.77.099902 | ADP-07-20/T660, HU-EP-07/62, LMU-ASC 73/07, DESY 07-219 | hep-lat | null | A detailed comparison is made between the topological structure of quenched
QCD as revealed by the recently proposed over-improved stout-link smearing in
conjunction with an improved gluonic definition of the topological density on
one hand and a similar analysis made possible by the overlap-fermionic
topological charge density both with and without variable ultraviolet cutoff
$\lambda_{cut}$. The matching is twofold, provided by fitting the
density-density two-point functions on one hand and by a point-by-point fitting
of the topological densities according to the two methods. We point out the
similar cluster structure of the topological density for moderate smearing and
$200 \mathrm{MeV} < \lambda_{cut} < 600 \mathrm{MeV}$, respectively. We
demonstrate the relation of the gluonic topological density for extensive
smearing to the location of the overlap zero modes and the lowest overlap
non-zero mode as found for the unsmeared configurations.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 06:55:49 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Ilgenfritz",
"E. -M.",
""
],
[
"Leinweber",
"D.",
""
],
[
"Moran",
"P.",
""
],
[
"Koller",
"K.",
""
],
[
"Schierholz",
"G.",
""
],
[
"Weinberg",
"V.",
""
]
] | [
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] |
801.1726 | S Habib Mazharimousavi | S. Habib Mazharimousavi and M. Halilsoy | Higher dimensional Yang-Mills black holes in third order Lovelock
gravity | 14 pages, 3 figures, to appear in Phys. Lett. B | Phys.Lett.B665:125-130,2008 | 10.1016/j.physletb.2008.06.007 | null | gr-qc | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | By employing the higher (N\TEXTsymbol{>}5) dimensional version of the Wu-Yang
Ansatz we obtain magnetically charged new black hole solutions in the
Einstein-Yang-Mills-Lovelock (EYML) theory with second ($\alpha_{2}$) and third
($\alpha_{3}$)order parameters. These parameters, where $\alpha_{2}$ is also
known as the Gauss-Bonnet parameter, modify the horizons (and the resulting
thermodynamical properties) of the black holes. It is shown also that
asymptotically ($r\to \infty $), these parameters contribute to an effective
cosmological constant -without cosmological constant- so that the solution
behaves de-Sitter (Anti de-Sitter) like.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 07:32:36 GMT"
},
{
"version": "v2",
"created": "Fri, 13 Jun 2008 08:20:09 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Mazharimousavi",
"S. Habib",
""
],
[
"Halilsoy",
"M.",
""
]
] | [
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] |
801.1727 | Shankar Prasad Das | Shankar P. Das and Gene F. Mazenko | Does Fluctuating Nonlinear Hydrodynamics Support an Ergodic-Nonergodic
Transition? | 11 pages | null | 10.1103/PhysRevE.79.021504 | null | cond-mat.soft | null | Despite its appeal, real and simulated glass forming systems do not undergo
an ergodic-nonergodic (ENE) transition. We reconsider whether the fluctuating
nonlinear hydrodynamics (FNH) model for this system, introduced by us in 1986,
supports an ENE transition. Using nonperturbative arguments, with no reference
to the hydrodynamic regime, we show that the FNH model does not support an ENE
transition. Our results support the findings in the original paper. Assertions
in the literature questioning the validity of the original work are shown to be
in error.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 07:39:56 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Das",
"Shankar P.",
""
],
[
"Mazenko",
"Gene F.",
""
]
] | [
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0.0045862561,
0.0214599576,
-0.001128474,
-0.0333270244,
-0.0866668001
] |
801.1728 | Gregory Teitel'baum B. | Lev P. Gor'kov and Gregory B. Teitel'baum | The two-component physics in cuprates in the real space and in the
momentum representation | 8 pages, 6 figures, reported at LEHTSC 2007 conference (Tsukuba),
submitted to Journal of Physics: Conference Series | null | 10.1088/1742-6596/108/1/012009 | null | cond-mat.supr-con | null | Gradual evolution of two phase coexistence between dynamical and static
regimes in cuprates is first investigated in the real space by making use of
the available neutron scattering, NMR and mSR data. Analysis of the Hall effect
and the ARPES spectra reveals the presence of two groups of charge carriers in
LSCO. The T-dependent component is due to the thermal activation of bound
electron-hole structures seen near antinodal points in the Brillouin zone, thus
introducing the two-component physics also for the momentum representation.
Interpretation of so-called "van Hove bands" undergoes drastic changes.
Importance of the findings for pseudo-gap physics is stressed. Relation to some
recent STM and STS results is discussed.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 07:52:49 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Gor'kov",
"Lev P.",
""
],
[
"Teitel'baum",
"Gregory B.",
""
]
] | [
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] |
801.1729 | Jinhui Chen | B.I. Abelev, et al (for the STAR Collaboration) | Spin alignment measurements of the $K^{*0}(892)$ and $\phi(1020)$ vector
mesons at RHIC | 7 pages, 4 figures. fig.1 updated; one more reference added, one typo
corrected, published in PRC.77.061902 | Phys.Rev.C77:061902,2008 | 10.1103/PhysRevC.77.061902 | null | nucl-ex | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We present the first spin alignment measurements for the $K^{*0}(892)$ and
$\phi(1020)$ vector mesons produced at mid-rapidity with transverse momenta up
to 5 GeV/c at $\sqrt{s_{NN}}$ = 200 GeV at RHIC. The diagonal spin density
matrix elements with respect to the reaction plane in Au+Au collisions are
$\rho_{00}$ = 0.32 $\pm$ 0.04 (stat) $\pm$ 0.09 (syst) for the $K^{*0}$
($0.8<p_T<5.0$ GeV/c) and $\rho_{00}$ = 0.34 $\pm$ 0.02 (stat) $\pm$ 0.03
(syst) for the $\phi$ ($0.4<p_T<5.0$ GeV/c), and are constant with transverse
momentum and collision centrality. The data are consistent with the unpolarized
expectation of 1/3 and thus no evidence is found for the transfer of the
orbital angular momentum of the colliding system to the vector meson spins.
Spin alignments for $K^{*0}$ and $\phi$ in Au+Au collisions were also measured
with respect to the particle's production plane. The $\phi$ result, $\rho_{00}$
= 0.41 $\pm$ 0.02 (stat) $\pm$ 0.04 (syst), is consistent with that in p+p
collisions, $\rho_{00}$ = 0.39 $\pm$ 0.03 (stat) $\pm$ 0.06 (syst), also
measured in this work. The measurements thus constrain the possible size of
polarization phenomena in the production dynamics of vector mesons.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 08:02:05 GMT"
},
{
"version": "v2",
"created": "Fri, 13 Jun 2008 14:10:52 GMT"
}
] | 2019-08-13T00:00:00 | [
[
"Abelev",
"B. I.",
""
]
] | [
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] |
801.173 | Satya N. Majumdar | David S. Dean and Satya N. Majumdar | Extreme Value Statistics of Eigenvalues of Gaussian Random Matrices | 17 pages Revtex, 5 .eps figures included | Phys. Rev. E, 77, 041108 (2008) | 10.1103/PhysRevE.77.041108 | null | cond-mat.stat-mech | null | We compute exact asymptotic results for the probability of the occurrence of
large deviations of the largest (smallest) eigenvalue of random matrices
belonging to the Gaussian orthogonal, unitary and symplectic ensembles. In
particular, we show that the probability that all the eigenvalues of an (NxN)
random matrix are positive (negative) decreases for large N as ~\exp[-\beta
\theta(0) N^2] where the Dyson index \beta characterizes the ensemble and the
exponent \theta(0)=(\ln 3)/4=0.274653... is universal. We compute the
probability that the eigenvalues lie in the interval [\zeta_1,\zeta_2] which
allows us to calculate the joint probability distribution of the minimum and
the maximum eigenvalue. As a byproduct, we also obtain exactly the average
density of states in Gaussian ensembles whose eigenvalues are restricted to lie
in the interval [\zeta_1,\zeta_2], thus generalizing the celebrated Wigner
semi-circle law to these restricted ensembles. It is found that the density of
states generically exhibits an inverse square-root singularity at the location
of the barriers. These results are confirmed by numerical simulations.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 08:24:25 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dean",
"David S.",
""
],
[
"Majumdar",
"Satya N.",
""
]
] | [
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] |
801.1731 | Laurentiu Leustean | Laurentiu Leustean | Proof mining in ${\mathbb R}$-trees and hyperbolic spaces | in G. Mints and R. de Queiroz (Eds.): Proceedings of the 13th
Workshop on Logic, Language, Information and Computation (WoLLIC 2006),
Stanford University, CA, USA, 18-21 July 2006 | Electronic Notes in Theoretical Computer Science, Vol. 165 (2006),
95-106 | null | null | math.LO math.FA | null | This paper is part of the general project of proof mining, developed by
Kohlenbach. By "proof mining" we mean the logical analysis of mathematical
proofs with the aim of extracting new numerically relevant information hidden
in the proofs.
We present logical metatheorems for classes of spaces from functional
analysis and hyperbolic geometry, like Gromov hyperbolic spaces, ${\mathbb
R}$-trees and uniformly convex hyperbolic spaces. Our theorems are adaptations
to these structures of previous metatheorems of Gerhardy and Kohlenbach, and
they guarantee a-priori, under very general logical conditions, the existence
of uniform bounds.
We give also an application in nonlinear functional analysis, more
specifically in metric fixed-point theory. Thus, we show that the uniform bound
on the rate of asymptotic regularity for the Krasnoselski-Mann iterations of
nonexpansive mappings in uniformly convex hyperbolic spaces obtained in a
previous paper is an instance of one of our metatheorems.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 08:27:14 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Leustean",
"Laurentiu",
""
]
] | [
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] |
801.1732 | Hans-Werner Hammer | Eric Braaten, H.-W. Hammer, Daekyoung Kang, Lucas Platter | Three-Body Recombination of Identical Bosons with a Large Positive
Scattering Length at Nonzero Temperature | 34 pages, 10 figures, published version | Phys.Rev.A78:043605,2008 | 10.1103/PhysRevA.78.043605 | HISKP-TH-08-01 | cond-mat.other hep-ph nucl-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | For identical bosons with a large scattering length, the dependence of the
3-body recombination rate on the collision energy is determined in the
zero-range limit by universal functions of a single scaling variable. There are
six scaling functions for angular momentum zero and one scaling function for
each higher partial wave. We calculate these universal functions by solving the
Skorniakov--Ter-Martirosian equation. The results for the 3-body recombination
as a function of the collision energy are in good agreement with previous
results from solving the 3-body Schroedinger equation for 4He atoms. The
universal scaling functions can be used to calculate the 3-body recombination
rate at nonzero temperature. We obtain an excellent fit to the data from the
Innsbruck group for 133Cs atoms with a large positive scattering length.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 08:37:46 GMT"
},
{
"version": "v2",
"created": "Fri, 14 Nov 2008 09:53:23 GMT"
}
] | 2008-12-18T00:00:00 | [
[
"Braaten",
"Eric",
""
],
[
"Hammer",
"H. -W.",
""
],
[
"Kang",
"Daekyoung",
""
],
[
"Platter",
"Lucas",
""
]
] | [
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-0.0622910373,
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0.0930054784,
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0.063260965,
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] |
801.1733 | Emmanuel Kowalski | F. Jouve, E. Kowalski, D. Zywina | An explicit integral polynomial whose splitting field has Galois group
W(E_8) | 18 pages | null | null | null | math.NT math.GR | null | Using the principle that characteristic polynomials of matrices obtained from
elements of a reductive group over a number field typically have splitting
field with Galois group isomorphic to its Weyl group, we construct an explicit
monic integral polynomial of degree 240 whose splitting field has Galois group
the Weyl group of the exceptional group of type E_8.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 08:41:12 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Jouve",
"F.",
""
],
[
"Kowalski",
"E.",
""
],
[
"Zywina",
"D.",
""
]
] | [
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] |
801.1734 | Brandon DiNunno | Brandon S. DiNunno and Richard A. Matzner | The Volume Inside a Black Hole | 17 pages, 5 figures | Gen.Rel.Grav.42:63-76,2010 | 10.1007/s10714-009-0814-x | null | gr-qc | null | The horizon (the surface) of a black hole is a null surface, defined by those
hypothetical "outgoing" light rays that just hover under the influence of the
strong gravity at the surface. Because the light rays are orthogonal to the
spatial 2-dimensional surface at one instant of time, the surface of the black
hole is the same for all observers (i.e. the same for all coordinate
definitions of "instant of time"). This value is 4*(pi)* (2Gm/c^2)^2 for
nonspinning black holes, with G= Newton's constant, c= speed of light, and m=
mass of the black hole.
The 3-dimensional spatial volume inside a black hole, in contrast, depends
explicitly on the definition of time, and can even be time dependent, or zero.
We give examples of the volume found inside a standard, nonspinning spherical
black hole, for several different standard time-coordinate definitions.
Elucidating these results for the volume provides a new pedagogical resource of
facts already known in principle to the relativity community, but rarely worked
out.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 08:44:01 GMT"
}
] | 2010-01-04T00:00:00 | [
[
"DiNunno",
"Brandon S.",
""
],
[
"Matzner",
"Richard A.",
""
]
] | [
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] |
801.1735 | Janyska Josef | Josef Jany\v{s}ka, Marco Modugno | Geometric structures of the classical general relativistic phase space | null | null | 10.1142/S021988780800303X | null | math-ph math.DG math.MP | null | This paper is concerned with basic geometric properties of the phase space of
a classical general relativistic particle, regarded as the 1st jet space of
motions, i.e. as the 1st jet space of timelike 1--dimensional submanifolds of
spacetime.
This setting allows us to skip constraints.
Our main goal is to determine the geometric conditions by which the Lorentz
metric and a connection of the phase space yield contact and Jacobi structures.
In particular, we specialise these conditions to the cases when the
connection of the phase space is generated by the metric and an additional
tensor.
Indeed, the case generated by the metric and the electromagnetic field is
included, as well.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 08:51:10 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Janyška",
"Josef",
""
],
[
"Modugno",
"Marco",
""
]
] | [
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] |
801.1736 | Walid Hachem | Abla Kammoun, Malika Kharouf, Walid Hachem, Jamal Najim | A Central Limit Theorem for the SNR at the Wiener Filter Output for
Large Dimensional Signals | null | null | null | null | cs.IT math.IT | null | Consider the quadratic form $\beta = {\bf y}^* ({\bf YY}^* + \rho {\bf
I})^{-1} {\bf y}$ where $\rho$ is a positive number, where ${\bf y}$ is a
random vector and ${\bf Y}$ is a $N \times K$ random matrix both having
independent elements with different variances, and where ${\bf y}$ and ${\bf
Y}$ are independent. Such quadratic forms represent the Signal to Noise Ratio
at the output of the linear Wiener receiver for multi dimensional signals
frequently encountered in wireless communications and in array processing.
Using well known results of Random Matrix Theory, the quadratic form $\beta$
can be approximated with a known deterministic real number $\bar\beta_K$ in the
asymptotic regime where $K\to\infty$ and $K/N \to \alpha > 0$. This paper
addresses the problem of convergence of $\beta$. More specifically, it is shown
here that $\sqrt{K}(\beta - \bar\beta_K)$ behaves for large $K$ like a Gaussian
random variable which variance is provided.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 09:18:52 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Kammoun",
"Abla",
""
],
[
"Kharouf",
"Malika",
""
],
[
"Hachem",
"Walid",
""
],
[
"Najim",
"Jamal",
""
]
] | [
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] |
801.1737 | Rico Zenklusen | Rico Zenklusen | Extensions to Network Flow Interdiction on Planar Graphs | 16 pages, 3 figures | null | null | null | cs.DM | null | Network flow interdiction analysis studies by how much the value of a maximum
flow in a network can be diminished by removing components of the network
constrained to some budget. Although this problem is strongly NP-complete on
general networks, pseudo-polynomial algorithms were found for planar networks
with a single source and a single sink and without the possibility to remove
vertices. In this work we introduce pseudo-polynomial algorithms which overcome
some of the restrictions of previous methods. We propose a planarity-preserving
transformation that allows to incorporate vertex removals and vertex capacities
in pseudo-polynomial interdiction algorithms for planar graphs. Additionally, a
pseudo-polynomial algorithm is introduced for the problem of determining the
minimal interdiction budget which is at least needed to make it impossible to
satisfy the demand of all sink nodes, on planar networks with multiple sources
and sinks satisfying that the sum of the supplies at the source nodes equals
the sum of the demands at the sink nodes. Furthermore we show that the
k-densest subgraph problem on planar graphs can be reduced to a network flow
interdiction problem on a planar graph with multiple sources and sinks and
polynomially bounded input numbers. However it is still not known if either of
these problems can be solved in polynomial time.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 09:13:23 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Zenklusen",
"Rico",
""
]
] | [
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801.1738 | Alejandro Fernandez-Martinez | Gabriela Roman-Ross (LGIT), Gabriel Cuello (ILL), Xavier Turrillas
(ICC), Alejandro Fernandez-Martinez (LGIT, ILL), Laurent Charlet (LGIT) | Arsenite sorption and co-precipitation with calcite | 9 pages | Chemical Geology 233, 3-4 (2006) 328-336 | 10.1016/j.chemgeo.2006.04.007 | null | physics.chem-ph physics.geo-ph | null | Sorption of As(III) by calcite was investigated as a function of As(III)
concentration, time and pH. The sorption isotherm, i.e. the log As(III) vs. log
[As(OH)3 degrees / Assat] plot is S-shaped and has been modelled on an extended
version of the surface precipitation model. At low concentrations, As(OH)3
degrees is adsorbed by complexation to surface Ca surface sites, as previously
described by the X-ray standing wave technique. The inflexion point of the
isotherm, where As(OH)3 degrees is limited by the amount of surface sites (ST),
yields 6 sites nm-2 in good agreement with crystallographic data. Beyond this
value, the amount of sorbed arsenic increases linearly with solution
concentration, up to the saturation of arsenic with respect to the
precipitation of CaHAsO3(s). The solid solutions formed in this concentration
range were examined by X-ray and neutron diffraction. The doped calcite lattice
parameters increase with arsenic content while c/a ratio remains constant. Our
results made on bulk calcite on the atomic displacement of As atoms along
[0001] direction extend those published by Cheng et al., (1999) on calcite
surface. This study provides a molecular-level explanation for why As(III) is
trapped by calcite in industrial treatments.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 09:19:53 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Roman-Ross",
"Gabriela",
"",
"LGIT"
],
[
"Cuello",
"Gabriel",
"",
"ILL"
],
[
"Turrillas",
"Xavier",
"",
"ICC"
],
[
"Fernandez-Martinez",
"Alejandro",
"",
"LGIT, ILL"
],
[
"Charlet",
"Laurent",
"",
"LGIT"
]
] | [
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801.1739 | Shigeru Yamagami | Shigeru Yamagami | Geometry of Quasi-Free States of CCR Algebras | 34 pages | Int.J.Math.21:875-913,2010 | 10.1142/S0129167X10006306 | null | math-ph math.MP math.OA | null | Geometric positions of square roots of quasi-free states of CCR algebras are
investigated together with an explicit formula for transition amplitudes among
them.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 09:29:29 GMT"
}
] | 2014-11-18T00:00:00 | [
[
"Yamagami",
"Shigeru",
""
]
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] |
801.174 | Sergio Caracciolo | Sergio Caracciolo, Bortolo Matteo Mognetti, Andrea Pelissetto | Third virial coefficient for 4-arm and 6-arm star polymers | 11 pages, 2 figures | Macromol. Theory Simul. 17 (2008) 67-72 | 10.1002/mats.200800001 | null | cond-mat.soft cond-mat.stat-mech | null | We discuss the computation of the third virial coefficient in polymer
systems, focusing on an additional contribution absent in the case of
monoatomic fluids. We determine the interpenetration ratio and several
quantities that involve the third virial coefficient for star polymers with 4
and 6 arms in the good-solvent regime, in the limit of a large degree of
polymerization.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 09:41:54 GMT"
},
{
"version": "v2",
"created": "Fri, 15 Feb 2008 11:46:50 GMT"
}
] | 2008-04-14T00:00:00 | [
[
"Caracciolo",
"Sergio",
""
],
[
"Mognetti",
"Bortolo Matteo",
""
],
[
"Pelissetto",
"Andrea",
""
]
] | [
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] |
801.1741 | Marcello Rosini | Marcello Rosini, Rita Magri, Peter Kratzer | Adsorption of Indium on a InAs wetting layer deposited on the GaAs(001)
surface | null | null | 10.1103/PhysRevB.77.165323 | null | cond-mat.mtrl-sci | null | In this work we perform a first-principles study of the adsorption properties
of an In adatom deposited on 1.75 monolayers (ML) InAs, forming a wetting layer
on GaAs$(001)$ with the $\alpha_2 (2\times4)$ or $\beta_2 (2\times4)$
reconstruction. The structural properties of these reconstructions have been
studied: we determine the equilibrium geometry of the surfaces and their
stability for various growth conditions. We have then carried out a detailed
study of the potential energy surface (PES) for an In adsorbate, finding the
minima and the saddle points. The main characteristics of the PES and the
bonding configurations of the In adatom on the surface are analyzed by
comparing with analogous studies reported in the literature, trying to extract
the effects due to: (i) the compressive strain to which the InAs adlayer is
subjected, (ii) the particular surface reconstruction, and (iii) the wetting
layer composition. We found that, in general, stable adsorption sites are
located at: (i) locations besides the As in-dimers, (ii) positions bridging two
As in-dimers, (iii) between two adjacent ad-dimers (only in $\beta_2$), and
(iv) locations bridging two As ad-dimers. We find also other shallower
adsorption sites which are more reconstruction specific due to the lower
symmetry of the $\alpha_2$ reconstruction compared to the $\beta_2$
reconstruction.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 09:54:35 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Rosini",
"Marcello",
""
],
[
"Magri",
"Rita",
""
],
[
"Kratzer",
"Peter",
""
]
] | [
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] |
801.1742 | Mancho Manev | Dimitar Mekerov, Mancho Manev | On 4n-dimensional Lie groups as quasi-Kaehler manifolds with Killing
Norden metric | 11 pages | Novi Sad J. Math., vol. 38, no. 2 (2008), 105--113 | null | null | math.DG | null | A 4n-parametric family of 4n-dimensional quasi-Kaehler manifolds with Killing
Norden metric is constructed on a Lie group. This family is characterized
geometrically.
| [
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] | 2014-04-15T00:00:00 | [
[
"Mekerov",
"Dimitar",
""
],
[
"Manev",
"Mancho",
""
]
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801.1743 | H. Caldas | Heron Caldas, and A. L. Mota | Temperature Effects in a Fermi Gas with Population Imbalance | 9 pages, 12 figures; minor typos corrected, references added | J.Stat.Mech.0808:P08013,2008 | 10.1088/1742-5468/2008/08/P08013 | null | cond-mat.str-el cond-mat.supr-con hep-ph nucl-th | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We investigate temperature effects in a Fermi gas with imbalanced spin
populations. From the general expression of the thermal gap equation we find,
in {\it weak coupling limit}, an analytical expression for the transition
temperature $T_c$ as a function of various possibilities of chemical potential
and mass asymmetries between the two particle species. For a range of asymmetry
between certain specific values, this equation always has two solutions for
$T_c$ which has been interpreted as a reentrant phenomena or a pairing induced
by temperature effect. We show that the lower $T_c$ is never related to a
stable solution. The same results are obtained in {\it strong coupling limit}.
The thermodynamical potential is carefully analyzed to avoid the consideration
of the unstable solutions. We also obtain the tricritical points for the
chemical potential and mass imbalanced cases, and beyond these points we
properly minimize the thermodynamic potential to find the stable and metastable
first order transition lines.
| [
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"created": "Fri, 29 Aug 2008 03:47:28 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Caldas",
"Heron",
""
],
[
"Mota",
"A. L.",
""
]
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801.1744 | L. Sunil Chandran | Manu Basavaraju, L. Sunil Chandran | Acyclic Edge Coloring of Graphs with Maximum Degree 4 | 13 pages | null | null | null | math.CO | null | An $acyclic$ edge coloring of a graph is a proper edge coloring such that
there are no bichromatic cycle s. The \emph{acyclic chromatic index} of a graph
is the minimum number k such that there is an acyclic e dge coloring using k
colors and is denoted by $a'(G)$. It was conjectured by Alon, Sudakov and Zaks
that for any simple and finite graph $G$, $a'(G)\le \Delta+2$, where $\Delta
=\Delta(G)$ denotes the maximum degree of $G$. We prove the conjecture for
connected graphs with $\Delta(G) \le 4$, with the additional restriction that
$m \le 2n-1$, where $n$ is the number of vertices and $m$ is the number of
edges in $G $. Note that for any graph $G$, $m \le 2n$, when $\Delta(G) \le 4$.
It follows that for any graph $G$ if $\Delta(G) \le 4$, then $a'(G) \le 7$.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 10:17:27 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Basavaraju",
"Manu",
""
],
[
"Chandran",
"L. Sunil",
""
]
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-0.0404778272,
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-0.0162734985,
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] |
801.1745 | Maria Vallarino | S. Meda, P. Sjogren, M. Vallarino | On the H^1-L^1 boundedness of operators | This paper will appear in Proceedings of the American Mathematical
Society | null | null | null | math.CA | null | We prove that if q is in (1,\infty), Y is a Banach space and T is a linear
operator defined on the space of finite linear combinations of (1,q)-atoms in
R^n which is uniformly bounded on (1,q)-atoms, then T admits a unique
continuous extension to a bounded linear operator from H^1(R^n) to Y. We show
that the same is true if we replace (1,q)-atoms with continuous
(1,\infty)-atoms. This is known to be false for (1,\infty)-atoms.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 10:22:26 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Meda",
"S.",
""
],
[
"Sjogren",
"P.",
""
],
[
"Vallarino",
"M.",
""
]
] | [
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-0.0621140487,
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] |
801.1746 | Armando Flavio Rodrigues | L. V. Belvedere and A. F. Rodrigues | Bosonized Quantum Hamiltonian of the Two-Dimensional Derivative-Coupling
Model | 17 pages | null | null | null | hep-th | null | Using the operator formulation we discuss the bosonization of the
two-dimensional derivative-coupling model. The fully bosonized quantum
Hamiltonian is obtained by computing the composite operators as the leading
terms in the Wilson short distance expansion for the operator products at the
same point. In addition, the quantum Hamiltonian contains topological terms
which give trivial contributions to the equations of motion. Taking into
account the quantum corrections to the bosonic equations of motion and to the
scale dimension of the Fermi field operator, the operator solution is obtained
in terms of a generalized Mandelstam soliton operator with continuous Lorentz
spin (generalized statistics).
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 10:23:10 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Belvedere",
"L. V.",
""
],
[
"Rodrigues",
"A. F.",
""
]
] | [
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] |
801.1747 | Isabel P\'erez-Arjona | Isabel Perez-Arjona, Victor J. Sanchez-Morcillo and Victor Espinosa | Bistable and dynamic states of parametrically excited ultrasound in a
fluid-filled cavity | 5 figures. Submitted to JASA | null | 10.1121/1.3119628 | null | nlin.CD | null | In this paper we have considered the problem of parametric sound generation
in an acoustic resonator flled with a fluid, taking explicitely into account
the influence of the nonlinearly generated second harmonic. A simple model is
presented, and its stationary solutions obtained. The main feature of these
solutions is the appearance of bistable states of the fundamental field
resulting from the coupling to the second harmonic. An experimental setup was
designed to check the predictions of the theory. The results are consistent
with the predicted values for the mode amplitudes and parametric thresholds. At
higher driving values a self-modulation of the amplitudes is observed. We
identify this phenomenon with a secondary instability previously reported in
the frame of the theoretical model.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 10:24:16 GMT"
},
{
"version": "v2",
"created": "Tue, 20 May 2008 15:45:19 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Perez-Arjona",
"Isabel",
""
],
[
"Sanchez-Morcillo",
"Victor J.",
""
],
[
"Espinosa",
"Victor",
""
]
] | [
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] |
801.1748 | Jonas Bj\"ornsson | Jonas Bjornsson, Stephen Hwang | On small tension p-branes | 7 pages | Phys.Lett.B662:270-274,2008 | 10.1016/j.physletb.2008.03.013 | null | hep-th | null | This paper deals with p-branes with small but non-zero tension. We prove the
existence of canonical transformations, within a perturbation theory, that link
specific geometries of p-branes to solvable theories, namely string-like and
particle-like theories. The specific shapes correspond to stretched
configurations. For configurations linked to string-like theories one will upon
quantization get a critical dimension of (25+p).
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 10:27:30 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Bjornsson",
"Jonas",
""
],
[
"Hwang",
"Stephen",
""
]
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] |
801.1749 | Julius Borcea | Julius Borcea, Alexander Guterman, Boris Shapiro | Preserving positive polynomials and beyond | 15 pages, no figures, LaTeX2e | null | null | null | math.CA math.FA | null | Following the classical approach of P\'olya-Schur theory we initiate in this
paper the study of linear operators acting on $\mathbb{R}[x]$ and preserving
either the set of positive univariate polynomials or similar sets of
non-negative and elliptic polynomials.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 14:11:52 GMT"
},
{
"version": "v2",
"created": "Tue, 22 Jan 2008 01:15:59 GMT"
}
] | 2008-01-22T00:00:00 | [
[
"Borcea",
"Julius",
""
],
[
"Guterman",
"Alexander",
""
],
[
"Shapiro",
"Boris",
""
]
] | [
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] |
801.175 | Alex Zazunov | L. Dell'Anna, A. Zazunov, and R. Egger | Superconducting non-equilibrium transport through a weakly interacting
quantum dot | 6 pages, 6 figures, replaced with published version | Phys. Rev. B 77, 104525 (2008) | 10.1103/PhysRevB.77.104525 | null | cond-mat.supr-con cond-mat.mes-hall | null | We study the out-of-equilibrium current through an interacting quantum dot
modelled as an Anderson impurity contacted by two BCS superconductors held at
fixed voltage bias. In order to account for multiple Andreev reflections, we
develop a Keldysh Green's function scheme perturbative in the dot's interaction
strength. We find an unexpected enhancement of the current due to repulsive
interactions for small lead-to-dot couplings.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 10:42:50 GMT"
},
{
"version": "v2",
"created": "Wed, 26 Mar 2008 15:04:13 GMT"
}
] | 2008-03-26T00:00:00 | [
[
"Dell'Anna",
"L.",
""
],
[
"Zazunov",
"A.",
""
],
[
"Egger",
"R.",
""
]
] | [
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801.1751 | Antonino Di Piazza | A. Di Piazza | Exact solution of the Landau-Lifshitz equation in a plane wave | 11 pages, Lett. Math. Phys. vol. 83, 305 (2008) | null | null | null | physics.optics physics.class-ph | null | The Landau-Lifshitz form of the Lorentz-Abraham-Dirac equation in the
presence of a plane wave of arbitrary shape and polarization is solved exactly
and in closed form. The explicit solution is presented in the particular,
paradigmatic cases of a constant crossed field and of a monochromatic wave with
circular and with linear polarization.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 10:49:36 GMT"
},
{
"version": "v2",
"created": "Tue, 26 Feb 2008 17:33:02 GMT"
}
] | 2008-02-26T00:00:00 | [
[
"Di Piazza",
"A.",
""
]
] | [
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801.1752 | Jaroslav Hruby | Jaroslav Hruby (Institute of Physics AV CR, Czech Republic) | Q-deformation, discrete time and quantum information as fiber space | QIP 2008. arXiv admin note: substantial text overlap (pp 5-10) with
arXiv:quant-ph/0503198 by different author | null | null | null | quant-ph | null | In this paper we show the connection between the q-deformation and discrete
time, starting from the q-deformed Heisenberg uncertainty relation and
q-deformation calculus. We show that time has discrete nature and for this case
we construct the connection between quantum information and spacetime via fiber
space structure.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 10:54:21 GMT"
}
] | 2012-07-31T00:00:00 | [
[
"Hruby",
"Jaroslav",
"",
"Institute of Physics AV CR, Czech Republic"
]
] | [
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801.1753 | Davide Emilio Galli | E. Vitali, M. Rossi, F. Tramonto, D.E. Galli, L. Reatto | Path Integral Ground State study of 2D solid 4He | 4 pages, 4 figures | null | null | null | cond-mat.other cond-mat.stat-mech | null | We have studied a two-dimensional triangular commensurate crystal of 4He with
the exact T=0 K Path Integral Ground State (PIGS) Monte Carlo method. We have
projected onto the true ground state both a Jastrow-Nosanow wave function, in
which equilibrium positions are explicitly given and no Bose-Einstein (BEC) is
present, and a translationally invariant shadow wave function, in which the
solid phase emerges through a spontaneously broken symmetry process and it has
BEC. We find a remarkable convergence to the same properties, both the diagonal
ones as well as the off-diagonal one-body density matrix rho_1. This supplies a
strong evidence that no variational bias are present in the PIGS method. We
find no BEC in the commensurate 2D 4He crystal at T=0 K, rho_1 shows an
exponential decay in the large distance range. The structure found in rho_1 is
due to virtual vacancy--interstitial pairs and this shows up in the momentum
distribution.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 10:57:49 GMT"
},
{
"version": "v2",
"created": "Thu, 17 Jan 2008 17:48:36 GMT"
},
{
"version": "v3",
"created": "Fri, 1 Feb 2008 14:56:09 GMT"
}
] | 2008-02-01T00:00:00 | [
[
"Vitali",
"E.",
""
],
[
"Rossi",
"M.",
""
],
[
"Tramonto",
"F.",
""
],
[
"Galli",
"D. E.",
""
],
[
"Reatto",
"L.",
""
]
] | [
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801.1754 | Ctirad Klimcik | Ctirad Klimcik | Affine Poisson Groups and WZW Model | This is a contribution to the Proc. of the Seventh International
Conference ''Symmetry in Nonlinear Mathematical Physics'' (June 24-30, 2007,
Kyiv, Ukraine), published in SIGMA (Symmetry, Integrability and Geometry:
Methods and Applications) at http://www.emis.de/journals/SIGMA/ | SIGMA 4:003,2008 | 10.3842/SIGMA.2008.003 | null | math-ph math.MP | null | We give a detailed description of a dynamical system which enjoys a
Poisson-Lie symmetry with two non-isomorphic dual groups. The system is
obtained by taking the $q\to\infty$ limit of the q-deformed WZW model and the
understanding of its symmetry structure results in uncovering an interesting
duality of its exchange relations.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 11:06:57 GMT"
}
] | 2008-12-19T00:00:00 | [
[
"Klimcik",
"Ctirad",
""
]
] | [
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801.1755 | Khamphee Karwan | Khamphee Karwan | The Coincidence Problem and Interacting Holographic Dark Energy | 16 pages, 5 figures; revised version to appear in JCAP; references
added | JCAP0805:011,2008 | 10.1088/1475-7516/2008/05/011 | null | astro-ph | null | We study the dynamical behaviour of the interacting holographic dark energy
model whose interaction term is $Q=3H(\lam_d\rho_d + \lam_c\rho_c)$, where
$\rho_d$ and $\rho_c$ are the energy density of dark energy and CDM
respectively. To satisfy the observational constraints from SNIa, CMB shift
parameter and BAO measurement, if $\lam_c = \lam_d$ or $\lam_d, \lam_c >0$, the
cosmic evolution will only reach the attractor in the future and the ratio
$\rho_c/\rho_d$ cannot be slowly varying at present. Since the cosmic attractor
can be reached in the future even when the present values of the cosmological
parameters do not satisfy the observational constraints, the coincidence
problem is not really alleviated in this case. However, if $\lam_c \neq \lam_d$
and they are allowed to be negative, the ratio $\rho_c/\rho_d$ can be slowly
varying at present and the cosmic attractor can be reached near the present
epoch. Hence, the alleviation of the coincidence problem is attainable in this
case. The alleviation of coincidence problem in this case is still attainable
when confronting this model to SDSS data.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 11:10:18 GMT"
},
{
"version": "v2",
"created": "Sun, 10 Feb 2008 12:40:48 GMT"
},
{
"version": "v3",
"created": "Wed, 14 May 2008 16:44:23 GMT"
}
] | 2008-11-26T00:00:00 | [
[
"Karwan",
"Khamphee",
""
]
] | [
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] |
801.1756 | Manuel J. Schmidt | Manuel J. Schmidt and Reinhold Oppermann | New technique for replica symmetry breaking with application to the
SK-model at and near T=0 | null | null | 10.1103/PhysRevE.77.061104 | null | cond-mat.dis-nn cond-mat.stat-mech | null | We describe a novel method which allows the treatment of high orders of
replica-symmetry-breaking (RSB) at low temperatures as well as at T=0 directly,
without a need for approximations or scaling assumptions. It yields the low
temperature order function q(a,T) in the full range $0\leq a <\infty$ and is
complete in the sense that all observables can be calculated from it. The
behavior of some observables and the finite RSB theory itself is analyzed as
one approaches continuous RSB. The validity and applicability of the
traditional continuous formulation is then scrutinized and a new continuous RSB
formulation is proposed.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 11:12:15 GMT"
}
] | 2013-05-29T00:00:00 | [
[
"Schmidt",
"Manuel J.",
""
],
[
"Oppermann",
"Reinhold",
""
]
] | [
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] |
801.1757 | Stanislaw Kryszewski | Stanislaw Kryszewski, Justyna Czechowska-Kryszk | Master equation - tutorial approach | 38 pages, 4 figures | null | null | null | quant-ph | null | We do not present any original or new material. This is a tutorial addressed
to students who need to study the microscopic derivation of the
quantum-mechanical master equation encountered in many practical physical
situations.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 11:26:09 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Kryszewski",
"Stanislaw",
""
],
[
"Czechowska-Kryszk",
"Justyna",
""
]
] | [
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] |
801.1758 | Piero Barone | Piero Barone | A new transform for solving the noisy complex exponentials approximation
problem | 42 pages, 5 figures | Journal of Approximation Theory, vol.155, pp. 1-27, 2008 | 10.1016/j.jat.2008.04.007 | null | math.ST math.NA stat.ME stat.TH | null | The problem of estimating a complex measure made up by a linear combination
of Dirac distributions centered on points of the complex plane from a finite
number of its complex moments affected by additive i.i.d. Gaussian noise is
considered. A random measure is defined whose expectation approximates the
unknown measure under suitable conditions. An estimator of the approximating
measure is then proposed as well as a new discrete transform of the noisy
moments that allows to compute an estimate of the unknown measure. A small
simulation study is also performed to experimentally check the goodness of the
approximations.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 11:30:34 GMT"
}
] | 2012-05-03T00:00:00 | [
[
"Barone",
"Piero",
""
]
] | [
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] |
801.1759 | Demetrios Vlachos Sotirios | D. Xenides, D. S. Vlachos, T. E. Simos | Synchronization in Complex Systems Following the Decision Based Queuing
Process: The Rhythmic Applause as a Test Case | 16 pages, 5 figures | null | 10.1088/1742-5468/2008/07/P07017 | null | cond-mat.stat-mech cond-mat.other | null | Living communities can be considered as complex systems, thus a fertile
ground for studies related to their statistics and dynamics. In this study we
revisit the case of the rhythmic applause by utilizing the model proposed by
V\'azquez et al. [A. V\'azquez et al., Phys. Rev. E 73, 036127 (2006)]
augmented with two contradicted {\it driving forces}, namely: {\it
Individuality} and {\it Companionship}. To that extend, after performing
computer simulations with a large number of oscillators we propose an
explanation on the following open questions (a) why synchronization occurs
suddenly, and b) why synchronization is observed when the clapping period
($T_c$) is $1.5 \cdot T_s < T_c < 2.0 \cdot T_s$ ($T_s$ is the mean self period
of the spectators) and is lost after a time. Moreover, based on the model, a
weak preferential attachment principle is proposed which can produce complex
networks obeying power law in the distribution of number edges per node with
exponent greater than 3.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 11:37:34 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Xenides",
"D.",
""
],
[
"Vlachos",
"D. S.",
""
],
[
"Simos",
"T. E.",
""
]
] | [
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] |
801.176 | Hiromichi Takagi | Hiromichi Takagi and Francesco Zucconi | Scorza quartics of trigonal spin curves and their varieties of power
sums | null | null | null | null | math.AG | null | Our fundamental result is the construction of new subvarieties in the
varieties of power sums for the Scorza quartic of any general pairs of trigonal
curves and non-effective theta characteristics. This is a generalization of
Mukai's description of smooth prime Fano threefolds of genus twelve as the
varieties of power sums for plane quartics. Among other applications, we give
an affirmative answer to the conjecture of Dolgachev and Kanev on the existence
of the Scorza quartic for any general pairs of curves and non-effective theta
characteristics.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 11:46:50 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Takagi",
"Hiromichi",
""
],
[
"Zucconi",
"Francesco",
""
]
] | [
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] |
801.1761 | Ramanpreet Kaur | Ramanpreet Kaur, Biswajit Paul, Brijesh Kumar, Ram Sagar | A study of the long term evolution of quasi periodic oscillations in the
accretion powered X-ray pulsar 4U 1626-67 | 14 pages, 3 figures. Accepted for publication in ApJ | null | 10.1086/529130 | null | astro-ph | null | We report here a study of the long term properties of Quasi Periodic
Oscillations (QPO) in an unusual accreting X-ray pulsar, 4U 1626--67. This is a
unique accretion powered X-ray pulsar in which we have found the QPOs to be
present during all sufficiently long X-ray observations with a wide range of
X-ray observatories. In the present spin-down era of this source, the QPO
central frequency is found to be decreasing. In the earlier spin-up era of this
source, there are only two reports of QPO detections, in 1983 with EXOSAT and
1988 with GINGA with an increasing trend. The QPO frequency evolution in 4U
1626--67 during the last 22 years changed from a positive to a negative trend,
somewhat coincident with the torque reversal in this source. In the accretion
powered X-ray pulsars, the QPO frequency is directly related to the inner
radius of the accretion disk, as per Keplerian Frequency Model (KFM) and Beat
Frequency Model (BFM). A gradual depletion of accretion disk is reported
earlier from the X-ray spectral, flux and pulse profile measurements. The
present QPO frequency evolution study shows that X-ray flux and mass accretion
rate may not change by the same factor, hence the simple KFM and BFM are not
able to explain the QPO evolution in this source. This is the only X-ray pulsar
to show persistent QPOs and is also the first accreting X-ray pulsar in which
the QPO history is reported for a long time scale relating it with the long
term evolution of the accretion disk.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 11:56:02 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Kaur",
"Ramanpreet",
""
],
[
"Paul",
"Biswajit",
""
],
[
"Kumar",
"Brijesh",
""
],
[
"Sagar",
"Ram",
""
]
] | [
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] |
801.1762 | Tzu Chiang Yuan | Kingman Cheung, Thomas W. Kephart, Wai-Yee Keung, and Tzu-Chiang Yuan | Decay of Z Boson into Photon and Unparticle | 12 pages, 2 figures plus 1 table | Phys.Lett.B662:436-440,2008 | 10.1016/j.physletb.2008.03.037 | null | hep-ph | null | We study the decay of the standard model Z boson into unparticle plus a
single photon through a one-loop process. As in the anomaly type decay, only
the axial-vector part of the Z coupling matching with the vector unparticle
and/or the vector part of the Z coupling matching with the axial-vector
unparticle can give a nonzero contribution to the decay. We show that the
photon spectrum terminates at the end point in accord with Yang's theorem.
Existing data on single photon production at LEP I is used to constrain the
unparticle sector.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 12:06:27 GMT"
}
] | 2010-10-27T00:00:00 | [
[
"Cheung",
"Kingman",
""
],
[
"Kephart",
"Thomas W.",
""
],
[
"Keung",
"Wai-Yee",
""
],
[
"Yuan",
"Tzu-Chiang",
""
]
] | [
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] |
801.1763 | Binoy Talukdar None | Amitava Choudhuri, B. Talukdar and U. Das | Modified KdV hierarchy : Lax pair representation and bi-Hamiltonian
structure | 8 pages, 2 figures | Z. Naturforsch, 64a, 171-179 (2008) | 10.1515/zna-2009-3-403 | null | nlin.SI | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | We consider equations in the modified KdV (mKdV) hierarchy and make use of
the Miura transformation to construct expressions for their Lax pair. We derive
a Lagrangian-based approach to study the bi-Hamiltonian structure of the mKdV
equations. We also show that the complex modified KdV (cmKdV) equation follows
from the action principle to have a Lagrangian representation. This
representation not only provides a basis to write the cmKdV equation in the
canonical form endowed with an appropriate Poisson structure but also help us
construct a semianalytical solution of it. The solution obtained by us may
serve as a useful guide for purely numerical routines which are currently being
used to solve the cmKdV eqution.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 12:14:25 GMT"
},
{
"version": "v2",
"created": "Fri, 9 Oct 2009 08:20:49 GMT"
}
] | 2015-05-13T00:00:00 | [
[
"Choudhuri",
"Amitava",
""
],
[
"Talukdar",
"B.",
""
],
[
"Das",
"U.",
""
]
] | [
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] |
801.1764 | Iosif Khriplovich | I.B. Khriplovich, A.A. Pomeransky | Does Cosmological Term Influence Gravitational Lensing? | 5 pages, 1 figure | Int.J.Mod.Phys.D17:2255-2259,2008 | 10.1142/S0218271808013832 | null | gr-qc astro-ph | null | We analyze the bending of light by galaxies or clusters of galaxies in the
presence of the cosmological term. Going over to the Friedmann-Robertson-Walker
coordinates, used in fact for the description of actual observations, we
demonstrate that the cosmological constant does not influence practically the
lensing effect.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 12:15:52 GMT"
}
] | 2009-02-11T00:00:00 | [
[
"Khriplovich",
"I. B.",
""
],
[
"Pomeransky",
"A. A.",
""
]
] | [
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] |
801.1765 | Matthias Troyer | A.F. Albuquerque, F. Alet, P. Corboz, P. Dayal, A. Feiguin, S. Fuchs,
L. Gamper, E. Gull, S. Guertler, A. Honecker, R. Igarashi, M. Koerner, A.
Kozhevnikov, A. Laeuchli, S.R. Manmana, M. Matsumoto, I.P. McCulloch, F.
Michel, R.M. Noack, G. Pawlowski, L. Pollet, T. Pruschke, U. Schollwock, S.
Todo, S. Trebst, M. Troyer, P. Werner, S. Wessel (for the ALPS collaboration) | The ALPS project release 1.3: open source software for strongly
correlated systems | null | Journal of Magnetism and Magnetic Materials 310, 1187 (2007) | 10.1016/j.jmmm.2006.10.304 | null | cond-mat.str-el cond-mat.stat-mech | null | We present release 1.3 of the ALPS (Algorithms and Libraries for Physics
Simulations) project, an international open source software project to develop
libraries and application programs for the simulation of strongly correlated
quantum lattice models such as quantum magnets, lattice bosons, and strongly
correlated fermion systems. Development is centered on common XML and binary
data formats, on libraries to simplify and speed up code development, and on
full-featured simulation programs. The programs enable non-experts to start
carrying out numerical simulations by providing basic implementations of the
important algorithms for quantum lattice models: classical and quantum Monte
Carlo (QMC) using non-local updates, extended ensemble simulations, exact and
full diagonalization (ED), as well as the density matrix renormalization group
(DMRG). Changes in the new release include a DMRG program for interacting
models, support for translation symmetries in the diagonalization programs, the
ability to define custom measurement operators, and support for inhomogeneous
systems, such as lattice models with traps. The software is available from our
web server at http://alps.comp-phys.org/ .
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 12:18:09 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Albuquerque",
"A. F.",
"",
"for the ALPS collaboration"
],
[
"Alet",
"F.",
"",
"for the ALPS collaboration"
],
[
"Corboz",
"P.",
"",
"for the ALPS collaboration"
],
[
"Dayal",
"P.",
"",
"for the ALPS collaboration"
],
[
"Feiguin",
"A.",
"",
"for the ALPS collaboration"
],
[
"Fuchs",
"S.",
"",
"for the ALPS collaboration"
],
[
"Gamper",
"L.",
"",
"for the ALPS collaboration"
],
[
"Gull",
"E.",
"",
"for the ALPS collaboration"
],
[
"Guertler",
"S.",
"",
"for the ALPS collaboration"
],
[
"Honecker",
"A.",
"",
"for the ALPS collaboration"
],
[
"Igarashi",
"R.",
"",
"for the ALPS collaboration"
],
[
"Koerner",
"M.",
"",
"for the ALPS collaboration"
],
[
"Kozhevnikov",
"A.",
"",
"for the ALPS collaboration"
],
[
"Laeuchli",
"A.",
"",
"for the ALPS collaboration"
],
[
"Manmana",
"S. R.",
"",
"for the ALPS collaboration"
],
[
"Matsumoto",
"M.",
"",
"for the ALPS collaboration"
],
[
"McCulloch",
"I. P.",
"",
"for the ALPS collaboration"
],
[
"Michel",
"F.",
"",
"for the ALPS collaboration"
],
[
"Noack",
"R. M.",
"",
"for the ALPS collaboration"
],
[
"Pawlowski",
"G.",
"",
"for the ALPS collaboration"
],
[
"Pollet",
"L.",
"",
"for the ALPS collaboration"
],
[
"Pruschke",
"T.",
"",
"for the ALPS collaboration"
],
[
"Schollwock",
"U.",
"",
"for the ALPS collaboration"
],
[
"Todo",
"S.",
"",
"for the ALPS collaboration"
],
[
"Trebst",
"S.",
"",
"for the ALPS collaboration"
],
[
"Troyer",
"M.",
"",
"for the ALPS collaboration"
],
[
"Werner",
"P.",
"",
"for the ALPS collaboration"
],
[
"Wessel",
"S.",
"",
"for the ALPS collaboration"
]
] | [
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] |
801.1766 | Pinyan Lu | Jin-Yi Cai, Pinyan Lu and Mingji Xia | A Family of Counter Examples to an Approach to Graph Isomorphism | null | null | null | null | cs.CC cs.DM | null | We give a family of counter examples showing that the two sequences of
polytopes $\Phi_{n,n}$ and $\Psi_{n,n}$ are different. These polytopes were
defined recently by S. Friedland in an attempt at a polynomial time algorithm
for graph isomorphism.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 12:28:05 GMT"
},
{
"version": "v2",
"created": "Sat, 12 Jan 2008 10:12:53 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Cai",
"Jin-Yi",
""
],
[
"Lu",
"Pinyan",
""
],
[
"Xia",
"Mingji",
""
]
] | [
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] |
801.1767 | Aldo Dall'Aglio | Aldo Dall'Aglio, Lutz Wisotzki, Gabor Worseck (Astrophysikalisches
Institut Potsdam) | The line-of-sight proximity effect in individual quasar spectra | A&A accepted for publication, 14 pages, 24 figures (including 17
online figures) | null | 10.1051/0004-6361:20077088 | null | astro-ph | null | We exploit a set of high signal-to-noise (~70), low-resolution (R~800) quasar
spectra to search for the signature of the so-called proximity effect in the HI
Ly alpha forest. Our sample consists of 17 bright quasars in the redshift range
2.7<z<4.1. Analysing the spectra with the flux transmission technique, we
detect the proximity effect in the sample at high significance. We use this to
estimate the average intensity of the metagalactic UV background, assuming it
to be constant over this redshift range. We obtain a value of J =
(9+-4)x10^{-22}ergcm^{-2}s^{-1}Hz^{-1}sr^{-1}, in good agreement with previous
measurements at similar z. We then apply the same procedure to individual lines
of sight, finding a significant deficit in the effective optical depth close to
the emission redshift in every single object except one (which by a different
line of evidence does nevertheless show a noticeable proximity effect). Thus,
we clearly see the proximity effect as a universal phenomenon associated with
individual quasars. Using extensive Monte-Carlo simulations to quantify the
error budget, we assess the expected statistical scatter in the strength of the
proximity effect due to shot noise (cosmic variance). The observed scatter is
larger than the predicted one, so that additional sources of scatter are
required. We rule out a dispersion of spectral slopes as a significant
contributor. Possible effects are long time-scale variability of the quasars
and/or gravitational clustering of Ly alpha forest lines. We speculate on the
possibility of using the proximity effect as a tool to constrain individual
quasar ages, finding that ages between ~10^6 and ~10^8 yrs might produce a
characteristic signature in the optical depth profile towards the QSO. We
identify one possible candidate for this effect in our sample.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 12:41:20 GMT"
},
{
"version": "v2",
"created": "Fri, 18 Jan 2008 08:38:19 GMT"
}
] | 2009-11-13T00:00:00 | [
[
"Dall'Aglio",
"Aldo",
"",
"Astrophysikalisches\n Institut Potsdam"
],
[
"Wisotzki",
"Lutz",
"",
"Astrophysikalisches\n Institut Potsdam"
],
[
"Worseck",
"Gabor",
"",
"Astrophysikalisches\n Institut Potsdam"
]
] | [
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] |
801.1768 | Luciano Lapas Calheiros | Agustin P\'erez-Madrid, Jos\'e M. Rub\'i, and Luciano C. Lapas | Heat transfer between nanoparticles: Thermal conductance for near-field
interactions | null | Phys. Rev. B 77, 155417 (2008) | 10.1103/PhysRevB.77.155417 | null | cond-mat.mtrl-sci cond-mat.mes-hall | null | We analyze the heat transfer between two nanoparticles separated by a
distance lying in the near-field domain in which energy interchange is due to
Coulomb interactions. The thermal conductance is computed by assuming that the
particles have charge distributions characterized by fluctuating multipole
moments in equilibrium with heat baths at two different temperatures. This
quantity follows from the fluctuation-dissipation theorem (FDT) for the
fluctuations of the multipolar moments. We compare the behavior of the
conductance as a function of the distance between the particles with the result
obtained by means of molecular dynamics simulations. The formalism proposed
enables us to provide a comprehensive explanation of the marked growth of the
conductance when decreasing the distance between the nanoparticles.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 12:32:23 GMT"
}
] | 2008-04-18T00:00:00 | [
[
"Pérez-Madrid",
"Agustin",
""
],
[
"Rubí",
"José M.",
""
],
[
"Lapas",
"Luciano C.",
""
]
] | [
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] |
801.1769 | Antonio Pipino | Antonio Pipino (Astrophysics, Oxford University, UK), Francesca
Matteucci (Dipartimento di Astronomia, Universita'di Trieste, Italy) and
Thomas H. Puzia (Herzberg Institute of Astrophysics, Canada) | Stars, gas and dust in elliptical galaxies | 12 pages, 4 figures, to appear on the proceedings of "XIXemes
Rencontres de Blois" | null | null | null | astro-ph | null | I will present recent theoretical results on the formation and the high
redshift assembly of spheroids. These findings have been obtained by utilising
different and complementary techniques: chemodynamical models offer great
insight in the radial abundance gradients in the stars; while state
semi-analytic codes implementing a detailed treatment of the chemical evolution
allow an exploration of the role of the galactic mass in shaping many observed
relations. The results will be shown by following the path represented by the
evolution of the mass-metallicity relation in stars, gas and dust. I will show
how, under a few sensible assumptions, it is possible to reproduce a large
number of observables ranging from the Xrays to the Infrared. By comparing
model predictions with observations, we derive a picture of galaxy formation in
which the higher is the mass of the galaxy, the shorter are the infall and the
star formation timescales. Therefore, the stellar component of the most massive
and luminous galaxies might attain a metallicity Z > Z_sun in only 0.5 Gyr.
Each galaxy is created outside-in, i.e. the outermost regions accrete gas, form
stars and develop a galactic wind very quickly, compared to the central core in
which the star formation can last up to ~ 1.3 Gyr.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 12:49:10 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Pipino",
"Antonio",
"",
"Astrophysics, Oxford University, UK"
],
[
"Matteucci",
"Francesca",
"",
"Dipartimento di Astronomia, Universita'di Trieste, Italy"
],
[
"Puzia",
"Thomas H.",
"",
"Herzberg Institute of Astrophysics, Canada"
]
] | [
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] |
801.177 | Vincent Tatischeff | V. Tatischeff and M. Hernanz | Evidence for Nonlinear Diffusive Shock Acceleration of Cosmic Rays in
the 2006 Outburst of RS Ophiuchi | 4 pages, 2 figures. To appear in "RS Ophiuchi (2006) and the
recurrent nova phenomenon", eds. A. Evans, M.F. Bode & T.J. O'Brien, ASP
Conf. Ser | null | null | null | astro-ph | null | Spectroscopic observations of the 2006 outburst of RS Oph at both infrared
(IR) and X-ray wavelengths have shown that the blast wave has decelerated at a
higher rate than predicted by the standard test-particle adiabatic shock-wave
model. The observed blast-wave evolution can be explained, however, by the
diffusive shock acceleration of particles at the forward shock and the
subsequent escape of the highest energy ions from the acceleration region.
Nonlinear particle acceleration can also account for the difference of shock
velocities deduced from the IR and X-ray data. We discuss the evolution of the
nova remnant in the light of efficient particle acceleration at the blast wave.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 12:45:52 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Tatischeff",
"V.",
""
],
[
"Hernanz",
"M.",
""
]
] | [
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801.1771 | Malgorzata Krolikowska | Malgorzata Krolikowska and Grzegorz Sitarski | Asteroid 2007 WD5 will not impact Mars on January 30! | 7 pages | null | null | null | astro-ph | null | The Monte Carlo method of the nominal orbit clonning was applied to the case
of 2007 WD5, the asteroid from the Apollo group. Calculations based on 33
observations from the time interval of 2007 11 08 - 2008 01 02 showed that the
asteroid will pass near planet Mars at the minimum distance of 10.9\pm 2.9
R_{Mars}, what implies that probability that 2007 WD5 strike the planet
decreased to the value of 0.03% from the value of about 3--4% previously
announced by NASA. The additional observations taken on January 3--9 reduce
further the asteroid's impact chances, effectively to nil: the asteroid will
pass near planet Mars at the minimum distance of 8.4\pm 1.1 R_{Mars}.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 12:46:45 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Krolikowska",
"Malgorzata",
""
],
[
"Sitarski",
"Grzegorz",
""
]
] | [
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] |
801.1772 | Veronika Rehn-Sonigo | Anne Benoit (INRIA Rh\^one-Alpes, LIP), Harald Kosch, Veronika
Rehn-Sonigo (INRIA Rh\^one-Alpes, LIP), Yves Robert (INRIA Rh\^one-Alpes,
LIP) | Bi-criteria Pipeline Mappings for Parallel Image Processing | null | null | null | null | cs.DC | null | Mapping workflow applications onto parallel platforms is a challenging
problem, even for simple application patterns such as pipeline graphs. Several
antagonistic criteria should be optimized, such as throughput and latency (or a
combination). Typical applications include digital image processing, where
images are processed in steady-state mode. In this paper, we study the mapping
of a particular image processing application, the JPEG encoding. Mapping
pipelined JPEG encoding onto parallel platforms is useful for instance for
encoding Motion JPEG images. As the bi-criteria mapping problem is NP-complete,
we concentrate on the evaluation and performance of polynomial heuristics.
| [
{
"version": "v1",
"created": "Fri, 11 Jan 2008 14:48:43 GMT"
}
] | 2008-01-14T00:00:00 | [
[
"Benoit",
"Anne",
"",
"INRIA Rhône-Alpes, LIP"
],
[
"Kosch",
"Harald",
"",
"INRIA Rhône-Alpes, LIP"
],
[
"Rehn-Sonigo",
"Veronika",
"",
"INRIA Rhône-Alpes, LIP"
],
[
"Robert",
"Yves",
"",
"INRIA Rhône-Alpes,\n LIP"
]
] | [
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] |
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