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704.0801 | Brice Camus | Brice Camus | Fundamental solutions for a class of non-elliptic homogeneous
differential operators | 15 pages, perhaps to be revised | null | null | null | math.AP math.GM | null | We compute temperate fundamental solutions of homogeneous differential
operators with real-principal type symbols. Via analytic continuation of
meromorphic distributions, fundamental solutions for these non-elliptic
operators can be constructed in terms of radial averages and invariant
distributions on the unit sphere.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 20:35:58 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Camus",
"Brice",
""
]
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704.0802 | Caleb Lo | Caleb K. Lo, Robert W. Heath, Jr. and Sriram Vishwanath | Hybrid-ARQ in Multihop Networks with Opportunistic Relay Selection | 4 pages, 5 figures, to appear in Proceedings of the 2007
International Conference on Acoustics, Speech, and Signal Processing in
Honolulu, HI | null | null | null | cs.IT math.IT | null | This paper develops a contention-based opportunistic feedback technique
towards relay selection in a dense wireless network. This technique enables the
forwarding of additional parity information from the selected relay to the
destination. For a given network, the effects of varying key parameters such as
the feedback probability are presented and discussed. A primary advantage of
the proposed technique is that relay selection can be performed in a
distributed way. Simulation results find its performance to closely match that
of centralized schemes that utilize GPS information, unlike the proposed
method. The proposed relay selection method is also found to achieve throughput
gains over a point-to-point transmission strategy.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 20:37:44 GMT"
}
] | "2012-08-27T00:00:00" | [
[
"Lo",
"Caleb K.",
""
],
[
"Heath,",
"Robert W.",
"Jr."
],
[
"Vishwanath",
"Sriram",
""
]
] | [
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704.0803 | Josephine Nanao | Walter A. Simmons and Sandip S. Pakvasa | Geometric Phase and Superconducting Flux Quantization | 5 pages, pdf format | null | null | null | quant-ph | null | In a ring of s-wave superconducting material the magnetic flux is quantized
in units of $\Phi_0 = \frac{h}{2e}$. It is well known from the theory of
Josephson junctions that if the ring is interrupted with a piece of d-wave
material, then the flux is quantized in one-half of those units due to a
additional phase shift of $\pi$. We reinterpret this phenomenon in terms of
geometric phase.
We consider an idealized hetero-junction superconductor with pure s-wave and
pure d-wave electron pairs. We find, for this idealized configuration, that the
phase shift of $\pi$ follows from the discontinuity in the geometric phase and
is thus a fundamental consequence of quantum mechanics.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 20:42:18 GMT"
}
] | "2019-08-19T00:00:00" | [
[
"Simmons",
"Walter A.",
""
],
[
"Pakvasa",
"Sandip S.",
""
]
] | [
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0.0008223138,
0.0251922198,
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0.0293868594,
-0.0195709169,
0.1510069966,
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] |
704.0804 | Francis Alexander | Francis J. Alexander, Gregory Johnson, Gregory L. Eyink, and Ioannis
G. Kevrekidis | Equation-free implementation of statistical moment closures | 7 pages, 2 figures | null | 10.1103/PhysRevE.77.026701 | null | cond-mat.stat-mech cond-mat.other | null | We present a general numerical scheme for the practical implementation of
statistical moment closures suitable for modeling complex, large-scale,
nonlinear systems. Building on recently developed equation-free methods, this
approach numerically integrates the closure dynamics, the equations of which
may not even be available in closed form. Although closure dynamics introduce
statistical assumptions of unknown validity, they can have significant
computational advantages as they typically have fewer degrees of freedom and
may be much less stiff than the original detailed model. The closure method can
in principle be applied to a wide class of nonlinear problems, including
strongly-coupled systems (either deterministic or stochastic) for which there
may be no scale separation. We demonstrate the equation-free approach for
implementing entropy-based Eyink-Levermore closures on a nonlinear stochastic
partial differential equation.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 20:45:34 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Alexander",
"Francis J.",
""
],
[
"Johnson",
"Gregory",
""
],
[
"Eyink",
"Gregory L.",
""
],
[
"Kevrekidis",
"Ioannis G.",
""
]
] | [
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] |
704.0805 | Caleb Lo | Caleb K. Lo, Robert W. Heath, Jr. and Sriram Vishwanath | Opportunistic Relay Selection with Limited Feedback | 5 pages, 6 figures, to appear in Proceedings of 2007 IEEE Vehicular
Technology Conference-Spring in Dublin, Ireland | null | 10.1109/VETECS.2007.40 | null | cs.IT math.IT | null | It has been shown that a decentralized relay selection protocol based on
opportunistic feedback from the relays yields good throughput performance in
dense wireless networks. This selection strategy supports a hybrid-ARQ
transmission approach where relays forward parity information to the
destination in the event of a decoding error. Such an approach, however,
suffers a loss compared to centralized strategies that select relays with the
best channel gain to the destination. This paper closes the performance gap by
adding another level of channel feedback to the decentralized relay selection
problem. It is demonstrated that only one additional bit of feedback is
necessary for good throughput performance. The performance impact of varying
key parameters such as the number of relays and the channel feedback threshold
is discussed. An accompanying bit error rate analysis demonstrates the
importance of relay selection.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 20:52:26 GMT"
}
] | "2016-11-17T00:00:00" | [
[
"Lo",
"Caleb K.",
""
],
[
"Heath,",
"Robert W.",
"Jr."
],
[
"Vishwanath",
"Sriram",
""
]
] | [
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] |
704.0806 | Daniel E. Vanden Berk | Donald P. Schneider, Patrick B. Hall, Gordon T. Richards, Michael A.
Strauss, Daniel E. Vanden Berk, Scott F. Anderson, W.N. Brandt, Xiaohui Fan,
Sebastian Jester, Jim Gray, James E. Gunn, Mark U. SubbaRao, Anirudda R.
Thakar, Chris Stoughton, Alexander S. Szalay, Brian Yanny, Donald G. York,
Neta A. Bahcall, J. Barentine, Michael R. Blanton, Howard Brewington, J.
Brinkmann, Robert J. Brunner, Francisco J. Castander, Istvan Csabai, Joshua
A. Frieman, Masataka Fukugita, Michael Harvanek, David W. Hogg, Zeljko
Ivezic, Stephen M. Kent, S. J. Kleinman, G. R. Knapp, Richard G. Kron, Jurek
Krzesinski, Daniel C. Long, Robert H. Lupton, Atsuko Nitta, Jeffrey R. Pier,
David H. Saxe, Yue Shen, Stephanie A. Snedden, David H. Weinberg, and Jian Wu | The Sloan Digital Sky Survey Quasar Catalog IV. Fifth Data Release | 37 pages, Accepted for publication in AJ | Astron.J.134:102-117,2007 | 10.1086/518474 | null | astro-ph | null | We present the fourth edition of the Sloan Digital Sky Survey (SDSS) Quasar
Catalog. The catalog contains 77,429 objects; this is an increase of over
30,000 entries since the previous edition. The catalog consists of the objects
in the SDSS Fifth Data Release that have luminosities larger than M_i = -22.0
(in a cosmology with H_0 = 70 km/s/Mpc, Omega_M = 0.3, and Omega_Lambda = 0.7)
have at least one emission line with FWHM larger than 1000 km/s, or have
interesting/complex absorption features, are fainter than i=15.0, and have
highly reliable redshifts. The area covered by the catalog is 5740 sq. deg. The
quasar redshifts range from 0.08 to 5.41, with a median value of 1.48; the
catalog includes 891 quasars at redshifts greater than four, of which 36 are at
redshifts greater than five. Approximately half of the catalog quasars have i <
19; nearly all have i < 21. For each object the catalog presents positions
accurate to better than 0.2 arcsec. rms per coordinate, five-band (ugriz)
CCD-based photometry with typical accuracy of 0.03 mag, and information on the
morphology and selection method. The catalog also contains basic radio,
near-infrared, and X-ray emission properties of the quasars, when available,
from other large-area surveys. The calibrated digital spectra cover the
wavelength region 3800--9200A at a spectral resolution of ~2000. The spectra
can be retrieved from the public database using the information provided in the
catalog. The average SDSS colors of quasars as a function of redshift, derived
from the catalog entries, are presented in tabular form. Approximately 96% of
the objects in the catalog were discovered by the SDSS.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 21:00:10 GMT"
}
] | "2008-11-26T00:00:00" | [
[
"Schneider",
"Donald P.",
""
],
[
"Hall",
"Patrick B.",
""
],
[
"Richards",
"Gordon T.",
""
],
[
"Strauss",
"Michael A.",
""
],
[
"Berk",
"Daniel E. Vanden",
""
],
[
"Anderson",
"Scott F.",
""
],
[
"Brandt",
"W. N.",
""
],
[
"Fan",
"Xiaohui",
""
],
[
"Jester",
"Sebastian",
""
],
[
"Gray",
"Jim",
""
],
[
"Gunn",
"James E.",
""
],
[
"SubbaRao",
"Mark U.",
""
],
[
"Thakar",
"Anirudda R.",
""
],
[
"Stoughton",
"Chris",
""
],
[
"Szalay",
"Alexander S.",
""
],
[
"Yanny",
"Brian",
""
],
[
"York",
"Donald G.",
""
],
[
"Bahcall",
"Neta A.",
""
],
[
"Barentine",
"J.",
""
],
[
"Blanton",
"Michael R.",
""
],
[
"Brewington",
"Howard",
""
],
[
"Brinkmann",
"J.",
""
],
[
"Brunner",
"Robert J.",
""
],
[
"Castander",
"Francisco J.",
""
],
[
"Csabai",
"Istvan",
""
],
[
"Frieman",
"Joshua A.",
""
],
[
"Fukugita",
"Masataka",
""
],
[
"Harvanek",
"Michael",
""
],
[
"Hogg",
"David W.",
""
],
[
"Ivezic",
"Zeljko",
""
],
[
"Kent",
"Stephen M.",
""
],
[
"Kleinman",
"S. J.",
""
],
[
"Knapp",
"G. R.",
""
],
[
"Kron",
"Richard G.",
""
],
[
"Krzesinski",
"Jurek",
""
],
[
"Long",
"Daniel C.",
""
],
[
"Lupton",
"Robert H.",
""
],
[
"Nitta",
"Atsuko",
""
],
[
"Pier",
"Jeffrey R.",
""
],
[
"Saxe",
"David H.",
""
],
[
"Shen",
"Yue",
""
],
[
"Snedden",
"Stephanie A.",
""
],
[
"Weinberg",
"David H.",
""
],
[
"Wu",
"Jian",
""
]
] | [
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704.0807 | Ruprecht Machleidt | R. Machleidt | Nuclear forces from chiral effective field theory | 54 pages, 12 figures; lectures presented at the DAE-BRNS workshop on
physics and astrophysics of hadrons and hadronic matter, Visva Bharati
University, Santiniketan, West Begal, India, November 2006 | null | null | null | nucl-th nucl-ex | null | In this lecture series, I present the recent progress in our understanding of
nuclear forces in terms of chiral effective field theory.
| [
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704.0808 | Michael T. Lacey | Michael Lacey and Xiaochun Li | On a Conjecture of EM Stein on the Hilbert Transform on Vector Fields | 92 pages, 20+ figures. Final version of the paper. To appear in
Memoirs AMS | Mem. Amer. Math. Soc., vol. 205 (2010) No. 965 | 10.1090/S0065-9266-10-00572-7 | null | math.CA | null | Let $ v$ be a smooth vector field on the plane, that is a map from the plane
to the unit circle. We study sufficient conditions for the boundedness of the
Hilbert transform
\operatorname H_{v, \epsilon}f(x) := \text{p.v.}\int_{-\epsilon}^ \epsilon
f(x-yv(x)) \frac{dy}y where $ \epsilon $ is a suitably chosen parameter,
determined by the smoothness properties of the vector field. It is a
conjecture, due to E.\thinspace M.\thinspace Stein, that if $ v$ is Lipschitz,
there is a positive $ \epsilon $ for which the transform above is bounded on $
L ^{2}$. Our principal result gives a sufficient condition in terms of the
boundedness of a maximal function associated to $ v$. This sufficient condition
is that this new maximal function be bounded on some $ L ^{p}$, for some $
1<p<2$. We show that the maximal function is bounded from $ L ^{2}$ to weak $ L
^{2}$ for all Lipschitz maximal function. The relationship between our results
and other known sufficient conditions is explored.
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704.0809 | Andy Lawrence | A.Lawrence | Wide Field Surveys and Astronomical Discovery Space | Review for publication in Astronomy and Geophysics, based on talk at
UK National Astronomy Meeting, 2006. Fifteen pages, nine figures (figs 4,5,6
have parts a and b) | null | 10.1111/j.1468-4004.2007.48327.x | null | astro-ph | null | I review the status of science with wide field surveys. For many decades
surveys have been the backbone of astronomy, and the main engine of discovery,
as we have mapped the sky at every possible wavelength. Surveys are an
efficient use of resources. They are important as a fundamental resource; to
map intrinsically large structures; to gain the necessary statistics to address
some problems; and to find very rare objects. I summarise major recent wide
field surveys - 2MASS, SDSS, 2dfGRS, and UKIDSS - and look at examples of the
exciting science they have produced, covering the structure of the Milky Way,
the measurement of cosmological parameters, the creation of a new field
studying substellar objects, and the ionisation history of the Universe. I then
look briefly at upcoming projects in the optical-IR survey arena - VISTA,
PanSTARRS, WISE, and LSST. Finally I ask, now we have opened up essentially all
wavelength windows, whether the exploration of survey discovery space is ended.
I examine other possible axes of discovery space, and find them mostly to be
too expensive to explore or otherwise unfruitful, with two exceptions : the
first is the time axis, which we have only just begun to explore properly; and
the second is the possibility of neutrino astrophysics.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 21:45:43 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Lawrence",
"A.",
""
]
] | [
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] |
704.081 | Carlos Alexandre Wuensche | Rodrigo Leonardi, Brian Williams, Marco Bersanelli, Ivan Ferreira,
Philip M. Lubin, Peter R. Meinhold, Hugh O'Neill, Nathan C. Stebor, Fabrizio
Villa, Thyrso Villela, Carlos A. Wuensche | The Cosmic Foreground Explorer (COFE): A balloon-borne microwave
polarimeter to characterize polarized foregrounds | 15 pages Version 2 - missing pictures now appear at the end of the
text | New Astron.Rev.50:977-983,2006 | 10.1016/j.newar.2006.09.004 | null | astro-ph | null | The COsmic Foreground Explorer (COFE) is a balloon-borne microwave polarime-
ter designed to measure the low-frequency and low-l characteristics of dominant
diffuse polarized foregrounds. Short duration balloon flights from the Northern
and Southern Hemispheres will allow the telescope to cover up to 80% of the sky
with an expected sensitivity per pixel better than 100 $\mu K / deg^2$ from 10
GHz to 20 GHz. This is an important effort toward characterizing the polarized
foregrounds for future CMB experiments, in particular the ones that aim to
detect primordial gravity wave signatures in the CMB polarization angular power
spectrum.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 22:00:09 GMT"
},
{
"version": "v2",
"created": "Mon, 9 Apr 2007 19:56:07 GMT"
}
] | "2009-06-23T00:00:00" | [
[
"Leonardi",
"Rodrigo",
""
],
[
"Williams",
"Brian",
""
],
[
"Bersanelli",
"Marco",
""
],
[
"Ferreira",
"Ivan",
""
],
[
"Lubin",
"Philip M.",
""
],
[
"Meinhold",
"Peter R.",
""
],
[
"O'Neill",
"Hugh",
""
],
[
"Stebor",
"Nathan C.",
""
],
[
"Villa",
"Fabrizio",
""
],
[
"Villela",
"Thyrso",
""
],
[
"Wuensche",
"Carlos A.",
""
]
] | [
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] |
704.0811 | Paula Benaglia | Gustavo E. Romero | Jet interactions in massive X-ray binaries | 5 pages, 5 figures. Invited talk presented at the meeting: "Massive
Stars: fundamental parameters and circumstellar interactions", Carilo, Dec
2006 | null | null | null | astro-ph | null | Massive X-ray binaries are formed by a compact object that accretes matter
from the stellar wind of an early-type donor star. In some of these systems,
called microquasars, relativistic jets are launched from the surroundings of
the compact object. Such jets interact with the photon field of the companion
star, the stellar wind, and, at large distances, with the interstellar medium.
In this paper I will review the main results of such interactions with
particular emphasis on the production of high-energy photons and neutrinos. The
case of some specific systems, like LS I +61 303, will be discussed in some
detail. Prospects for future observations at different wavelengths of this type
of objects will be presented.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 22:11:03 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Romero",
"Gustavo E.",
""
]
] | [
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] |
704.0812 | Rodrigo D\'iaz Mr. | Rodrigo F. D\'iaz, Carolina Cincunegui and Pablo J. D. Mauas
(Instituto de Astronom\'ia y F\'isica del Espacio (IAFE). Buenos Aires,
Argentina) | The Na I D resonance lines in main sequence late-type stars | 12 pages, including 14 figures and 4 tables. Accepted for publication
in MNRAS | Mon.Not.Roy.Astron.Soc.378:1007-1018,2007 | 10.1111/j.1365-2966.2007.11833.x | null | astro-ph | null | We study the sodium D lines (D1: 5895.92 \AA; D2: 5889.95 \AA) in late-type
dwarf stars. The stars have spectral types between F6 and M5.5 (B-V between
0.457 and 1.807) and metallicity between [Fe/H] = -0.82 and 0.6. We obtained
medium resolution echelle spectra using the 2.15-m telescope at the argentinian
observatory CASLEO. The observations have been performed periodically since
1999. The spectra were calibrated in wavelength and in flux. A definition of
the pseudo-continuum level is found for all our observations. We also define a
continuum level for calibration purposes. The equivalent width of the D lines
is computed in detail for all our spectra and related to the colour index (B-V)
of the stars. When possible, we perform a careful comparison with previous
studies. Finally, we construct a spectral index (R_D') as the ratio between the
flux in the D lines, and the bolometric flux. We find that, once corrected for
the photospheric contribution, this index can be used as a chromospheric
activity indicator in stars with a high level of activity. Additionally, we
find that combining some of our results, we obtain a method to calibrate in
flux stars of unknown colour.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 22:49:11 GMT"
}
] | "2009-06-23T00:00:00" | [
[
"Díaz",
"Rodrigo F.",
"",
"Instituto de Astronomía y Física del Espacio"
],
[
"Cincunegui",
"Carolina",
"",
"Instituto de Astronomía y Física del Espacio"
],
[
"Mauas",
"Pablo J. D.",
"",
"Instituto de Astronomía y Física del Espacio"
]
] | [
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704.0813 | Benjamin Schlein | Benjamin Schlein | Dynamics of Bose-Einstein Condensates | 20 pages, 2 figures; contribution to the Proceedings of the
International Congress on Mathematical Physics held at IMPA in Rio de Janeiro
in August 2006 | null | null | null | math-ph math.MP | null | We report on some recent results concerning the dynamics of Bose-Einstein
condensates, obtained in a series of joint papers with L. Erdos and H.-T. Yau.
Starting from many body quantum dynamics, we present a rigorous derivation of a
cubic nonlinear Schroedinger equation known as the Gross-Pitaevskii equation
for the time evolution of the condensate wave function.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 22:59:56 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Schlein",
"Benjamin",
""
]
] | [
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] |
704.0814 | Alexander I. Lvovsky | K.-P. Marzlin, Juergen Appel, A. I. Lvovsky | Photons as quasi-charged particles | null | Phys. Rev. A 77, 043813 (2008) | 10.1103/PhysRevA.77.043813 | null | quant-ph | null | The Schrodinger motion of a charged quantum particle in an electromagnetic
potential can be simulated by the paraxial dynamics of photons propagating
through a spatially inhomogeneous medium. The inhomogeneity induces geometric
effects that generate an artificial vector potential to which signal photons
are coupled. This phenomenon can be implemented with slow light propagating
through an a gas of double-Lambda atoms in an electromagnetically-induced
transparency setting with spatially varied control fields. It can lead to a
reduced dispersion of signal photons and a topological phase shift of
Aharonov-Bohm type.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 23:07:42 GMT"
},
{
"version": "v2",
"created": "Tue, 16 Oct 2007 16:24:34 GMT"
}
] | "2009-12-29T00:00:00" | [
[
"Marzlin",
"K. -P.",
""
],
[
"Appel",
"Juergen",
""
],
[
"Lvovsky",
"A. I.",
""
]
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] |
704.0815 | Sergio Duarte | D. Portes Jr., H. Rodrigues, S. B. Duarte and B. Baseia | Exchange of quantum states between coupled oscillators | 10 pages, no figure, Latex file | null | null | null | quant-ph | null | Exchange of quantum states between two interacting harmonic oscillator along
their evolution time is discussed. It is analyzed the conditions for such
exchange starting from a generic initial state and demonstrating that the
effect occurs exactly only for the particular states C0|0>+Cn|N>, which
includes the interesting qubits components |0>,|1>. It is also determined the
relation between the coupling constant and characteristic frequencies of the
oscillators to have the complete exchange.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 23:52:16 GMT"
},
{
"version": "v2",
"created": "Sat, 7 Apr 2007 22:14:46 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Portes",
"D.",
"Jr."
],
[
"Rodrigues",
"H.",
""
],
[
"Duarte",
"S. B.",
""
],
[
"Baseia",
"B.",
""
]
] | [
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] |
704.0816 | Brian Punsly | Brian Punsly | 3-D Simulations of Ergospheric Disk Driven Poynting Jets | To appear in ApJ Letters. A version with high res images is at
http://85.20.11.14/hosting/punsly/APJLetter4.2.07/ | null | 10.1086/518601 | null | astro-ph | null | This Letter reports on 3-dimensional simulations of Kerr black hole
magnetospheres that obey the general relativistic equations of perfect
magnetohydrodynamics (MHD). In particular, we study powerful Poynting flux
dominated jets that are driven from dense gas in the equatorial plane in the
ergosphere. The physics of which has been previously studied in the simplified
limit of an ergopsheric disk. For high spin black holes, $a/M > 0.95$, the
ergospheric disk is prominent in the 3-D simulations and is responsible for
greatly enhanced Poynting flux emission. Any large scale poloidal magnetic flux
that is trapped in the equatorial region leads to an enormous release of
electromagnetic energy that dwarfs the jet energy produced by magnetic flux
threading the event horizon. The implication is that magnetic flux threading
the equatorial plane of the ergosphere is a likely prerequisite for the central
engine of powerful FRII quasars.
| [
{
"version": "v1",
"created": "Thu, 5 Apr 2007 23:57:44 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Punsly",
"Brian",
""
]
] | [
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] |
704.0817 | Alexander Yong | Hugh Thomas, Alexander Yong | An S_3-symmetric Littlewood-Richardson rule | 9 pages | Math. Res. Lett. 15 (2008), no. 5, 1027--1037 | null | null | math.CO math.RT | null | The classical Littlewood-Richardson coefficients C(lambda,mu,nu) carry a
natural $S_3$ symmetry via permutation of the indices. Our "carton rule" for
computing these numbers transparently and uniformly explains these six
symmetries; previously formulated Littlewood-Richardson rules manifest at most
three of the six.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 00:25:00 GMT"
}
] | "2010-02-18T00:00:00" | [
[
"Thomas",
"Hugh",
""
],
[
"Yong",
"Alexander",
""
]
] | [
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] |
704.0818 | Michael Shay | M. A. Shay, J. F. Drake, and M. Swisdak | Two-scale structure of the electron dissipation region during
collisionless magnetic reconnection | Submitted to Physical Review Letters, 4 pages, 4 figures | null | 10.1103/PhysRevLett.99.155002 | null | physics.plasm-ph physics.space-ph | null | Particle in cell (PIC) simulations of collisionless magnetic reconnection are
presented that demonstrate that the electron dissipation region develops a
distinct two-scale structure along the outflow direction. The length of the
electron current layer is found to decrease with decreasing electron mass,
approaching the ion inertial length for a proton-electron plasma. A surprise,
however, is that the electrons form a high-velocity outflow jet that remains
decoupled from the magnetic field and extends large distances downstream from
the x-line. The rate of reconnection remains fast in very large systems,
independent of boundary conditions and the mass of electrons.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 00:11:21 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Shay",
"M. A.",
""
],
[
"Drake",
"J. F.",
""
],
[
"Swisdak",
"M.",
""
]
] | [
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] |
704.0819 | Lucero Uscanga | Lucero Uscanga, Jorge Cant\'o and Alejandro C. Raga | Position-Velocity Diagrams for the Maser Emission coming from a
Keplerian Ring | 13 pages, 7 figures, to appear in the 2007 July 20 issue of The
Astrophysical Journal | Astrophys.J.663:857-865,2007 | 10.1086/518640 | null | astro-ph | null | We have studied the maser emission from a thin, planar, gaseous ring in
Keplerian rotation around a central mass observed edge-on. The absorption
coefficient within the ring is assumed to follow a power law dependence with
the distance from the central mass as, k=k0r^{-q}. We have calculated
position-velocity diagrams for the most intense maser features, for different
values of the exponent q. We have found that, depending on the value of q,
these diagrams can be qualitatively different. The most intense maser emission
at a given velocity can either come mainly from regions close to the inner or
outer edges of the amplifying ring or from the line perpendicular to the line
of sight and passing through the central mass (as is commonly assumed).
Particularly, when q>1 the position-velocity diagram is qualitatively similar
to the one observed for the water maser emission in the nucleus of the galaxy
NGC 4258. In the context of this simple model, we conclude that in this object
the absorption coefficient depends on the radius of the amplifying ring as a
decreasing function, in order to have significant emission coming from the
inner edge of the ring.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 00:15:24 GMT"
}
] | "2009-06-23T00:00:00" | [
[
"Uscanga",
"Lucero",
""
],
[
"Cantó",
"Jorge",
""
],
[
"Raga",
"Alejandro C.",
""
]
] | [
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] |
704.082 | Svetlana Boriskina | Svetlana V. Boriskina | Coupling of whispering-gallery modes in size-mismatched microdisk
photonic molecules | 3 pages with 5 figures (to appear in Opt. Lett. 2007) | Opt. Lett. 32(11) 1557-1559 (2007) | 10.1364/OL.32.001557 | null | physics.optics | null | Mechanisms of whispering-gallery (WG) modes coupling in microdisk photonic
molecules (PMs) with slight and significant size mismatch are numerically
investigated. The results reveal two different scenarios of modes interaction
depending on the degree of this mismatch and offer new insight into how PM
parameters can be tuned to control and modify WG-modes wavelengths and
Q-factors. From a practical point of view, these findings offer a way to
fabricate PM microlaser structures that exhibit low thresholds and directional
emission, and at the same time are more tolerant to fabrication errors than
previously explored coupled-cavity structures composed of identical
microresonators.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 00:23:59 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Boriskina",
"Svetlana V.",
""
]
] | [
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] |
704.0821 | Karol Gregor | Karol Gregor, Olexei I. Motrunich | Spin solid phases of spin 1 and spin 3/2 antiferromagnets on a cubic
lattice | 15 pages, 8 figures | null | 10.1103/PhysRevB.76.174404 | null | cond-mat.str-el | null | We study spin S=1 and S=3/2 Heisenberg antiferromagnets on a cubic lattice
focusing on spin solid states. Using Schwinger boson formulation for spins, we
start in a U(1) spin liquid phase proximate to Neel phase and explore possible
confining paramagnetic phases as we transition away from the spin liquid by the
process of monopole condensation. Electromagnetic duality is used to rewrite
the theory in terms of monopoles. For spin 1 we find several candidate phases
of which the most natural one is a phase with spins organized into parallel
Haldane chains. For spin 3/2 we find that the most natural phase has spins
organized into parallel ladders. As a by-product, we also write a Landau theory
of the ordering in two special classical frustrated XY models on the cubic
lattice, one of which is the fully frustrated XY model. In a particular limit
our approach maps to a dimer model with 2S dimers coming out of every site, and
we find the same spin solid phases in this regime as well.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 00:25:56 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Gregor",
"Karol",
""
],
[
"Motrunich",
"Olexei I.",
""
]
] | [
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] |
704.0822 | Yuya Sasai | Yuya Sasai, Naoki Sasakura | Braided quantum field theories and their symmetries | 36 pages, 18 figures, a comment added and typos corrected | Prog.Theor.Phys.118:785-814,2007 | 10.1143/PTP.118.785 | YITP-07-14 | hep-th | null | Braided quantum field theories proposed by Oeckl can provide a framework for
defining quantum field theories having Hopf algebra symmetries. In quantum
field theories, symmetries lead to non-perturbative relations among correlation
functions. We discuss Hopf algebra symmetries and such relations in braided
quantum field theories. We give the four algebraic conditions between Hopf
algebra symmetries and braided quantum field theories, which are required for
the relations to hold. As concrete examples, we apply our discussions to the
Poincare symmetries of two examples of noncommutative field theories. One is
the effective quantum field theory of three-dimensional quantum gravity coupled
with spinless particles given by Freidel and Livine, and the other is
noncommutative field theory on Moyal plane. We also comment on quantum field
theory on kappa-Minkowski spacetime.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 00:28:12 GMT"
},
{
"version": "v2",
"created": "Tue, 1 May 2007 06:00:46 GMT"
},
{
"version": "v3",
"created": "Fri, 11 May 2007 05:00:57 GMT"
},
{
"version": "v4",
"created": "Wed, 23 May 2007 07:51:41 GMT"
},
{
"version": "v5",
"created": "Mon, 23 Jul 2007 04:46:19 GMT"
},
{
"version": "v6",
"created": "Mon, 27 Aug 2007 05:46:56 GMT"
}
] | "2008-11-26T00:00:00" | [
[
"Sasai",
"Yuya",
""
],
[
"Sasakura",
"Naoki",
""
]
] | [
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] |
704.0823 | Hugh Hudson | Hugh S. Hudson | Chromospheric Flares | Coimbra Solar Physics Meeting on The Physics of Chromospheric Plasmas
- Petr Heinzl, Ivan Dorotovic and Robert J. Rutten, eds | null | null | null | astro-ph | null | In this topical review I revisit the "chromospheric flare." This should
currently be an outdated concept, because modern data seem to rule out the
possiblity of a major flare happening independently in the chromosphere alone,
but the chromosphere still plays a major observational role in many ways. It is
the source of the bulk of a flare's radiant energy - in particular the
visible/UV continuum radiation. It also provides tracers that guide us to the
coronal source of the energy, even though we do not yet understand the
propagation of the energy from its storage in the corona to its release in the
chromosphere. The formation of chromospheric radiations during a flare presents
several difficult and interesting physical problems.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 01:22:41 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Hudson",
"Hugh S.",
""
]
] | [
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] |
704.0824 | Eddy Pariguan | Mauricio Angel, Jaime Camacaro and Rafael Diaz | On the (3,N) Maurer-Cartan equation | 21 pages | J. Nonlinear Math. Phys 14 (4) (2007) 440-461 | 10.1080/jnmp.2007.14.4.4 | null | math.QA | null | Deformations of the 3-differential of 3-differential graded algebras are
controlled by the (3,N) Maurer-Cartan equation. We find explicit formulae for
the coefficients appearing in that equation, introduce new geometric examples
of N-differential graded algebras, and use these results to study N Lie
algebroids.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 01:04:43 GMT"
},
{
"version": "v2",
"created": "Fri, 19 Oct 2007 22:59:40 GMT"
},
{
"version": "v3",
"created": "Fri, 4 Jan 2008 18:19:31 GMT"
}
] | "2015-05-13T00:00:00" | [
[
"Angel",
"Mauricio",
""
],
[
"Camacaro",
"Jaime",
""
],
[
"Diaz",
"Rafael",
""
]
] | [
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] |
704.0825 | Shiping Feng | Yu Lan, Jihong Qin and Shiping Feng | Electronic structure of kinetic energy driven superconductors in the
presence of bilayer splitting | 11 pages, 4 figures, replotted figures and added references, accepted
for publication in Phys. Rev. B | Phys. Rev. B 76, 014533 (2007) | 10.1103/PhysRevB.76.014533 | null | cond-mat.supr-con cond-mat.str-el | null | Within the framework of the kinetic energy driven superconductivity, the
electronic structure of bilayer cuprate superconductors in the superconducting
state is studied. It is shown that the electron spectrum of bilayer cuprate
superconductors is split into the bonding and antibonding components by the
bilayer splitting, then the observed peak-dip-hump structure around the
$[\pi,0]$ point is mainly caused by this bilayer splitting, with the
superconducting peak being related to the antibonding component, and the hump
being formed by the bonding component. The spectral weight increases with
increasing the doping concentration. In analogy to the normal state case, both
electron antibonding peak and bonding hump have the weak dispersions around the
$[\pi,0]$ point.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 01:08:40 GMT"
},
{
"version": "v2",
"created": "Tue, 24 Jul 2007 08:10:00 GMT"
}
] | "2007-08-02T00:00:00" | [
[
"Lan",
"Yu",
""
],
[
"Qin",
"Jihong",
""
],
[
"Feng",
"Shiping",
""
]
] | [
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] |
704.0826 | Varsha P. Kulkarni | Varsha P. Kulkarni, Donald G. York, Giovanni Vladilo, Daniel E. Welty | 9.7 micrometer Silicate Absorption in a Damped Lyman-alpha Absorber at
z=0.52 | 4 pages, 2 figures, submitted to Astrophysical Journal Letters
(revised version including referee's comments) | Astrophys.J.663:L81-L84,2007 | 10.1086/520048 | null | astro-ph | null | We report a detection of the 9.7 micrometer silicate absorption feature in a
damped Lyman-alpha (DLA) system at z_{abs} = 0.524 toward AO0235+164, using the
Infrared Spectrograph (IRS) onboard the Spitzer Space Telescope. The feature
shows a broad shallow profile over about 8-12 micrometers in the absorber rest
frame and appears to be > 15 sigma significant in equivalent width. The feature
is fit reasonably well by the silicate absorption profiles for laboratory
amorphous olivine or diffuse Galactic interstellar clouds. To our knowledge,
this is the first indication of 9.7 micrometer silicate absorption in a DLA. We
discuss potential implications of this finding for the nature of the dust in
quasar absorbers. Although the feature is relatively shallow (tau_{9.7} =
0.08-0.09), it is about 2 times deeper than expected from extrapolation of the
tau_{9.7} vs. E(B-V) relation known for diffuse Galactic interstellar clouds.
Further studies of the 9.7 micrometer silicate feature in quasar absorbers will
open a new window on the dust in distant galaxies.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 01:25:25 GMT"
},
{
"version": "v2",
"created": "Wed, 2 May 2007 20:16:34 GMT"
}
] | "2009-06-23T00:00:00" | [
[
"Kulkarni",
"Varsha P.",
""
],
[
"York",
"Donald G.",
""
],
[
"Vladilo",
"Giovanni",
""
],
[
"Welty",
"Daniel E.",
""
]
] | [
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] |
704.0827 | Eric Sandquist | Nassissie Fekadu, Eric L. Sandquist, Michael Bolte | Photometry of the Globular Cluster NGC 5466: Red Giants and Blue
Stragglers | 51 pages, 21 figures, 1 electronic table, accepted to ApJ | Astrophys.J.663:277-295,2007 | 10.1086/518637 | null | astro-ph | null | We present wide-field BVI photometry for about 11,500 stars in the
low-metallicity cluster NGC 5466. We have detected the red giant branch bump
for the first time, although it is at least 0.2 mag fainter than expected
relative to the turnoff. The number of red giants (relative to main sequence
turnoff stars) is in excellent agreement with stellar models from the
Yonsei-Yale and Teramo groups, and slightly high compared to Victoria-Regina
models. This adds to evidence that an abnormally large ratio of red giant to
main-sequence stars is not correlated with cluster metallicity. We discuss
theoretical predictions from different research groups and find that the
inclusion or exclusion of helium diffusion and strong limit Coulomb
interactions may be partly responsible.
We also examine indicators of dynamical history: the mass function exponent
and the blue straggler frequency. NGC 5466 has a very shallow mass function,
consistent with large mass loss and recently-discovered tidal tails. The blue
straggler sample is significantly more centrally concentrated than the HB or
RGB stars. We see no evidence of an upturn in the blue straggler frequency at
large distances from the center. Dynamical friction timescales indicate that
the stragglers should be more concentrated if the cluster's present density
structure has existed for most of its history. NGC 5466 also has an unusually
low central density compared to clusters of similar luminosity. In spite of
this, the specific frequency of blue stragglers that puts it right on the
frequency -- cluster M_V relation observed for other clusters.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 01:27:03 GMT"
}
] | "2009-06-23T00:00:00" | [
[
"Fekadu",
"Nassissie",
""
],
[
"Sandquist",
"Eric L.",
""
],
[
"Bolte",
"Michael",
""
]
] | [
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] |
704.0828 | Cynthia J. Olson Reichhardt | C. Reichhardt and C. J. Olson Reichhardt | Vortex Molecular Crystal and Vortex Plastic Crystal States in Honeycomb
and Kagome Pinning Arrays | 19 pages, 22 postscript figures. Version to appear in Phys. Rev. B | Phys. Rev. B 76, 064523 (2007) | 10.1103/PhysRevB.76.064523 | null | cond-mat.supr-con cond-mat.soft | null | Using numerical simulations, we investigate vortex configurations and pinning
in superconductors with honeycomb and kagome pinning arrays. We find that a
variety of novel vortex crystal states can be stabilized at integer and
fractional matching field densities. The honeycomb and kagome pinning arrays
produce considerably more pronounced commensuration peaks in the critical
depinning force than triangular pinning arrays, and also cause additional peaks
at noninteger matching fields where a portion of the vortices are located in
the large interstitial regions of the pinning lattices. For the honeycomb
pinning array, we find matching effects of equal strength at most fillings
B/B_\phi=n/2 for n>2, where n is an integer, in agreement with recent
experiments. For kagome pinning arrays, pronounced matching effects generally
occur at B/B_\phi=n/3 for n>3, while for triangular pinning arrays pronounced
matching effects are observed only at integer fillings B/B_\phi=n. At the
noninteger matching field peaks in the honeycomb and kagome pinning arrays, the
interstitial vortices are arranged in dimer, trimer, and higher order n-mer
states that have an overall orientational order. We call these n-mer states
"vortex molecular crystals" and "vortex plastic crystals" since they are
similar to the states recently observed in colloidal molecular crystal systems.
We argue that the vortex molecular crystals have properties in common with
certain spin systems such as Ising and n-state Potts models. We show that
kagome and honeycomb pinning arrays can be useful for increasing the critical
current above that of purely triangular pinning arrays.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 02:03:01 GMT"
},
{
"version": "v2",
"created": "Thu, 26 Jul 2007 20:21:35 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Reichhardt",
"C.",
""
],
[
"Reichhardt",
"C. J. Olson",
""
]
] | [
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] |
704.0829 | Bang-Rong Zhou | Bang-Rong Zhou (Graduate School of Chinese Academy of Sciences) | Quark-Antiquark and Diquark Condensates in Vacuum in a 3D Two-Flavor
Gross-Neveu Model | 5 pages, revtex4, no figure, minor typos corrected | Commun.Theor. Phys. 47 (2007) 695 | 10.1088/0253-6102/47/4/027 | null | hep-th | null | The effective potential analysis indicates that, in a 3D two-flavor
Gross-Neveu model in vacuum, depending on less or bigger than the critical
value 2/3 of $G_S/H_P$, where $G_S$ and $H_P$ are respectively the coupling
constants of scalar quark-antiquark channel and pseudoscalar diquark channel,
the system will have the ground state with pure diquark condensates or with
pure quark-antiquark condensates, but no the one with coexistence of the two
forms of condensates. The similarities and differences in the interplay between
the quark-antiquark and the diquark condensates in vacuum in the 2D, 3D and 4D
two-flavor four-fermion interaction models are summarized.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 02:22:22 GMT"
},
{
"version": "v2",
"created": "Sat, 23 Jun 2007 16:34:04 GMT"
}
] | "2015-05-13T00:00:00" | [
[
"Zhou",
"Bang-Rong",
"",
"Graduate School of Chinese Academy of Sciences"
]
] | [
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] |
704.083 | Qin Liu | Qin Liu, Tianxing Ma, Shou-Cheng Zhang | Spin accumulation from the non-Abelian Aharonov-Bohm effect | 4 pages, 4 figures | Phys. Rev. B 76, 233409 (2007) | 10.1103/PhysRevB.76.233409 | null | cond-mat.mes-hall | null | Recently, it has been shown that the spin-orbit coupling (SOC) of the
Dresselhaus type in $[110]$ quantum wells can be mathematically removed by a
non-Abelian gauge transformation. In the presence of an additional uniform
magnetic field, such a non-Abelian gauge flux leads to a spin accumulation at
the edges of the sample, where the relative sign of the spin accumulation
between the edges can be tuned by the sign of the Dresselhaus SOC constant. Our
prediction can be tested by Kerr measurements within the available experimental
sensitivities.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 02:24:02 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Liu",
"Qin",
""
],
[
"Ma",
"Tianxing",
""
],
[
"Zhang",
"Shou-Cheng",
""
]
] | [
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] |
704.0831 | Brooke Shrader | Brooke Shrader and Anthony Ephremides | On packet lengths and overhead for random linear coding over the erasure
channel | 5 pages, 5 figures, submitted to the 2007 International Wireless
Communications and Mobile Computing Conference | null | null | null | cs.IT math.IT | null | We assess the practicality of random network coding by illuminating the issue
of overhead and considering it in conjunction with increasingly long packets
sent over the erasure channel. We show that the transmission of increasingly
long packets, consisting of either of an increasing number of symbols per
packet or an increasing symbol alphabet size, results in a data rate
approaching zero over the erasure channel. This result is due to an erasure
probability that increases with packet length. Numerical results for a
particular modulation scheme demonstrate a data rate of approximately zero for
a large, but finite-length packet. Our results suggest a reduction in the
performance gains offered by random network coding.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 02:25:40 GMT"
}
] | "2007-07-13T00:00:00" | [
[
"Shrader",
"Brooke",
""
],
[
"Ephremides",
"Anthony",
""
]
] | [
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] |
704.0832 | Nader Haghighipour | Nader Haghighipour, Steinn Sigurdsson, Jack Lissauer, Sean Raymond | Terrestrial and Habitable Planet Formation in Binary and Multi-star
Systems | 7 pages, White Paper Submitted to the NASA/NSF ExoPlanet Task Force | null | null | null | astro-ph | null | One of the most surprising discoveries of extrasolar planets is the detection
of planets in moderately close binary star systems. The Jovian-type planets in
the two binaries of Gamma Cephei and GJ 86 have brought to the forefront
questions on the formation of giant planets and the possibility of the
existence of smaller bodies in such dynamically complex environments. The
diverse dynamical characteristics of these objects have made scientists wonder
to what extent the current theories of planet formation can be applied to
binaries and multiple star systems. At present, the sensitivity of the
detection techniques does not allow routine discovery of Earth-sized bodies in
binary systems. However, with the advancement of new techniques, and with the
recent launch of CoRoT and the launch of Kepler in late 2008, the detection of
more planets (possibly terrestrial-class objects) in such systems is on the
horizon. Theoretical studies and numerical modeling of terrestrial and
habitable planet formation are, therefore, necessary to gain fundamental
insights into the prospects for life in such systems and have great strategic
impact on NASA science and missions.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 02:34:35 GMT"
}
] | "2009-09-29T00:00:00" | [
[
"Haghighipour",
"Nader",
""
],
[
"Sigurdsson",
"Steinn",
""
],
[
"Lissauer",
"Jack",
""
],
[
"Raymond",
"Sean",
""
]
] | [
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] |
704.0833 | Kasso Okoudjou | \'Arp\'ad B\'enyi, Kasso A. Okoudjou | Local well-posedness of nonlinear dispersive equations on modulation
spaces | 11 pages | null | 10.1112/blms/bdp027 | null | math.AP math.CA | null | By using tools of time-frequency analysis, we obtain some improved local
well-posedness results for the NLS, NLW and NLKG equations with Cauchy data in
modulation spaces $M{p, 1}_{0,s}$.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 13:36:04 GMT"
}
] | "2014-02-26T00:00:00" | [
[
"Bényi",
"Árpád",
""
],
[
"Okoudjou",
"Kasso A.",
""
]
] | [
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] |
704.0834 | Anatoly Rodionov | Anatoly Rodionov, Sergey Volkov | P-adic arithmetic coding | 29 pages | null | null | null | cs.DS | null | A new incremental algorithm for data compression is presented. For a sequence
of input symbols algorithm incrementally constructs a p-adic integer number as
an output. Decoding process starts with less significant part of a p-adic
integer and incrementally reconstructs a sequence of input symbols. Algorithm
is based on certain features of p-adic numbers and p-adic norm. p-adic coding
algorithm may be considered as of generalization a popular compression
technique - arithmetic coding algorithms. It is shown that for p = 2 the
algorithm works as integer variant of arithmetic coding; for a special class of
models it gives exactly the same codes as Huffman's algorithm, for another
special model and a specific alphabet it gives Golomb-Rice codes.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 02:30:42 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Rodionov",
"Anatoly",
""
],
[
"Volkov",
"Sergey",
""
]
] | [
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] |
704.0835 | Teddy Cheung | C.C. Cheung | Compton X-ray and Gamma-ray Emission from Extended Radio Galaxies | 3 pages, one 3 panel figure. Proceedings of the First GLAST
Symposium. (The actual submitted version is 2 pages with references used more
sparingly.) | AIP Conf.Proc.921:325-326,2007 | 10.1063/1.2757334 | null | astro-ph | null | The extended lobes of radio galaxies are examined as sources of X-ray and
gamma-ray emission via inverse Compton scattering of 3K background photons. The
Compton spectra of two exemplary examples, Fornax A and Centaurus A, are
estimated using available radio measurements in the ~10's MHz - 10's GHz range.
For average lobe magnetic fields of >~0.3-1 micro-G, the lobe spectra are
predicted to extend into the soft gamma-rays making them likely detectable with
the GLAST LAT. If detected, their large angular extents (~1 deg and 8 deg) will
make it possible to ``image'' the radio lobes in gamma-rays. Similarly, this
process operates in more distant radio galaxies and the possibility that such
systems will be detected as unresolved gamma-ray sources with GLAST is briefly
considered.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 02:42:24 GMT"
}
] | "2009-06-23T00:00:00" | [
[
"Cheung",
"C. C.",
""
]
] | [
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] |
704.0836 | Kurt Luoto | Kurt W. Luoto | A matroid-friendly basis for the quasisymmetric functions | 25 pages; exposition tightened, typos corrected; to appear in the
Journal of Combinatorial Theory, Series A | Journal of Combinatorial Theory, Series A 115 (2008) 777-798 | 10.1016/j.jcta.2007.10.003 | null | math.CO | null | A new Z-basis for the space of quasisymmetric functions (QSym, for short) is
presented. It is shown to have nonnegative structure constants, and several
interesting properties relative to the space of quasisymmetric functions
associated to matroids by the Hopf algebra morphism (F) of Billera, Jia, and
Reiner. In particular, for loopless matroids, this basis reflects the grading
by matroid rank, as well as by the size of the ground set. It is shown that the
morphism F is injective on the set of rank two matroids, and that
decomposability of the quasisymmetric function of a rank two matroid mirrors
the decomposability of its base polytope. An affirmative answer is given to the
Hilbert basis question raised by Billera, Jia, and Reiner.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 02:43:59 GMT"
},
{
"version": "v2",
"created": "Fri, 16 Nov 2007 18:35:09 GMT"
}
] | "2010-11-30T00:00:00" | [
[
"Luoto",
"Kurt W.",
""
]
] | [
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] |
704.0837 | Jaeweon Lee Dr. | Jae-Weon Lee, Kyungsub Kim, Chul H. Lee, Ji-ho Jang | Bremsstrahlung Radiation At a Vacuum Bubble Wall | 6 pages, 2 figures, revtex, to appear in JKPS | Journal of the Korean Physical Society, 50, 1229 (2007) | 10.3938/jkps.50.1229 | null | hep-th | null | When charged particles collide with a vacuum bubble, they can radiate strong
electromagnetic waves due to rapid deceleration. Owing to the energy loss of
the particles by this bremsstrahlung radiation, there is a non-negligible
damping pressure acting on the bubble wall even when thermal equilibrium is
maintained. In the non-relativistic region, this pressure is proportional to
the velocity of the wall and could have influenced the bubble dynamics in the
early universe.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 02:55:57 GMT"
}
] | "2013-08-22T00:00:00" | [
[
"Lee",
"Jae-Weon",
""
],
[
"Kim",
"Kyungsub",
""
],
[
"Lee",
"Chul H.",
""
],
[
"Jang",
"Ji-ho",
""
]
] | [
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] |
704.0838 | Gil Shamir | Gil I. Shamir | Universal Source Coding for Monotonic and Fast Decaying Monotonic
Distributions | Submitted to IEEE Transactions on Information Theory | null | null | null | cs.IT math.IT | null | We study universal compression of sequences generated by monotonic
distributions. We show that for a monotonic distribution over an alphabet of
size $k$, each probability parameter costs essentially $0.5 \log (n/k^3)$ bits,
where $n$ is the coded sequence length, as long as $k = o(n^{1/3})$. Otherwise,
for $k = O(n)$, the total average sequence redundancy is $O(n^{1/3+\epsilon})$
bits overall. We then show that there exists a sub-class of monotonic
distributions over infinite alphabets for which redundancy of
$O(n^{1/3+\epsilon})$ bits overall is still achievable. This class contains
fast decaying distributions, including many distributions over the integers and
geometric distributions. For some slower decays, including other distributions
over the integers, redundancy of $o(n)$ bits overall is achievable, where a
method to compute specific redundancy rates for such distributions is derived.
The results are specifically true for finite entropy monotonic distributions.
Finally, we study individual sequence redundancy behavior assuming a sequence
is governed by a monotonic distribution. We show that for sequences whose
empirical distributions are monotonic, individual redundancy bounds similar to
those in the average case can be obtained. However, even if the monotonicity in
the empirical distribution is violated, diminishing per symbol individual
sequence redundancies with respect to the monotonic maximum likelihood
description length may still be achievable.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 03:12:02 GMT"
}
] | "2007-07-13T00:00:00" | [
[
"Shamir",
"Gil I.",
""
]
] | [
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] |
704.0839 | Grigory Mikhalkin | Grigory Mikhalkin | Moduli spaces of rational tropical curves | For the Proceedings of the Gokova Geometry/Topology Conference | null | null | null | math.AG math.CO math.GT math.SG | null | This note is devoted to the definition of moduli spaces of rational tropical
curves with n marked points. We show that this space has a structure of a
smooth tropical variety of dimension n-3. We define the Deligne-Mumford
compactification of this space and tropical $\psi$-class divisors.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 03:19:00 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Mikhalkin",
"Grigory",
""
]
] | [
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] |
704.084 | Yao-Bei Liu | Yao-Bei Liu, Jie-Fen Shen | Associated production of the charged Higgs boson and single top quark at
the LHC | This paper has been withdrawn by the author(s) due to some mistakes
in this paper | Mod.Phys.Lett.A24:143-150,2009 | 10.1142/S0217732309026711 | null | hep-ph | null | The left-right twin Higgs(LRTH) model predicts the existence of the charged
Higgs $\phi^{\pm}$. In this paper, we study the production of the charged Higgs
boson $\phi^{-}$ with single top quark via the process $bg\to t\phi^{-}$ at the
$CERN$ Large Hadron Collider(LHC). The numerical results show that the
production cross section can reach the level of $10 pb$ in the reasonable
parameter space of the LRTH model. We expect that, as long as it is not too
heavy, the possible signatures of the heavy charged Higgs boson $\phi^{-}$
might be detected via the decay mode $\phi^{-}\to \bar{t}b$ at the LHC
experiments.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 04:12:24 GMT"
},
{
"version": "v2",
"created": "Sat, 8 Mar 2008 14:05:11 GMT"
},
{
"version": "v3",
"created": "Thu, 13 Sep 2012 03:58:04 GMT"
}
] | "2012-09-14T00:00:00" | [
[
"Liu",
"Yao-Bei",
""
],
[
"Shen",
"Jie-Fen",
""
]
] | [
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704.0841 | Bang-Rong Zhou | Bang-Rong Zhou (Graduate School of Chinese Academy of Sciences) | Difermion condensates in vacuum in 2-4D four-fermion interaction models | 11 pages, 4 figures, General Poster 76 (Physical sciences) at 2007
AAAS Annual Meeting, San Francisco, Feb. 14-20, 2007, minor typos
corrected,acknowledgment to financial supporter added | null | null | null | hep-th | null | Theoretical analysis of interplay between the condensates $<\bar{q}q>$ and
$<qq>$ in vacuum is generally made by relativistic effective potentials in the
mean field approximation in 2D, 3D and 4D models with two flavor and $N_c$
color massless fermions. It is found that in ground states of these models,
interplay between the two condensates mainly depend on the ratio $G_S/H_S$ for
2D and 4D case or $G_S/H_P$ for 3D case, where $G_S$, $H_S$ and $H_P$ are
respectively the coupling constants in a scalar $(\bar{q}q)$, a scalar $(qq)$
and a pseudoscalar $(qq)$ channel. In ground states of all the models, only
pure $<\bar{q}q>$ condensates could exist if $G_S/H_S$ or $G_S/H_P$ is bigger
than the critical value $2/N_c$, the ratio of the color numbers of the fermions
entering into the condensates $<qq>$ and $<\bar{q}q>$. As $G_S/H_S$ or
$G_S/H_P$ decreases to the region below $2/N_c$, differences of the models will
manifest themselves. Depending on different models, and also on $N_c$ in 3D
model, one will have or have no the coexistence phase of the two condensates,
besides the pure $<qq>$ condensate phase. The $G_S-H_S$ (or $G_S-H_P$) phase
diagrams in these models are given. The results also implicate a real
constraint on two-flavor QCD-analogous NJL model.
| [
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704.0842 | Yanzhang He | Chengguang Bao | Oscillation bands of condensates on a ring: Beyond the mean field theory | 7 pages, 8 figures | Phys. Rev. A 75 (2007) 063626 | 10.1103/PhysRevA.75.063626 | null | cond-mat.other | null | The Hamiltonian of a N-boson system confined on a ring with zero spin and
repulsive interaction is diagonalized. The excitation of a pair of
p-wave-particles rotating reversely appears to be a basic mode. The fluctuation
of many of these excited pairs provides a mechanism of oscillation, the states
can be thereby classified into oscillation bands. The particle correlation is
studied intuitively via the two-body densities. Bose-clustering originating
from the symmetrization of wave functions is found, which leads to the
appearance of 1-, 2-, and 3-cluster structures. The motion is divided into
being collective and relative, this leads to the establishment of a relation
between the very high vortex states and the low-lying states.
| [
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0.0331532471
] |
704.0843 | Takuya Okabe | Takuya Okabe | Kadowaki-Woods Ratio of Strongly Coupled Fermi Liquids | null | Phys. Rev. B 76, 193109 (2007) | 10.1103/PhysRevB.76.193109 | null | cond-mat.str-el | null | On the basis of the Fermi liquid theory, the Kadowaki-Woods ratio
$A/\gamma^2$ is evaluated by using a first principle band calculation for
typical itinerant $d$ and $f$ electron systems. It is found as observed that
the ratio for the $d$ electron systems is significantly smaller than the normal
$f$ systems, even without considering their relatively weak correlation. The
difference in the ratio value comes from different characters of the Fermi
surfaces. By comparing Pd and USn$_3$ as typical cases, we discuss the
importance of the Fermi surface dependence of the quasiparticle transport
relaxation.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 06:09:57 GMT"
},
{
"version": "v2",
"created": "Tue, 2 Oct 2007 01:11:15 GMT"
}
] | "2008-02-08T00:00:00" | [
[
"Okabe",
"Takuya",
""
]
] | [
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704.0844 | Masayuki Matsuzaki | Masayuki Matsuzaki and Etsuchika Kobayashi (Fukuoka Univ. of Educ.) | Structure of Strange Dwarfs with Color Superconducting Core | 8 pages 5 figures, J. Phys. G, accepted | J.Phys.G34:1621-1626,2007 | 10.1088/0954-3899/34/7/004 | null | astro-ph hep-ph nucl-th | null | We study effects of two-flavor color superconductivity on the structure of
strange dwarfs, which are stellar objects with similar masses and radii with
ordinary white dwarfs but stabilized by the strange quark matter core. We find
that unpaired quark matter is a good approximation to the core of strange
dwarfs.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 05:42:41 GMT"
}
] | "2009-06-23T00:00:00" | [
[
"Matsuzaki",
"Masayuki",
"",
"Fukuoka Univ. of Educ."
],
[
"Kobayashi",
"Etsuchika",
"",
"Fukuoka Univ. of Educ."
]
] | [
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] |
704.0845 | Antti O. Niskanen | A. O. Niskanen, Y. Nakamura, J. P. Pekola | Information entropic superconducting microcooler | 4 pages, 3 figures | null | 10.1103/PhysRevB.76.174523 | null | cond-mat.supr-con | null | We consider a design for a cyclic microrefrigerator using a superconducting
flux qubit. Adiabatic modulation of the flux combined with thermalization can
be used to transfer energy from a lower temperature normal metal thin film
resistor to another one at higher temperature. The frequency selectivity of
photonic heat conduction is achieved by including the hot resistor as part of a
high frequency LC resonator and the cold one as part of a low-frequency
oscillator while keeping both circuits in the underdamped regime. We discuss
the performance of the device in an experimentally realistic setting. This
device illustrates the complementarity of information and thermodynamic entropy
as the erasure of the quantum bit directly relates to the cooling of the
resistor.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 07:05:03 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Niskanen",
"A. O.",
""
],
[
"Nakamura",
"Y.",
""
],
[
"Pekola",
"J. P.",
""
]
] | [
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] |
704.0846 | Heidi Haynal | Heidi Haynal | PI degree parity in q-skew polynomial rings | 43 pages; Submitted to the Journal of Algebra | null | null | null | math.RA math.QA | null | For k a field of arbitrary characteristic, and R a k-algebra, we show that
the PI degree of an iterated skew polynomial ring
R[x_1;\tau_1,\delta_1]...b[x_n;\tau_n,\delta_n] agrees with the PI degree of
R[x_1;\tau_1]...b[x_n;\tau_n] when each (\tau_i,\delta_i) satisfies a q_i-skew
relation for q_i \in k^{\times} and extends to a higher q_i-skew
\tau_i-derivation. We confirm the quantum Gel'fand-Kirillov conjecture for
various quantized coordinate rings, and calculate their PI degrees. We extend
these results to completely prime factor algebras.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 07:10:19 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Haynal",
"Heidi",
""
]
] | [
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704.0847 | Dorin Poenaru | D. N. Poenaru, R. A. Gherghescu, A. V. Solov'yov, W. Greiner | Semi-spheroidal Quantum Harmonic Oscillator | 4 pages, 3 figures, 1 table | null | 10.1016/j.physleta.2008.06.054 | null | physics.atm-clus | null | A new single-particle shell model is derived by solving the Schr\"odinger
equation for a semi-spheroidal potential well. Only the negative parity states
of the $Z(z)$ component of the wave function are allowed, so that new magic
numbers are obtained for oblate semi-spheroids, semi-sphere and prolate
semi-spheroids. The semi-spherical magic numbers are identical with those
obtained at the oblate spheroidal superdeformed shape: 2, 6, 14, 26, 44, 68,
100, 140, ... The superdeformed prolate magic numbers of the semi-spheroidal
shape are identical with those obtained at the spherical shape of the
spheroidal harmonic oscillator: 2, 8, 20, 40, 70, 112, 168 ...
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 17:51:47 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Poenaru",
"D. N.",
""
],
[
"Gherghescu",
"R. A.",
""
],
[
"Solov'yov",
"A. V.",
""
],
[
"Greiner",
"W.",
""
]
] | [
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704.0848 | Hyeong-Chai Jeong | Hyeong-Chai Jeong | Growing Perfect Decagonal Quasicrystals by Local Rules | 4pages, 2figures | Phys. Rev. Lett. 98, 135501 (2007) | 10.1103/PhysRevLett.98.135501 | null | cond-mat.dis-nn cond-mat.stat-mech math-ph math.MP | null | A local growth algorithm for a decagonal quasicrystal is presented. We show
that a perfect Penrose tiling (PPT) layer can be grown on a decapod tiling
layer by a three dimensional (3D) local rule growth. Once a PPT layer begins to
form on the upper layer, successive 2D PPT layers can be added on top resulting
in a perfect decagonal quasicrystalline structure in bulk with a point defect
only on the bottom surface layer. Our growth rule shows that an ideal
quasicrystal structure can be constructed by a local growth algorithm in 3D,
contrary to the necessity of non-local information for a 2D PPT growth.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 07:07:20 GMT"
}
] | "2015-05-13T00:00:00" | [
[
"Jeong",
"Hyeong-Chai",
""
]
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] |
704.0849 | Dr. Anirudh Pradhan | Anirudh Pradhan, J. P. Shahi and C. V. Singh | LRS Bianchi Type-V Viscous Fluid Universe With a Time Dependent
Cosmological Term $\Lambda$ | 13 pages, no figure | null | null | null | gr-qc | null | An LRS Bianchi type-V cosmological models representing a viscous fluid
distribution with a time dependent cosmological term $\Lambda$ is investigated.
To get a determinate solution, the viscosity coefficient of bulk viscous fluid
is assumed to be a power function of mass density. It turns out that the
cosmological term $\Lambda(t)$ is a decreasing function of time, which is
consistent with recent observations of type Ia supernovae. Various physical and
kinematic features of these models have also been explored.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 07:08:10 GMT"
},
{
"version": "v2",
"created": "Mon, 6 Aug 2007 05:58:45 GMT"
}
] | "2007-08-06T00:00:00" | [
[
"Pradhan",
"Anirudh",
""
],
[
"Shahi",
"J. P.",
""
],
[
"Singh",
"C. V.",
""
]
] | [
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] |
704.085 | Jun Sato | Jun Sato, Masahiro Shiroishi | Density matrix elements and entanglement entropy for the spin-1/2 XXZ
chain at $\Delta$=1/2 | 12 pages, 3 eps figures, 2 authors | J. Phys. A: Math. Theor. 40 8739-8749 (2007) | 10.1088/1751-8113/40/30/009 | null | cond-mat.stat-mech | null | We have analytically obtained all the density matrix elements up to six
lattice sites for the spin-1/2 Heisenberg XXZ chain at $\Delta=1/2$. We use the
multiple integral formula of the correlation function for the massless XXZ
chain derived by Jimbo and Miwa. As for the spin-spin correlation functions, we
have newly obtained the fourth- and fifth-neighbour transverse correlation
functions. We have calculated all the eigenvalues of the density matrix and
analyze the eigenvalue-distribution. Using these results the exact values of
the entanglement entropy for the reduced density matrix up six lattice sites
have been obtained. We observe that our exact results agree quite well with the
asymptotic formula predicted by the conformal field theory.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 07:19:49 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Sato",
"Jun",
""
],
[
"Shiroishi",
"Masahiro",
""
]
] | [
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704.0851 | Milan Janjic | Milan Janjic | Counting on rectangular areas | null | null | null | null | math.CO | null | In the first section of this paper we prove a theorem for the number of
columns of a rectangular area that are identical to the given one. In the next
section we apply this theorem to derive several combinatorial identities by
counting specified subsets of a finite set.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 07:29:24 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Janjic",
"Milan",
""
]
] | [
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] |
704.0852 | Dmitri Peressounko | D.Peressounko (for the PHENIX Collaboration) | Bose-Einstein correlations of direct photons in Au+Au collisions at
$\sqrt{s_{NN}} = 200$ GeV | 6 pages, 3 figures, Proceedings of Poster Session, 19th International
Conference on Ultra-Relativistic Nucleus-Nucleus Collisions (Quark Matter
2006), November 14-20, 2006, Shanghai, P.R.China | Int.J.Mod.Phys.E16:2235-2240,2007 | 10.1142/S021830130700774X | null | nucl-ex | null | The current status of the analysis of direct photon Bose-Einstein
correlations in Au+Au collisions at $\sqrt{s_{NN}}=200$ GeV done by the PHENIX
collaboration is summarized. All possible sources of distortion of the
two-photon correlation function are discussed and methods to control them in
the PHENIX experiment are presented.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 07:32:57 GMT"
}
] | "2010-11-26T00:00:00" | [
[
"Peressounko",
"D.",
"",
"for the PHENIX Collaboration"
]
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] |
704.0853 | Hao Yin | Hao Yin | Normalized Ricci flow on nonparabolic surfaces | Some false statements corrected. Details of estimate and a discussion
on Uniformization added. 14 pages | null | null | null | math.DG | null | This paper studies normalized Ricci flow on a nonparabolic surface, whose
scalar curvature is asymptotically -1 in an integral sense. By a method
initiated by R. Hamilton, the flow is shown to converge to a metric of constant
scalar curvature -1. A relative estimate of Green's function is proved as a
tool.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 07:53:53 GMT"
},
{
"version": "v2",
"created": "Tue, 5 Jun 2007 01:44:15 GMT"
}
] | "2007-06-13T00:00:00" | [
[
"Yin",
"Hao",
""
]
] | [
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] |
704.0854 | Xifeng Ren | Xi-Feng Ren, Pei Zhang, Guo-Ping Guo, Yun-Feng Huang, Zhi-Wei Wang,
Guang-Can Guo | Polarization properties of subwavelength hole arrays consisting of
rectangular holes | 8 pages, 4 figures | Appl.Phys.B 91 601(2008) | 10.1007/s00340-008-3027-1 | null | physics.optics | null | Influence of hole shape on extraordinary optical transmission was
investigated using hole arrays consisting of rectangular holes with different
aspect ratio. It was found that the transmission could be tuned continuously by
rotating the hole array. Further more, a phase was generated in this process,
and linear polarization states could be changed to elliptical polarization
states. This phase was correlated with the aspect ratio of the holes. An
intuitional model was presented to explain these results.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 08:09:02 GMT"
},
{
"version": "v2",
"created": "Wed, 4 Jun 2008 01:41:36 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Ren",
"Xi-Feng",
""
],
[
"Zhang",
"Pei",
""
],
[
"Guo",
"Guo-Ping",
""
],
[
"Huang",
"Yun-Feng",
""
],
[
"Wang",
"Zhi-Wei",
""
],
[
"Guo",
"Guang-Can",
""
]
] | [
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] |
704.0855 | David Wilkowski | Thierry Chaneliere (LAC), Ling Xiang He, Robin Kaiser (INLN), David
Wilkowski (INLN) | Three dimensional cooling and trapping with a narrow line | null | null | 10.1140/epjd/e2007-00329-8 | null | physics.atom-ph | null | The intercombination line of Strontium at 689nm is successfully used in laser
cooling to reach the photon recoil limit with Doppler cooling in a
magneto-optical traps (MOT). In this paper we present a systematic study of the
loading efficiency of such a MOT. Comparing the experimental results to a
simple model allows us to discuss the actual limitation of our apparatus. We
also study in detail the final MOT regime emphasizing the role of gravity on
the position, size and temperature along the vertical and horizontal
directions. At large laser detuning, one finds an unusual situation where
cooling and trapping occur in the presence of a high bias magnetic field.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 08:06:59 GMT"
},
{
"version": "v2",
"created": "Fri, 10 Aug 2007 09:07:23 GMT"
}
] | "2015-05-13T00:00:00" | [
[
"Chaneliere",
"Thierry",
"",
"LAC"
],
[
"He",
"Ling Xiang",
"",
"INLN"
],
[
"Kaiser",
"Robin",
"",
"INLN"
],
[
"Wilkowski",
"David",
"",
"INLN"
]
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704.0856 | Iosif Khriplovich | I.B. Khriplovich and D.V. Matvienko | Approximate Selection Rule for Orbital Angular Momentum in Atomic
Radiative Transitions | 5 pages, 1 figure | Phys. Lett. A 368 (2007) 348 | 10.1016/j.physleta.2007.04.031 | null | physics.atom-ph physics.class-ph | null | We demonstrate that radiative transitions with \Delta l = - 1 are strongly
dominating for all values of n and l, except small region where l << n.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 08:08:30 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Khriplovich",
"I. B.",
""
],
[
"Matvienko",
"D. V.",
""
]
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704.0857 | Ivan L. Zhogin | I.L. Zhogin | Extrasolar scale change in Newton's Law from 5D `plain' R^2-gravity | Latex, 10 pages, 1 figure (poster.pdf submitted to NPPD-07 is addon) | null | null | null | astro-ph gr-qc hep-ph | null | Galactic rotation curves and lack of direct observations of Dark Matter may
indicate that General Relativity is not valid (on galactic scale) and should be
replaced with another theory. There is the only variant of Absolute Parallelism
which solutions are free of arising singularities, if D=5 (there is no room for
changes). This variant does not have a Lagrangian, nor match GR: an equation of
`plain' R^2-gravity (ie without R-term) is in sight instead. Arranging an
expanding O_4-symmetrical solution as the basis of 5D cosmological model, and
probing a universal_function of mass distribution (along very-very long the
extra dimension) to place into bi-Laplace equation (R^2 gravity), one can
derive the Law of Gravitation: 1/r^2 transforms to 1/r with distance (not with
acceleration).
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 08:47:44 GMT"
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] | "2009-04-16T00:00:00" | [
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"Zhogin",
"I. L.",
""
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] |
704.0858 | Mohamed Kaaniche | Eric Alata (LAAS), Vincent Nicomette (LAAS), Mohamed Ka\^aniche
(LAAS), Marc Dacier (LAAS), Matthieu Herrb (LAAS) | Lessons Learned from the deployment of a high-interaction honeypot | null | Proc. 6th European Dependable Computing Conference (EDCC-6),
Coimbra (Portugal), 18-20 octobre 2006 (18/10/2006) 39-44 | null | null | cs.CR | null | This paper presents an experimental study and the lessons learned from the
observation of the attackers when logged on a compromised machine. The results
are based on a six months period during which a controlled experiment has been
run with a high interaction honeypot. We correlate our findings with those
obtained with a worldwide distributed system of lowinteraction honeypots.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 08:22:50 GMT"
}
] | "2016-08-14T00:00:00" | [
[
"Alata",
"Eric",
"",
"LAAS"
],
[
"Nicomette",
"Vincent",
"",
"LAAS"
],
[
"Kaâniche",
"Mohamed",
"",
"LAAS"
],
[
"Dacier",
"Marc",
"",
"LAAS"
],
[
"Herrb",
"Matthieu",
"",
"LAAS"
]
] | [
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] |
704.0859 | B\'alint Farkas | Balint Farkas, Bela Nagy | Transfinite diameter, Chebyshev constant and energy on locally compact
spaces | null | null | null | null | math.CA | null | We study the relationship between transfinite diameter, Chebyshev constant
and Wiener energy in the abstract linear potential analytic setting pioneered
by Choquet, Fuglede and Ohtsuka. It turns out that, whenever the potential
theoretic kernel has the maximum principle, then all these quantities are equal
for all compact sets. For continuous kernels even the converse statement is
true: if the Chebyshev constant of any compact set coincides with its
transfinite diameter, the kernel must satisfy the maximum principle. An
abundance of examples is provided to show the sharpness of the results.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 08:30:02 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Farkas",
"Balint",
""
],
[
"Nagy",
"Bela",
""
]
] | [
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] |
704.086 | Mohamed Kaaniche | Cristina Simache (LAAS), Mohamed Kaaniche (LAAS) | Availability assessment of SunOS/Solaris Unix Systems based on Syslogd
and wtmpx logfiles : a case study | null | Proc. 2005 IEEE Pacific Rim International Symposium on Dependable
Computing (PRDC'2005), Changsha, Hunan (Chine), 12-14 D{\'e}cembre 2005
(18/12/2005) 49-56 | null | null | cs.PF | null | This paper presents a measurement-based availability assessment study using
field data collected during a 4-year period from 373 SunOS/Solaris Unix
workstations and servers interconnected through a local area network. We focus
on the estimation of machine uptimes, downtimes and availability based on the
identification of failures that caused total service loss. Data corresponds to
syslogd event logs that contain a large amount of information about the normal
activity of the studied systems as well as their behavior in the presence of
failures. It is widely recognized that the information contained in such event
logs might be incomplete or imperfect. The solution investigated in this paper
to address this problem is based on the use of auxiliary sources of data
obtained from wtmpx files maintained by the SunOS/Solaris Unix operating
system. The results obtained suggest that the combined use of wtmpx and syslogd
log files provides more complete information on the state of the target systems
that is useful to provide availability estimations that better reflect reality.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 08:24:47 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Simache",
"Cristina",
"",
"LAAS"
],
[
"Kaaniche",
"Mohamed",
"",
"LAAS"
]
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] |
704.0861 | Mohamed Kaaniche | Mohamed Kaaniche (LAAS), Y. Deswarte (LAAS), Eric Alata (LAAS), Marc
Dacier (SC), Vincent Nicomette (LAAS) | Empirical analysis and statistical modeling of attack processes based on
honeypots | null | IEEE/IFIP International Conference on Dependable Systems and
Networks (DSN-2006) (25/06/2006) 119-124 | null | null | cs.PF cs.CR | null | Honeypots are more and more used to collect data on malicious activities on
the Internet and to better understand the strategies and techniques used by
attackers to compromise target systems. Analysis and modeling methodologies are
needed to support the characterization of attack processes based on the data
collected from the honeypots. This paper presents some empirical analyses based
on the data collected from the Leurr{\'e}.com honeypot platforms deployed on
the Internet and presents some preliminary modeling studies aimed at fulfilling
such objectives.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 08:50:34 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Kaaniche",
"Mohamed",
"",
"LAAS"
],
[
"Deswarte",
"Y.",
"",
"LAAS"
],
[
"Alata",
"Eric",
"",
"LAAS"
],
[
"Dacier",
"Marc",
"",
"SC"
],
[
"Nicomette",
"Vincent",
"",
"LAAS"
]
] | [
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] |
704.0862 | Adam Leroy | Adam Leroy, John Cannon, Fabian Walter, Alberto Bolatto, Axel Weiss | The Low CO Content of the Extremely Metal Poor Galaxy I Zw 18 | 5 pages in emulateapj style, accepted by the Astrophysical Journal | Astrophys.J.663:990-994,2007 | 10.1086/518501 | null | astro-ph | null | We present sensitive molecular line observations of the metal-poor blue
compact dwarf I Zw 18 obtained with the IRAM Plateau de Bure interferometer.
These data constrain the CO J=1-0 luminosity within our 300 pc (FWHM) beam to
be L_CO < 1 \times 10^5 K km s^-1 pc^2 (I_CO < 1 K km s^-1), an order of
magnitude lower than previous limits. Although I Zw 18 is starbursting, it has
a CO luminosity similar to or less than nearby low-mass irregulars (e.g. NGC
1569, the SMC, and NGC 6822). There is less CO in I Zw 18 relative to its
B-band luminosity, HI mass, or star formation rate than in spiral or dwarf
starburst galaxies (including the nearby dwarf starburst IC 10). Comparing the
star formation rate to our CO upper limit reveals that unless molecular gas
forms stars much more efficiently in I Zw 18 than in our own galaxy, it must
have a very low CO-to-H_2 ratio, \sim 10^-2 times the Galactic value. We detect
3mm continuum emission, presumably due to thermal dust and free-free emission,
towards the radio peak.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 08:50:39 GMT"
}
] | "2009-06-23T00:00:00" | [
[
"Leroy",
"Adam",
""
],
[
"Cannon",
"John",
""
],
[
"Walter",
"Fabian",
""
],
[
"Bolatto",
"Alberto",
""
],
[
"Weiss",
"Axel",
""
]
] | [
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] |
704.0863 | Zhanwen Han | Z. Han, Ph. Podsiadlowski, A.E. Lynas-Gray | A binary model for the UV-upturn of elliptical galaxies (MNRAS version) | accepted for publication in MNRAS, 24 pages, 15 figures, 2 tables | null | 10.1111/j.1365-2966.2007.12151.x | UVX-MN-25June2007 | astro-ph | null | The discovery of a flux excess in the far-ultraviolet (UV) spectrum of
elliptical galaxies was a major surprise in 1969. While it is now clear that
this UV excess is caused by an old population of hot helium-burning stars
without large hydrogen-rich envelopes, rather than young stars, their origin
has remained a mystery. Here we show that these stars most likely lost their
envelopes because of binary interactions, similar to the hot subdwarf
population in our own Galaxy. We have developed an evolutionary population
synthesis model for the far-UV excess of elliptical galaxies based on the
binary model developed by Han et al (2002, 2003) for the formation of hot
subdwarfs in our Galaxy. Despite its simplicity, it successfully reproduces
most of the properties of elliptical galaxies with a UV excess: the range of
observed UV excesses, both in $(1550-V)$ and $(2000-V)$, and their evolution
with redshift. We also present colour-colour diagrams for use as diagnostic
tools in the study of elliptical galaxies. The model has major implications for
understanding the evolution of the UV excess and of elliptical galaxies in
general. In particular, it implies that the UV excess is not a sign of age, as
had been postulated previously, and predicts that it should not be strongly
dependent on the metallicity of the population, but exists universally from
dwarf ellipticals to giant ellipticals.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 13:55:07 GMT"
},
{
"version": "v2",
"created": "Mon, 30 Apr 2007 03:12:38 GMT"
},
{
"version": "v3",
"created": "Mon, 25 Jun 2007 11:49:33 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Han",
"Z.",
""
],
[
"Podsiadlowski",
"Ph.",
""
],
[
"Lynas-Gray",
"A. E.",
""
]
] | [
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] |
704.0864 | Istvan Horvath | Z. Bagoly, I. Csabai, A. Meszaros, P. Meszaros, I. Horvath, L.G.
Balazs, R. Vavrek | Redshifts of the Long Gamma-Ray Bursts | published in Baltic Astronomy | Baltic Astron. 13 (2004) 227 | null | null | astro-ph | null | The low energy spectra of some gamma-ray bursts' show excess components
beside the power-law dependence. The consequences of such a feature allows to
estimate the gamma photometric redshift of the long gamma-ray bursts in the
BATSE Catalog. There is good correlation between the measured optical and the
estimated gamma photometric redshifts. The estimated redshift values for the
long bright gamma-ray bursts are up to z=4, while for the the faint long bursts
- which should be up to z=20 - the redshifts cannot be determined unambiguously
with this method. The redshift distribution of all the gamma-ray bursts with
known optical redshift agrees quite well with the BATSE based gamma photometric
redshift distribution.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 09:09:15 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Bagoly",
"Z.",
""
],
[
"Csabai",
"I.",
""
],
[
"Meszaros",
"A.",
""
],
[
"Meszaros",
"P.",
""
],
[
"Horvath",
"I.",
""
],
[
"Balazs",
"L. G.",
""
],
[
"Vavrek",
"R.",
""
]
] | [
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] |
704.0865 | Mohamed Kaaniche | Ana-Elena Rugina (LAAS), Karama Kanoun (LAAS), Mohamed Kaaniche (LAAS) | An architecture-based dependability modeling framework using AADL | null | Proc. 10th IASTED International Conference on Software Engineering
and Applications (SEA'2006), Dallas (USA), 13-15 November2006 (13/11/2006)
222-227 | null | null | cs.PF cs.SE | null | For efficiency reasons, the software system designers' will is to use an
integrated set of methods and tools to describe specifications and designs, and
also to perform analyses such as dependability, schedulability and performance.
AADL (Architecture Analysis and Design Language) has proved to be efficient for
software architecture modeling. In addition, AADL was designed to accommodate
several types of analyses. This paper presents an iterative dependency-driven
approach for dependability modeling using AADL. It is illustrated on a small
example. This approach is part of a complete framework that allows the
generation of dependability analysis and evaluation models from AADL models to
support the analysis of software and system architectures, in critical
application domains.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 09:33:06 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Rugina",
"Ana-Elena",
"",
"LAAS"
],
[
"Kanoun",
"Karama",
"",
"LAAS"
],
[
"Kaaniche",
"Mohamed",
"",
"LAAS"
]
] | [
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] |
704.0866 | Ahmed Zeriahi | S.Benelkourchi, V.Guedj and A.Zeriahi | A priori estimates for weak solutions of complex Monge-Amp\`ere
equations | Corrected typos, added details to one proof | Ann. Scuola Norm. Sup. Pisa, Cl. Sci. (5) Vol. VII (2008), 1-16 | null | null | math.CV math.DG | null | Let $X$ be a compact K\"ahler manifold and $\om$ a smooth closed form of
bidegree $(1,1)$ which is nonnegative and big. We study the classes ${\mathcal
E}_{\chi}(X,\om)$ of $\om$-plurisubharmonic functions of finite weighted
Monge-Amp\`ere energy. When the weight $\chi$ has fast growth at infinity, the
corresponding functions are close to be bounded.
We show that if a positive Radon measure is suitably dominated by the
Monge-Amp\`ere capacity, then it belongs to the range of the Monge-Amp\`ere
operator on some class ${\mathcal E}_{\chi}(X,\om)$. This is done by
establishing a priori estimates on the capacity of sublevel sets of the
solutions.
Our result extends U.Cegrell's and S.Kolodziej's results and puts them into a
unifying frame. It also gives a simple proof of S.T.Yau's celebrated a priori
${\mathcal C}^0$-estimate.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 10:06:50 GMT"
},
{
"version": "v2",
"created": "Fri, 22 Feb 2008 08:17:56 GMT"
}
] | "2008-02-22T00:00:00" | [
[
"Benelkourchi",
"S.",
""
],
[
"Guedj",
"V.",
""
],
[
"Zeriahi",
"A.",
""
]
] | [
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] |
704.0867 | Yanzhang He | Shuping Situ, Yanzhang He and Chengguang Bao | Density oscillation in highly flattened quantum elliptic rings and
tunable strong dipole radiation | 5 pages, 8 figures | null | null | null | cond-mat.other | null | A narrow elliptic ring containing an electron threaded by a magnetic field B
is studied. When the ring is highly flattened, the increase of B would lead to
a big energy gap between the ground and excited states, and therefore lead to a
strong emission of dipole photons. The photon frequency can be tuned in a wide
range by changing B and/or the shape of the ellipse. The particle density is
found to oscillate from a pattern of distribution to another pattern back and
forth against $B$. This is a new kind of Aharonov-Bohm oscillation originating
from symmetry breaking and is different from the usual oscillation of
persistent current.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 10:11:40 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Situ",
"Shuping",
""
],
[
"He",
"Yanzhang",
""
],
[
"Bao",
"Chengguang",
""
]
] | [
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] |
704.0868 | Andrea Bertoni | Juan I. Climente, Andrea Bertoni, Guido Goldoni, Massimo Rontani,
Elisa Molinari | Effect of electron-electron interaction on the phonon-mediated spin
relaxation in quantum dots | 12 pages, 10 figures. Revised version. Changes in section V
(simulation of PRL 98, 126601 experiment) | Phys. Rev. B 76, 085305 (2007) | 10.1103/PhysRevB.76.085305 | null | cond-mat.mes-hall | null | We estimate the spin relaxation rate due to spin-orbit coupling and acoustic
phonon scattering in weakly-confined quantum dots with up to five interacting
electrons. The Full Configuration Interaction approach is used to account for
the inter-electron repulsion, and Rashba and Dresselhaus spin-orbit couplings
are exactly diagonalized. We show that electron-electron interaction strongly
affects spin-orbit admixture in the sample. Consequently, relaxation rates
strongly depend on the number of carriers confined in the dot. We identify the
mechanisms which may lead to improved spin stability in few electron (>2)
quantum dots as compared to the usual one and two electron devices. Finally, we
discuss recent experiments on triplet-singlet transitions in GaAs dots subject
to external magnetic fields. Our simulations are in good agreement with the
experimental findings, and support the interpretation of the observed spin
relaxation as being due to spin-orbit coupling assisted by acoustic phonon
emission.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 10:28:43 GMT"
},
{
"version": "v2",
"created": "Mon, 11 Jun 2007 09:30:17 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Climente",
"Juan I.",
""
],
[
"Bertoni",
"Andrea",
""
],
[
"Goldoni",
"Guido",
""
],
[
"Rontani",
"Massimo",
""
],
[
"Molinari",
"Elisa",
""
]
] | [
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] |
704.0869 | O. Golinelli | O. Golinelli, K. Mallick (Cea Saclay, France) | Connected Operators for the Totally Asymmetric Exclusion Process | 10 pages | J. Phys. A: Math. Theor. 40 (2007) 13231-13236 | 10.1088/1751-8113/40/44/004 | null | cond-mat.stat-mech math-ph math.MP | null | We fully elucidate the structure of the hierarchy of the connected operators
that commute with the Markov matrix of the Totally Asymmetric Exclusion Process
(TASEP). We prove for the connected operators a combinatorial formula that was
conjectured in a previous work. Our derivation is purely algebraic and relies
on the algebra generated by the local jump operators involved in the TASEP.
Keywords: Non-Equilibrium Statistical Mechanics, ASEP, Exact Results,
Algebraic Bethe Ansatz.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 10:15:25 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Golinelli",
"O.",
"",
"Cea Saclay, France"
],
[
"Mallick",
"K.",
"",
"Cea Saclay, France"
]
] | [
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] |
704.087 | Evgeniy Bessonov | E.G. Bessonov, M.V. Gorbunkov (Lebedev Phys. Inst. RAS, Moscow,
Russia), A.A.Mikhailichenko (Cornell University, Ithaca, NY, U.S.A.) | Proposal for an Enhanced Optical Cooling System Test in an Electron
Storage Ring | 21 pages, pdf. The number of electrons in the bunch in the example is
decreased, the volume of the paper is increased, Misprints are corrected | Phys.Rev.STAccel.Beams11:011302,2008 | 10.1103/PhysRevSTAB.11.011302 | null | physics.acc-ph | null | We are proposing to test experimentally the new idea of Enhanced Optical
Cooling (EOC) in an electron storage ring. This experiment will confirm new
fundamental processes in beam physics and will demonstrate new unique
possibilities with this cooling technique. It will open important applications
of EOC in nuclear physics, elementary particle physics and in Light Sources
(LS) based on high brightness electron and ion beams.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 10:25:48 GMT"
},
{
"version": "v2",
"created": "Wed, 16 May 2007 09:49:23 GMT"
}
] | "2008-11-26T00:00:00" | [
[
"Bessonov",
"E. G.",
"",
"Lebedev Phys. Inst. RAS, Moscow,\n Russia"
],
[
"Gorbunkov",
"M. V.",
"",
"Lebedev Phys. Inst. RAS, Moscow,\n Russia"
],
[
"Mikhailichenko",
"A. A.",
"",
"Cornell University, Ithaca, NY, U.S.A."
]
] | [
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] |
704.0871 | Krisztina Eva Gabanyi | K. E. Gabanyi (1,2), N. Marchili (1), T. P. Krichbaum (1), S. Britzen
(1), L. Fuhrmann (1), A. Witzel (1), J. A. Zensus (1), P. Muller (1), X. Liu
(3), H. G. Song (3), J. L. Han (4), X. H. Sun (4) ((1) Max-Planck-Institut
fur Radioastronomie, (2) Hungarian Academy of Sciences, Research Group for
Physical Geodesy and Geodynamics, (3) Urumqi Observatory, the National
Astronomical Observatories, the Chinese Academy of Sciences, (4) National
Astronomical Observatories, Chinese Academy of Sciences) | The IDV source J1128+5925, a new candidate for annual modulation? | 15 pages, 9 figures Accepted for publication in Astronomy and
Astrophysics | null | 10.1051/0004-6361:20067033 | null | astro-ph | null | Short time-scale radio variations of compact extragalactic radio sources,
known as IntraDay Variability, can be explained in at least some sources by a
source-extrinsic effect, in which the variations are interpreted as
scintillation of radio waves caused by the turbulent ISM of the Milky Way. One
of the most convincing observational arguments in favour of propagation-induced
variability is the so called annual modulation of the characteristic
variability time-scale, which is due to the orbital motion of the Earth. Data
for the recently discovered and highly variable IDV source J1128+5925 are
presented. We study the frequency and time dependence of the IDV in this
compact quasar. We measure the characteristic variability time-scale of the IDV
throughout the year, and analyze whether the observed changes in the
variability time-scale are consistent with annual modulation. We monitored the
flux density variability of J1128+5925 with dense time sampling between 2.7 and
10.45GHz with the 100m Effelsberg radio telescope of the MPIfR and with the 25m
Urumqi radio telescope. From ten observing sessions, we determine the
variability characteristics and time-scales. The observed pronounced changes of
the variability time-scale of J1128+5925 are modelled with an anisotropic
annual modulation model. The observed frequency dependence of the variation is
in good agreement with the prediction from interstellar scintillation. Adopting
a simple model for the annual modulation model and using also the frequency
dependence of the IDV, we derive a lower limit to the distance of the
scattering screen and an upper limit to the scintillating source size. The
latter is found to be consistent with the measured core size from VLBI.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 10:54:17 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Gabanyi",
"K. E.",
""
],
[
"Marchili",
"N.",
""
],
[
"Krichbaum",
"T. P.",
""
],
[
"Britzen",
"S.",
""
],
[
"Fuhrmann",
"L.",
""
],
[
"Witzel",
"A.",
""
],
[
"Zensus",
"J. A.",
""
],
[
"Muller",
"P.",
""
],
[
"Liu",
"X.",
""
],
[
"Song",
"H. G.",
""
],
[
"Han",
"J. L.",
""
],
[
"Sun",
"X. H.",
""
]
] | [
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] |
704.0872 | Kre\v{s}imir Veseli\'c | K. Veselic | Spectral perturbation bounds for selfadjoint operators | 30 pages | null | null | null | math.SP | null | We give general spectral and eigenvalue perturbation bounds for a selfadjoint
operator perturbed in the sense of the pseudo-Friedrichs extension. We also
give several generalisations of the aforementioned extension. The spectral
bounds for finite eigenvalues are obtained by using analyticity and
monotonicity properties (rather than variational principles) and they are
general enough to include eigenvalues in gaps of the essential spectrum.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 10:47:51 GMT"
},
{
"version": "v2",
"created": "Mon, 21 Jan 2008 17:24:43 GMT"
}
] | "2008-01-21T00:00:00" | [
[
"Veselic",
"K.",
""
]
] | [
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] |
704.0873 | Jane Greaves | J.S. Greaves, D.A. Fischer, M.C. Wyatt, C.A. Beichman and G. Bryden | Predicting the frequencies of diverse exo-planetary systems | 5 pages, 2 figures; accepted by MNRAS | Mon.Not.Roy.Astron.Soc.Lett.378:L1-L5,2007 | 10.1111/j.1745-3933.2007.00315.x | null | astro-ph | null | Extrasolar planetary systems range from hot Jupiters out to icy comet belts
more distant than Pluto. We explain this diversity in a model where the mass of
solids in the primordial circumstellar disk dictates the outcome. The star
retains measures of the initial heavy-element (metal) abundance that can be
used to map solid masses onto outcomes, and the frequencies of all classes are
correctly predicted. The differing dependences on metallicity for forming
massive planets and low-mass cometary bodies are also explained. By
extrapolation, around two-thirds of stars have enough solids to form Earth-like
planets, and a high rate is supported by the first detections of low-mass
exo-planets.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 11:04:07 GMT"
}
] | "2009-06-23T00:00:00" | [
[
"Greaves",
"J. S.",
""
],
[
"Fischer",
"D. A.",
""
],
[
"Wyatt",
"M. C.",
""
],
[
"Beichman",
"C. A.",
""
],
[
"Bryden",
"G.",
""
]
] | [
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] |
704.0874 | Gavril Farkas | Gavril Farkas | Higher ramification and varieties of secant divisors on the generic
curve | 25 pages. Numerous changes suggested by the referee, several proofs
explained in more detail. To appear in the Journal of the London Mathematical
Society | J. London Math. Soc. 78(2008) 418-440 | null | null | math.AG | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | For a smooth projective curve, the cycles of e-secant k-planes are among the
most studied objects in classical enumerative geometry and there are well-known
formulas due to Castelnuovo, Cayley and MacDonald concerning them. Despite
various attempts, surprisingly little is known about the enumerative validity
of such formulas. The aim of this paper is to completely clarify this problem
in the case of the generic curve C of given genus. Using degeneration
techniques and a few facts about the birational geometry of moduli spaces of
stable pointed curves we determine precisely under which conditions the cycle
of e-secant k-planes in non-empty and we compute its dimension. We also
precisely determine the dimension of the variety of linear series on C carrying
e-secant k-planes. In a different direction, in the last part of the paper we
study the distribution of ramification points of the powers of a line bundle on
C having prescribed ramification at a given point.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 11:07:01 GMT"
},
{
"version": "v2",
"created": "Wed, 30 Apr 2008 17:03:55 GMT"
},
{
"version": "v3",
"created": "Thu, 20 Nov 2014 15:03:16 GMT"
}
] | "2014-11-21T00:00:00" | [
[
"Farkas",
"Gavril",
""
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] |
704.0875 | Boris Tarasov | Boris V. Tarasov | The concrete theory of numbers: initial numbers and wonderful properties
of numbers repunit | 8 pages ; v3: minor grammatical changes, etc | null | null | null | math.GM | null | In this work initial numbers and repunit numbers have been studied. All
numbers have been considered in a decimal notation. The problem of simplicity
of initial numbers has been studied. Interesting properties of numbers repunit
are proved:
$gcd(R_a, R_b) = R_{gcd(a,b)}$;
$R_{ab}/(R_aR_b)$ is an integer only if $gcd(a,b) = 1$, where $a\geq1$,
$b\geq1$ are integers. Dividers of numbers repunit, are researched by a degree
of prime number.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 11:08:20 GMT"
},
{
"version": "v2",
"created": "Sat, 7 Apr 2007 10:15:04 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Tarasov",
"Boris V.",
""
]
] | [
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704.0876 | Josef Teichmann | Walter Schachermayer, Uwe Schmock, Josef Teichmann | Non-monotone convergence in the quadratic Wasserstein distance | null | null | null | null | math.PR | null | We give an easy counter-example to Problem 7.20 from C. Villani's book on
mass transport: in general, the quadratic Wasserstein distance between $n$-fold
normalized convolutions of two given measures fails to decrease monotonically.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 11:15:47 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Schachermayer",
"Walter",
""
],
[
"Schmock",
"Uwe",
""
],
[
"Teichmann",
"Josef",
""
]
] | [
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] |
704.0877 | Filippo Mannucci | F. Mannucci, N. Panagia, M. Della Valle | The bimodality of type Ia Supernovae | 5 pages, to appear in the AIP conference proceedings of "Supernova
1987A: 20 Years after Supernovae and Gamma-Ray Bursters", Feb 19-23, 2007,
Aspen, CO. Replaced figure 1 | AIP Conf.Proc.937:293-297,2007 | 10.1063/1.2803580 | null | astro-ph | null | We comment on the presence of a bimodality in the distribution of delay time
between the formation of the progenitors and their explosion as type Ia SNe.
Two "flavors" of such bimodality are present in the literature: a "weak"
bimodality, in which type Ia SNe must explode from both young and old
progenitors, and a "strong" bimodality, in which about half of the systems
explode within 10^8 years from formation. The "weak" bimodality is
observationally based on the dependence of the rates with the host galaxy SFR,
while the "strong" one on the different rates in radio-loud and radio-quiet
early-type galaxies. We review the evidence for these bimodalities. Finally, we
estimate the fraction of SNe which are missed by optical and near-IR searches
because of dust extinction in massive starbursts.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 11:28:09 GMT"
},
{
"version": "v2",
"created": "Wed, 4 Jul 2007 13:11:02 GMT"
}
] | "2009-09-29T00:00:00" | [
[
"Mannucci",
"F.",
""
],
[
"Panagia",
"N.",
""
],
[
"Della Valle",
"M.",
""
]
] | [
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] |
704.0878 | Amelie Juhin | Am\'elie Juhin (IMPMC), Georges Calas (IMPMC), Delphine Cabaret
(IMPMC), Laurence Galoisy (IMPMC), Jean-Louis Hazemann | Structural relaxation around substitutional Cr3+ in MgAl2O4 | 7 pages, 4 figures | null | 10.1103/PhysRevB.76.054105 | null | cond-mat.mtrl-sci | null | The structural environment of substitutional Cr3+ ion in MgAl2O4 spinel has
been investigated by Cr K-edge Extended X-ray Absorption Fine Structure (EXAFS)
and X-ray Absorption Near Edge Structure (XANES) spectroscopies.
First-principles computations of the structural relaxation and of the XANES
spectrum have been performed, with a good agreement to the experiment. The Cr-O
distance is close to that in MgCr2O4, indicating a full relaxation of the first
neighbors, and the second shell of Al atoms relaxes partially. These
observations demonstrate that Vegard's law is not obeyed in the MgAl2O4-MgCr2O4
solid solution. Despite some angular site distortion, the local D3d symmetry of
the B-site of the spinel structure is retained during the substitution of Cr
for Al. Here, we show that the relaxation is accomodated by strain-induced bond
buckling, with angular tilts of the Mg-centred tetrahedra around the Cr-centred
octahedron. By contrast, there is no significant alteration of the angles
between the edge-sharing octahedra, which build chains aligned along the three
four-fold axes of the cubic structure.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 11:46:08 GMT"
}
] | "2016-08-14T00:00:00" | [
[
"Juhin",
"Amélie",
"",
"IMPMC"
],
[
"Calas",
"Georges",
"",
"IMPMC"
],
[
"Cabaret",
"Delphine",
"",
"IMPMC"
],
[
"Galoisy",
"Laurence",
"",
"IMPMC"
],
[
"Hazemann",
"Jean-Louis",
""
]
] | [
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704.0879 | Mohamed Kaaniche | Mohamed Kaaniche (LAAS), Luigi Romano (UIUC), Zbigniew Kalbarczyk
(UIUC), Ravishankar Iyer (UIUC), Rick Karcich (STORAGETEK) | A Hierarchical Approach for Dependability Analysis of a Commercial
Cache-Based RAID Storage Architecture | null | Proc. 28th IEEE International Symposium on Fault-Tolerant
Computing (FTCS-28), Munich (Germany), IEEE Computer Society, June 1998,
pp.6-15 (1998) 6-15 | null | null | cs.PF | null | We present a hierarchical simulation approach for the dependability analysis
and evaluation of a highly available commercial cache-based RAID storage
system. The archi-tecture is complex and includes several layers of
overlap-ping error detection and recovery mechanisms. Three ab-straction levels
have been developed to model the cache architecture, cache operations, and
error detection and recovery mechanism. The impact of faults and errors
oc-curring in the cache and in the disks is analyzed at each level of the
hierarchy. A simulation submodel is associated with each abstraction level. The
models have been devel-oped using DEPEND, a simulation-based environment for
system-level dependability analysis, which provides facili-ties to inject
faults into a functional behavior model, to simulate error detection and
recovery mechanisms, and to evaluate quantitative measures. Several fault
models are defined for each submodel to simulate cache component failures, disk
failures, transmission errors, and data errors in the cache memory and in the
disks. Some of the parame-ters characterizing fault injection in a given
submodel cor-respond to probabilities evaluated from the simulation of the
lower-level submodel. Based on the proposed method-ology, we evaluate and
analyze 1) the system behavior un-der a real workload and high error rate
(focusing on error bursts), 2) the coverage of the error detection mechanisms
implemented in the system and the error latency distribu-tions, and 3) the
accumulation of errors in the cache and in the disks.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 11:46:49 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Kaaniche",
"Mohamed",
"",
"LAAS"
],
[
"Romano",
"Luigi",
"",
"UIUC"
],
[
"Kalbarczyk",
"Zbigniew",
"",
"UIUC"
],
[
"Iyer",
"Ravishankar",
"",
"UIUC"
],
[
"Karcich",
"Rick",
"",
"STORAGETEK"
]
] | [
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] |
704.088 | Qiuping A. Wang | Q. A. Wang (ISMANS), F. Tsobnang (ISMANS), S. Bangoup (ISMANS), F.
Dzangue (ISMANS), A. Jeatsa (ISMANS), A. Le M\'ehaut\'e (ISMANS) | Stochastic action principle and maximum entropy | This work is a further development of the idea proposed in the paper
cond-mat/0407515, 15 pages | Chaos, Solitons and Fractals, 40(2009)2550-2556 | 10.1016/j.chaos.2007.10.047 | null | cond-mat.stat-mech | null | A stochastic action principle for stochastic dynamics is revisited. We
present first numerical diffusion experiments showing that the diffusion path
probability depend exponentially on average Lagrangian action. This result is
then used to derive an uncertainty measure defined in a way mimicking the heat
or entropy in the first law of thermodynamics. It is shown that the path
uncertainty (or path entropy) can be measured by the Shannon information and
that the maximum entropy principle and the least action principle of classical
mechanics can be unified into a concise form. It is argued that this action
principle, hence the maximum entropy principle, is simply a consequence of the
mechanical equilibrium condition extended to the case of stochastic dynamics.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 11:53:21 GMT"
}
] | "2020-11-25T00:00:00" | [
[
"Wang",
"Q. A.",
"",
"ISMANS"
],
[
"Tsobnang",
"F.",
"",
"ISMANS"
],
[
"Bangoup",
"S.",
"",
"ISMANS"
],
[
"Dzangue",
"F.",
"",
"ISMANS"
],
[
"Jeatsa",
"A.",
"",
"ISMANS"
],
[
"Méhauté",
"A. Le",
"",
"ISMANS"
]
] | [
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704.0881 | Jounghun Lee | Jounghun Lee, Daeseong Park (Seoul Nat'l Univ.) | Constraining the Dark Energy Equation of State with Cosmic Voids | ApJL in press, growth factor corrected, parameter degeneracy
calculated | Astrophys.J.696:L10-L12,2009 | 10.1088/0004-637X/696/1/L10 | null | astro-ph | http://arxiv.org/licenses/nonexclusive-distrib/1.0/ | Our universe is observed to be accelerating due to the dominant dark energy
with negative pressure. The dark energy equation of state (w) holds a key to
understanding the ultimate fate of the universe. The cosmic voids behave like
bubbles in the universe so that their shapes must be quite sensitive to the
background cosmology. Assuming a flat universe and using the priors on the
matter density parameter (Omega_m) and the dimensionless Hubble parameter (h),
we demonstrate analytically that the ellipticity evolution of cosmic voids may
be a sensitive probe of the dark energy equation of state. We also discuss the
parameter degeneracy between w and Omega_m.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 11:53:57 GMT"
},
{
"version": "v2",
"created": "Fri, 13 Mar 2009 17:47:40 GMT"
}
] | "2011-02-11T00:00:00" | [
[
"Lee",
"Jounghun",
"",
"Seoul Nat'l Univ."
],
[
"Park",
"Daeseong",
"",
"Seoul Nat'l Univ."
]
] | [
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704.0882 | Matts Roos | Matts Roos | A Dark Energy model combining DGP gravity and Chaplygin gas | 3 pages, 1 figure | null | null | null | astro-ph | null | The expansion of the Universe is accelerating, as testified by observations
of supernovae of type Ia as a function of redshift. Explanations are of two
types: modifications of Einstein gravity or new forms of energy, coined dark
energy.The accelerated expansion is explained here by a combination of
Dvali-Gabadadze-Porrati (DGP) model gravity and Chaplygin gas dark energy. Both
models are characterized by a length scale L which may be the same. The
continuity equation for the combined model is derived in flat geometry, and
solved by numerical methods. The solution is shown to have the expected
properties: at very small scales (a<<L) the energy density behaves as
pressureless dust, at very large scales (a>>L) as a cosmological constant. The
modifications to the DGP model and the Chaplygin gas model occur for values of
a L. The results show an increase in the present dark energy density relative
to the plain DGP model.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 12:00:14 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Roos",
"Matts",
""
]
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] |
704.0883 | Yutaka Hosotani | Yutaka Hosotani | Gauge-Higgs Unification and LHC/ILC | 16 pages. Proceeding for SCGT2006 (Nagoya, Nov. 2006) | null | 10.1142/9789812790750_0038 | OU-HET 579/2007 | hep-ph | null | In the gauge-Higgs unification scenario the 4D Higgs field is identified with
the zero mode of the extra-dimensional component of gauge potentials. The mass
of the Higgs particle in the unification in the Randall-Sundrum warped
spacetime is predicted to be in the range 100 GeV - 300 GeV. The WWZ gauge
couplings remains almost universal as in the standard model, but substantial
deviation results for the Higgs couplings. The WWH and ZZH couplings are
suppressed by a factor \cos \theta_H from the values in the standard model,
where \theta_H is the Yang-Mills AB phase along the fifth dimension. These can
be tested at LHC and ILC.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 12:50:53 GMT"
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] | "2017-08-23T00:00:00" | [
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704.0884 | Viet-Anh Nguyen | Peter Pflug and Viet-Anh Nguyen | Extension theorems of Sakai type for separately holomorphic and
meromorphic functions | null | Ann. Polon. Math. 82 (2003), no. 2, 171--187 | null | null | math.CV | null | We first exhibit counterexamples to some open questions related to a theorem
of Sakai.
Then we establish an extension theorem of Sakai type for separately
holomorphic/meromorphic functions.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 13:02:19 GMT"
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] | "2007-05-23T00:00:00" | [
[
"Pflug",
"Peter",
""
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[
"Nguyen",
"Viet-Anh",
""
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704.0885 | Jan Pachl | Jan Pachl | Uniform measures and countably additive measures | LaTeX; 7 pages | null | null | null | math.FA math.GN | null | Uniform measures are defined as the functionals on the space of bounded
uniformly continuous functions that are continuous on bounded uniformly
equicontinuous sets. If every cardinal has measure zero then every countably
additive measure is a uniform measure. The functionals sequentially continuous
on bounded uniformly equicontinuous sets are exactly uniform measures on the
separable modification of the underlying uniform space.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 13:10:30 GMT"
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] | "2007-05-23T00:00:00" | [
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] |
704.0886 | Peter Jung | Peter Jung and Achim Rosch | Lower bounds for the conductivities of correlated quantum systems | Title changed; 9 pages, 2 figures | Phys. Rev. B 75, 245104 (2007) | 10.1103/PhysRevB.75.245104 | null | cond-mat.str-el | null | We show how one can obtain a lower bound for the electrical, spin or heat
conductivity of correlated quantum systems described by Hamiltonians of the
form H = H0 + g H1. Here H0 is an interacting Hamiltonian characterized by
conservation laws which lead to an infinite conductivity for g=0. The small
perturbation g H1, however, renders the conductivity finite at finite
temperatures. For example, H0 could be a continuum field theory, where momentum
is conserved, or an integrable one-dimensional model while H1 might describe
the effects of weak disorder. In the limit g to 0, we derive lower bounds for
the relevant conductivities and show how they can be improved systematically
using the memory matrix formalism. Furthermore, we discuss various applications
and investigate under what conditions our lower bound may become exact.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 13:32:51 GMT"
},
{
"version": "v2",
"created": "Wed, 20 Jun 2007 16:04:41 GMT"
}
] | "2007-06-20T00:00:00" | [
[
"Jung",
"Peter",
""
],
[
"Rosch",
"Achim",
""
]
] | [
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] |
704.0887 | Oleg Usatenko | S. S. Apostolov, Z. A. Mayzelis, O. V. Usatenko, V. A. Yampol'skii | Non-extensive thermodynamics of 1D systems with long-range interaction | 5 pages, 2 figures | null | null | null | physics.data-an physics.gen-ph | null | A new approach to non-extensive thermodynamical systems with non-additive
energy and entropy is proposed. The main idea of the paper is based on the
statistical matching of the thermodynamical systems with the additive
multi-step Markov chains. This general approach is applied to the Ising spin
chain with long-range interaction between its elements. The asymptotical
expressions for the energy and entropy of the system are derived for the
limiting case of weak interaction. These thermodynamical quantities are found
to be non-proportional to the length of the system (number of its particle).
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 13:37:45 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Apostolov",
"S. S.",
""
],
[
"Mayzelis",
"Z. A.",
""
],
[
"Usatenko",
"O. V.",
""
],
[
"Yampol'skii",
"V. A.",
""
]
] | [
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] |
704.0888 | Claude Berthier | S. Kramer (LCMI), R. Stern, M. Horvatic (LCMI), C. Berthier (LCMI), T.
Kimura (LANL), I.R. Fisher | NMR evidence for a strong modulation of the Bose-Einstein Condensate in
BaCuSi$_2$O$_6$ | null | Physical Review B 76, 10 (2007) 100406(R) | 10.1103/PhysRevB.76.100406 | null | cond-mat.str-el | null | We present a $^{63,65}$Cu and $^{29}$Si NMR study of the quasi-2D coupled
spin 1/2 dimer compound BaCuSi$_2$O$_6$ in the magnetic field range 13-26 T and
at temperatures as low as 50 mK. NMR data in the gapped phase reveal that below
90 K different intra-dimer exchange couplings and different gaps
($\Delta_{\rm{B}}/\Delta_{\rm{A}}$ = 1.16) exist in every second plane along
the c-axis, in addition to a planar incommensurate (IC) modulation. $^{29}$Si
spectra in the field induced magnetic ordered phase reveal that close to the
quantum critical point at $H_{\rm{c1}}$ = 23.35 T the average boson density
$\bar{n}$ of the Bose-Einstein condensate is strongly modulated along the
c-axis with a density ratio for every second plane
$\bar{n}_{\rm{A}}/\bar{n}_{\rm{B}} \simeq 5$. An IC modulation of the local
density is also present in each plane. This adds new constraints for the
understanding of the 2D value $\phi$ = 1 of the critical exponent describing
the phase boundary.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 13:49:04 GMT"
}
] | "2008-02-11T00:00:00" | [
[
"Kramer",
"S.",
"",
"LCMI"
],
[
"Stern",
"R.",
"",
"LCMI"
],
[
"Horvatic",
"M.",
"",
"LCMI"
],
[
"Berthier",
"C.",
"",
"LCMI"
],
[
"Kimura",
"T.",
"",
"LANL"
],
[
"Fisher",
"I. R.",
""
]
] | [
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] |
704.0889 | Anthony van Raan | Anthony F. J. van Raan | Bibliometric statistical properties of the 100 largest European
universities: prevalent scaling rules in the science system | 26 pages, 33 figures, 3 tables. submitted to the Journal of the
American Society for information Science and Technology | null | null | null | physics.data-an physics.soc-ph | null | For the 100 largest European universities we studied the statistical
properties of bibliometric indicators related to research performance, field
citation density and journal impact. We find a size-dependent cumulative
advantage for the impact of universities in terms of total number of citations.
In previous work a similar scaling rule was found at the level of research
groups. Therefore we conjecture that this scaling rule is a prevalent property
of the science system. We observe that lower performance universities have a
larger size-dependent cumulative advantage for receiving citations than
top-performance universities. We also find that for the lower-performance
universities the fraction of not-cited publications decreases considerably with
size. Generally, the higher the average journal impact of the publications of a
university, the lower the number of not-cited publications. We find that the
average research performance does not dilute with size. Large top-performance
universities succeed in keeping a high performance over a broad range of
activities. This most probably is an indication of their scientific attractive
power. Next we find that particularly for the lower-performance universities
the field citation density provides a strong cumulative advantage in citations
per publication. The relation between number of citations and field citation
density found in this study can be considered as a second basic scaling rule of
the science system. Top-performance universities publish in journals with
significantly higher journal impact as compared to the lower performance
universities. We find a significant decrease of the fraction of self-citations
with increasing research performance, average field citation density, and
average journal impact.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 14:13:34 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"van Raan",
"Anthony F. J.",
""
]
] | [
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704.089 | Salvatore Orlando | S. Orlando, F. Bocchino, F. Reale, G. Peres, O. Petruk | On the Origin of Asymmetries in Bilateral Supernova Remnants | 14 pages, 8 Figures; paper accepted for publication in A&A; the paper
with high-resolution figures can be downloaded at
http://www.astropa.unipa.it/~orlando/PAPERS/sorlando_6045.pdf | null | 10.1051/0004-6361:20066045 | null | astro-ph | null | AIMS: We investigate whether the morphology of bilateral supernova remnants
(BSNRs) observed in the radio band is determined mainly either by a non-uniform
interstellar medium (ISM) or by a non-uniform ambient magnetic field.
METHODS: We perform 3-D MHD simulations of a spherical SNR shock propagating
through a magnetized ISM. Two cases of shock propagation are considered: 1)
through a gradient of ambient density with a uniform ambient magnetic field; 2)
through a homogeneous medium with a gradient of ambient magnetic field
strength. From the simulations, we synthesize the synchrotron radio emission,
making different assumptions about the details of acceleration and injection of
relativistic electrons.
RESULTS: We find that asymmetric BSNRs are produced if the line-of-sight is
not aligned with the gradient of ambient plasma density or with the gradient of
ambient magnetic field strength. We derive useful parameters to quantify the
degree of asymmetry of the remnants that may provide a powerful diagnostic of
the microphysics of strong shock waves through the comparison between models
and observations.
CONCLUSIONS: BSNRs with two radio limbs of different brightness can be
explained if a gradient of ambient density or, most likely, of ambient magnetic
field strength is perpendicular to the radio limbs. BSNRs with converging
similar radio arcs can be explained if the gradient runs between the two arcs.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 14:13:38 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Orlando",
"S.",
""
],
[
"Bocchino",
"F.",
""
],
[
"Reale",
"F.",
""
],
[
"Peres",
"G.",
""
],
[
"Petruk",
"O.",
""
]
] | [
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-0.0403081812,
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] |
704.0891 | Michel Cribier | M. Cribier (APC) | Reactor Monitoring with Neutrinos | 5 pages - XXII International Conference On Neutrino Physics And
Astrophysics (Neutrino 2006) | XXII International Conference On Neutrino Physics And Astrophysics
(Neutrino 2006), Santa Fe, New Mexico : \'Etats-Unis (2006) | 10.1016/j.nuclphysbps.2011.03.094 | APC-123/conf | nucl-ex | null | The fundamental knowledge on neutrinos acquired in the recent years open the
possibility of applied neutrino physics. Among it the automatic and non
intrusive monitoring of nuclear reactor by its antineutrino signal could be
very valuable to IAEA in charge of the control of nuclear power plants. Several
efforts worldwide have already started.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 14:17:14 GMT"
}
] | "2012-10-09T00:00:00" | [
[
"Cribier",
"M.",
"",
"APC"
]
] | [
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704.0892 | Xingang Wang Dr | Xingang Wang, Meng Zhan, Ghuguang Guan, and Choy Heng Lai | Nonstationary pattern in unsynchronizable complex networks | 11 pages, 9 figures, preprints. Comments and suggestions are welcome | null | null | null | nlin.CD | null | Pattern formation and evolution in unsynchronizable complex networks are
investigated. Due to the asymmetric topology, the synchronous patterns formed
in complex networks are irregular and nonstationary. For coupling strength
immediately out of the synchronizable region, the typical phenomenon is the
on-off intermittency of the system dynamics. The patterns appeared in this
process are signatured by the coexistence of a giant cluster, which comprises
most of the nodes, and a few number of small clusters. The pattern evolution is
characterized by the giant cluster irregularly absorbs or emits the small
clusters. As the coupling strength leaves away from the synchronization
bifurcation point, the giant cluster is gradually dissolved into a number of
small clusters, and the system dynamics is characterized by the integration and
separation of the small clusters. Dynamical mechanisms and statistical
properties of the nonstationary pattern evolution are analyzed and conducted,
and some scalings are newly revealed. Remarkably, it is found that the few
active nodes, which escape from the giant cluster with a high frequency, are
independent of the coupling strength while are sensitive to the bifurcation
types. We hope our findings about nonstationary pattern could give additional
understandings to the dynamics of complex systems and have implications to some
real problems where systems maintain their normal functions only in the
unsynchronizable state.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 14:19:59 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Wang",
"Xingang",
""
],
[
"Zhan",
"Meng",
""
],
[
"Guan",
"Ghuguang",
""
],
[
"Lai",
"Choy Heng",
""
]
] | [
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] |
704.0893 | Antonio Khoury | C.E.R. Souza, J.A.O. Huguenin, P. Milman, and A.Z. Khoury | Topological phase for spin-orbit transformations on a laser beam | 4 pages, 4 figures | Phys. Rev. Lett. 99, 160401 (2007) | 10.1103/PhysRevLett.99.160401 | null | quant-ph | null | We investigate the topological phase associated with the double connectedness
of the SO(3) representation in terms of maximally entangled states. An
experimental demonstration is provided in the context of polarization and
spatial mode transformations of a laser beam carrying orbital angular momentum.
The topological phase is evidenced through interferometric measurements and a
quantitative relationship between the concurrence and the fringes visibility is
derived. Both the quantum and the classical regimes were investigated.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 14:27:51 GMT"
}
] | "2011-07-08T00:00:00" | [
[
"Souza",
"C. E. R.",
""
],
[
"Huguenin",
"J. A. O.",
""
],
[
"Milman",
"P.",
""
],
[
"Khoury",
"A. Z.",
""
]
] | [
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] |
704.0894 | John Subasavage Jr. | John P. Subasavage (1), Todd J. Henry (1), P. Bergeron (2), P. Dufour
(2), Nigel C. Hambly (3), Thomas D. Beaulieu (1) ((1) Georgia State
University, (2) University of Montreal, (3) University of Edinburgh Royal
Observatory) | The Solar Neighborhood. XIX. Discovery and Characterization of 33 New
Nearby White Dwarf Systems | 33 pages, 10 figures, accepted for publication in the Astronomical
Journal | Astron.J.134:252-261,2007 | 10.1086/518739 | null | astro-ph | null | We present spectra for 33 previously unclassified white dwarf systems
brighter than V = 17 primarily in the southern hemisphere. Of these new
systems, 26 are DA, 4 are DC, 2 are DZ, and 1 is DQ. We suspect three of these
systems are unresolved double degenerates. We obtained VRI photometry for these
33 objects as well as for 23 known white dwarf systems without trigonometric
parallaxes, also primarily in the southern hemisphere. For the 56 objects, we
converted the photometry values to fluxes and fit them to a spectral energy
distribution using the spectroscopy to determine which model to use (i.e. pure
hydrogen, pure helium, or metal-rich helium), resulting in estimates of
effective temperature and distance. Eight of the new and 12 known systems are
estimated to be within the NStars and Catalogue of Nearby Stars (CNS) horizons
of 25 pc, constituting a potential 18% increase in the nearby white dwarf
sample. Trigonometric parallax determinations are underway via CTIOPI for these
20 systems.
One of the DCs is cool so that it displays absorption in the near infrared.
Using the distance determined via trigonometric parallax, we are able to
constrain the model-dependent physical parameters and find that this object is
most likely a mixed H/He atmosphere white dwarf similar to other cool white
dwarfs identified in recent years with significant absorption in the infrared
due to collision-induced absorptions by molecular hydrogen.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 15:08:34 GMT"
}
] | "2009-09-29T00:00:00" | [
[
"Subasavage",
"John P.",
""
],
[
"Henry",
"Todd J.",
""
],
[
"Bergeron",
"P.",
""
],
[
"Dufour",
"P.",
""
],
[
"Hambly",
"Nigel C.",
""
],
[
"Beaulieu",
"Thomas D.",
""
]
] | [
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704.0895 | Perrin Nicolas | Nicolas Perrin | Gorenstein locus of minuscule Schubert varieties | 12 pages | null | null | null | math.AG math.CO | null | In this article, we describe explicitely the Gorenstein locus of all
minuscule Schubert varieties. This proves a special case of a conjecture of A.
Woo and A. Yong (see math.AG/0603273) on the Gorenstein locus of Schubert
varieties.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 15:00:40 GMT"
}
] | "2007-05-23T00:00:00" | [
[
"Perrin",
"Nicolas",
""
]
] | [
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704.0896 | Yurij Holovatch | M. Dudka, R. Folk, Yu. Holovatch, G. Moser | Model C critical dynamics of random anisotropy magnets | 8 figures, style files included | J. Phys. A: Math. Gen., vol. 40 (2007) 8247-8264 | 10.1088/1751-8113/40/29/004 | null | cond-mat.dis-nn cond-mat.stat-mech | null | We study the relaxational critical dynamics of the three-dimensional random
anisotropy magnets with the non-conserved n-component order parameter coupled
to a conserved scalar density. In the random anisotropy magnets the structural
disorder is present in a form of local quenched anisotropy axes of random
orientation. When the anisotropy axes are randomly distributed along the edges
of the n-dimensional hypercube, asymptotical dynamical critical properties
coincide with those of the random-site Ising model. However structural disorder
gives rise to considerable effects for non-asymptotic critical dynamics. We
investigate this phenomenon by a field-theoretical renormalization group
analysis in the two-loop order. We study critical slowing down and obtain
quantitative estimates for the effective and asymptotic critical exponents of
the order parameter and scalar density. The results predict complex scenarios
for the effective critical exponent approaching an asymptotic regime.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 15:08:06 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Dudka",
"M.",
""
],
[
"Folk",
"R.",
""
],
[
"Holovatch",
"Yu.",
""
],
[
"Moser",
"G.",
""
]
] | [
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] |
704.0897 | Viet-Anh Nguyen | Viet-Anh Nguyen | A unified approach to the theory of separately holomorphic mappings | 54 pages, preprint of the ICTP, Trieste, Italy (2007). I have added
some minor explanations, corrections and changes | null | null | null | math.CV | null | We extend the theory of separately holomorphic mappings between complex
analytic spaces. Our method is based on Poletsky theory of discs, Rosay Theorem
on holomorphic discs and our recent joint-work with Pflug on cross theorems in
dimension 1. It also relies on our new technique of conformal mappings and a
generalization of Siciak's relative extremal function.
Our approach illustrates the unified character: ``From local informations to
global extensions". Moreover, it avoids systematically the use of the classical
method of doubly orthogonal bases of Bergman type.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 15:31:38 GMT"
},
{
"version": "v2",
"created": "Sun, 4 Nov 2007 22:48:08 GMT"
}
] | "2007-11-05T00:00:00" | [
[
"Nguyen",
"Viet-Anh",
""
]
] | [
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] |
704.0898 | Xavier Bekaert | Xavier Bekaert | Higher spin algebras as higher symmetries | 14 pages, expanded version of the lectures presented at the ``5th
international school and workshop on QFT & Hamiltonian systems''
(Calimanesti, May 2006); v2: minor corrections performed, comments added and
refs updated | null | null | null | hep-th | null | The exhaustive study of the rigid symmetries of arbitrary free field theories
is motivated, along several lines, as a preliminary step in the completion of
the higher-spin interaction problem in full generality. Some results for the
simplest example (a scalar field) are reviewed and commented along these lines.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 15:59:02 GMT"
},
{
"version": "v2",
"created": "Thu, 23 Aug 2007 09:56:23 GMT"
}
] | "2007-08-23T00:00:00" | [
[
"Bekaert",
"Xavier",
""
]
] | [
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704.0899 | Van Dixon | W. V. Dixon (1), D. J. Sahnow (1), P. E. Barrett (2 and 3), T. Civeit
(1 and 4), J. Dupuis (1 and 5), A. W. Fullerton (1 and 6), B. Godard (1 and
7), J. C. Hsu (2 and 8), M. E. Kaiser (1), J. W. Kruk (1), S. Lacour (1 and
9), D. J. Lindler (10), D. Massa (11), R. D. Robinson (1 and 8), M. L.
Romelfanger (1), P. Sonnentrucker (1) ((1) Johns Hopkins University, (2)
Space Telescope Science Institute, (3) U.S. Naval Observatory, (4) Centre
National d'Etudes Spatiales, (5) Canadian Space Agency, (6) University of
Victoria, (7) Institut d'Astrophysique de Paris, (8) Retired, (9) Sydney
University, (10) Sigma Space Corporation, (11) SGT, Inc.) | CalFUSE v3: A Data-Reduction Pipeline for the Far Ultraviolet
Spectroscopic Explorer | To appear in PASP; 29 pages, 13 figures, uses aastex, emulateapj | null | 10.1086/518617 | null | astro-ph | null | Since its launch in 1999, the Far Ultraviolet Spectroscopic Explorer (FUSE)
has made over 4600 observations of some 2500 individual targets. The data are
reduced by the Principal Investigator team at the Johns Hopkins University and
archived at the Multimission Archive at Space Telescope (MAST). The
data-reduction software package, called CalFUSE, has evolved considerably over
the lifetime of the mission. The entire FUSE data set has recently been
reprocessed with CalFUSE v3.2, the latest version of this software. This paper
describes CalFUSE v3.2, the instrument calibrations upon which it is based, and
the format of the resulting calibrated data files.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 15:37:01 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Dixon",
"W. V.",
"",
"2 and 3"
],
[
"Sahnow",
"D. J.",
"",
"2 and 3"
],
[
"Barrett",
"P. E.",
"",
"2 and 3"
],
[
"Civeit",
"T.",
"",
"1 and 4"
],
[
"Dupuis",
"J.",
"",
"1 and 5"
],
[
"Fullerton",
"A. W.",
"",
"1 and 6"
],
[
"Godard",
"B.",
"",
"1 and\n 7"
],
[
"Hsu",
"J. C.",
"",
"2 and 8"
],
[
"Kaiser",
"M. E.",
"",
"1 and\n 9"
],
[
"Kruk",
"J. W.",
"",
"1 and\n 9"
],
[
"Lacour",
"S.",
"",
"1 and\n 9"
],
[
"Lindler",
"D. J.",
"",
"1 and 8"
],
[
"Massa",
"D.",
"",
"1 and 8"
],
[
"Robinson",
"R. D.",
"",
"1 and 8"
],
[
"Romelfanger",
"M. L.",
""
],
[
"Sonnentrucker",
"P.",
""
]
] | [
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704.09 | Benoit Doucot | Benoit Doucot and Lev B. Ioffe | Voltage-Current curves for small Josephson junction arrays | 12 pages, 4 figures | null | 10.1103/PhysRevB.76.214507 | null | cond-mat.supr-con cond-mat.mes-hall | null | We compute the current voltage characteristic of a chain of identical
Josephson circuits characterized by a large ratio of Josephson to charging
energy that are envisioned as the implementation of topologically protected
qubits. We show that in the limit of small coupling to the environment it
exhibits a non-monotonous behavior with a maximum voltage followed by a
parametrically large region where $V\propto 1/I$. We argue that its
experimental measurement provides a direct probe of the amplitude of the
quantum transitions in constituting Josephson circuits and thus allows their
full characterization.
| [
{
"version": "v1",
"created": "Fri, 6 Apr 2007 17:10:23 GMT"
}
] | "2009-11-13T00:00:00" | [
[
"Doucot",
"Benoit",
""
],
[
"Ioffe",
"Lev B.",
""
]
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