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astro-ph2003

Exploring the Nature of Weak Chandra Sources near the Galactic Centre

R. M. Bandyopadhyay, K. M. Blundell, Ph. Podsiadlowski +5

We present early results from the first IR imaging of the weak X-ray sources discovered in a recent Chandra survey towards the Galactic Centre. From our VLT observations we will id…

astro-ph2003★ 59 cited

Nucleosynthesis in The Oxygen-Rich Supernova Remnant G292.0+1.8 from Chandra X-Ray Spectroscopy

Sangwook Park, John P. Hughes, Patrick O. Slane +4

We continue our analysis of the Galactic oxygen-rich supernova remnant (SNR) G292.0+1.8, which was observed with the {\it Chandra X-ray Observatory}. The high angular resolution {\…

gr-qc2003★ 2 cited

Loop Quantum Cosmology and Boundary Proposals

Martin Bojowald, Kevin Vandersloot

For many years, the most active area of quantum cosmology has been the issue of choosing boundary conditions for the wave function of a universe. Recently, loop quantum cosmology,…

cond-mat.stat-mech2003★ 5 cited

Searching for self-similarity in switching time and turbulent cascades in ion transport through a biochannel. A time delay asymmetry

M. Ausloos, K. Ivanova, Z. Siwy

The process of ion transport through a locust potassium channel is described by means of the Fokker-Planck equation (FPE). The deterministic and stochastic components of the proces…

astro-ph2003★ 118 cited

Observations and Theoretical Implications of the Large Separation Lensed Quasar SDSS J1004+4112

M. Oguri, N. Inada, C. R. Keeton +25

We study the recently discovered gravitational lens SDSS J1004+4112, the first quasar lensed by a cluster of galaxies. It consists of four images with a maximum separation of 14.62…

math.CO2003★ 1 cited

On Non-Squashing Partitions

N. J. A. Sloane, James A. Sellers

A partition n = p_1 + p_2 + ... + p_k with 1 <= p_1 <= p_2 <= ... <= p_k is called non-squashing if p_1 + ... + p_j <= p_{j+1} for 1 <= j <= k-1. Hirschhorn and Sellers showed that…

math.CA2003

Ratio vectors of fourth degree polynomials

Alan Horwitz

Let p(x) be a polynomial of degree 4 with four distinct real roots r1<r2<r3<r4. Let x1<x2<x3 be the critical points of p, and define the ratios s_{k}=((x_{k}-r_{k})/(r_{k+1}-r_{k})…

astro-ph2003★ 93 cited

A Catalog of Compact Groups of Galaxies in the SDSS Commissioning Data

B. C. Lee, S. S. Allam, D. L. Tucker +20

Compact groups (CGs) of galaxies -- relatively poor groups of galaxies in which the typical separations between members is of the order of a galaxy diameter -- offer an exceptional…

hep-ex2003★ 14 cited

Isolated tau leptons in events with large missing transverse momentum at HERA

ZEUS collaboration

A search for events containing isolated tau leptons and large missing transverse momentum, not originating from the tau decay, has been performed with the ZEUS detector at the elec…

gr-qc2003★ 126 cited

Analysis of First LIGO Science Data for Stochastic Gravitational Waves

LIGO Scientific Collaboration, B. Abbott

We present the analysis of between 50 and 100 hrs of coincident interferometric strain data used to search for and establish an upper limit on a stochastic background of gravitatio…

astro-ph2003★ 17 cited

Search for Galaxy Clustering around a Quasar Pair at z=4.25 found in the Sloan Digital Sky Survey

Masataka Fukugita, Osamu Nakamura, Donald P. Schneider +2

We present an investigation of the environment (\approx 600 kpc radius) of a pair of luminous z=4.25 quasars, SDSS J1439-0034 A,B, separated by 33''. An analysis of high-quality Su…

astro-ph2003★ 20 cited

Spatial Variations of Galaxy Number Counts in the SDSS I.: Extinction, Large-Scale Structure and Photometric Homogeneity

Masataka Fukugita, Naoki Yasuda, Jon Brinkmann +5

We study the spatial variation of galaxy number counts using five band photometric images from the Sloan Digital Sky Survey. The spatial variation of this sample of 46 million gala…

astro-ph2003★ 63 cited

The H alpha Luminosity Function of Morphologically Classified Galaxies in the Sloan Digital Sky Survey

Osamu Nakamura, Masataka Fukugita, Jon Brinkmann +1

We present a study of the H line emission from a sample of 1482 optically-selected, morphologically-classified bright galaxies (median redshift of 0.05) derived from the Sloan D…

astro-ph2003★ 210 cited

A Gravitationally Lensed Quasar with Quadruple Images Separated by 14.62 Arcseconds

N. Inada, M. Oguri, B. Pindor +29

Gravitational lensing is a powerful tool for the study of the distribution of dark matter in the Universe. The cold-dark-matter model of the formation of large-scale structures pre…

astro-ph2003

Planetary Collisions: Electromagnetic Signals

Bing Zhang, Steinn Sigurdsson

We investigate the electromagnetic signals accompanied with planetary collisions and their event rate, and explore the possibility of directly detecting such events. A typical Eart…

math.NA2003★ 2 cited

AF embeddings and the numerical computation of spectra in irrational rotation algebras

Nathanial P. Brown

The spectral analysis of discretized one-dimensional Schrödinger operators is a very difficult problem which has been studied by numerous mathematicians. A natural problem at the i…

cond-mat.str-el2003★ 50 cited

Dynamical mean-field theory of Hubbard-Holstein model at half-filling: Zero temperature metal-insulator and insulator-insulator transitions

Gun Sang Jeon, Tae-Ho Park, Jung Hoon Han +2

We study the Hubbard-Holstein model, which includes both the electron-electron and electron-phonon interactions characterized by and , respectively, employing the dynamical…

astro-ph2003★ 156 cited

Quasi-universal Gaussian jets: a unified picture for gamma-ray bursts and X-ray flashes

Bing Zhang, Xinyu Dai, Nicole M. Lloyd-Ronning +1

An observed correlation Ep \propto (E_{iso})^{1/2} extending from Gamma-ray Bursts (GRBs) to X-ray flashes (XRFs) poses problems both for a power-law universal jet model where the…

astro-ph2003★ 44 cited

IZw1 observed with XMM-Newton: Low-energy spectral complexity, iron lines, and hard X-ray flares

L. C. Gallo, Th. Boller, W. N. Brandt +2

We present a 20 ks XMM-Newton observation of the prototypical Narrow-Line Seyfert 1 galaxy IZw1. The best-fit model to the data is a double blackbody plus a dominant power-law, on…

quant-ph2003★ 34 cited

Wigner quasi-probability distribution for the infinite square well: energy eigenstates and time-dependent wave packets

M. Belloni, M. A. Doncheski, R. W. Robinett

We calculate the Wigner quasi-probability distribution for position and momentum, P_W^(n)(x,p), for the energy eigenstates of the standard infinite well potential, using both x- an…

quant-ph2003★ 18 cited

Mimicking Time Evolution within a Quantum Ground State: Ground-State Quantum Computation, Cloning, and Teleportation

Ari Mizel

Ground-state quantum computers mimic quantum mechanical time evolution within the amplitudes of a time-independent quantum state. We explore the principles that constrain this mimi…

cond-mat2003★ 14 cited

Surface effects on nanowire transport: numerical investigation using the Boltzmann equation

Venkat S. Sundaram, Ari Mizel

A direct numerical solution of the steady-state Boltzmann equation in a cylindrical geometry is reported. Finite-size effects are investigated in large semiconducting nanowires usi…

astro-ph2003★ 47 cited

SDSS J115517.35+634622.0: A Newly Discovered Gravitationally Lensed Quasar

Bart Pindor, Daniel J. Eisenstein, Naohisa Inada +12

We report the discovery of SDSSJ115517.35+634622.0, a previously unknown gravitationally lensed quasar. The lens system exhibits two images of a quasar, with an image se…

nucl-ex2003★ 95 cited

Azimuthally sensitive Hanbury Brown-Twiss interferometry in Au+Au collisions at sqrt(s_{NN}) = 200 GeV

STAR Collaboration

We present the results of a systematic study of the shape of the pion distribution in coordinate space at freeze-out in Au+Au collisions at RHIC using two-pion Hanbury Brown-Twiss…