65,067 research outputs found
Electron scattering and transport in liquid argon
The transport of excess electrons in liquid argon driven out of equilibrium
by an applied electric field is revisited using a multi-term solution of
Boltzmann's equation together with ab initio liquid phase cross-sections
calculated using the Dirac-Fock scattering equations. The calculation of liquid
phase cross-sections extends previous treatments to consider multipole
polarisabilities and a non-local treatment of exchange while the accuracy of
the electron-argon potential is validated through comparison of the calculated
gas phase cross-section with experiment. The results presented highlight the
inadequacy of local treatments of exchange that are commonly used in liquid and
cluster phase cross-section calculations. The multi-term Boltzmann equation
framework accounting for coherent scattering enables the inclusion of the full
anisotropy in the differential cross-section arising from the interaction and
the structure factor, without an a priori assumption of quasi-isotropy in the
velocity distribution function. The model, which contains no free parameters
and accounts for both coherent scattering and liquid phase screening effects,
was found to reproduce well the experimental drift velocities and
characteristic energies.Comment: 32 pages, 16 figures; minor corrections, added 1 figur
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CCH <i>N</i> = 4-3 emission from dense interstellar clouds
The authors have searched for N = 4 - 3 rotational line emission from the ethynyl radical CCH, at 349 GHz toward a number of galactic molecular clouds. They have detected emission from ten giant molecular clouds and have derived CCH column densities on the order of 1014 - 1015cm-2. They find that CCH emission arises from dense gas, n(H2) ~ 104 - 105cm-3, but not from very dense material, n(H2) > 106cm-3, nor from hot gas such as the "hot core" region in Orion
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Near infrared spectroscopy of W51 IRS-2
Near-infrared spectra at 2.95-3.5 μm and 3.99-10 μm have been obtained towards W51 IRS-2 and its surroundings, in order to investigate the spatial variations in intensity of the 3.28 μm unidentified feature and the 4.05 μm Brackett-α line. The Br-α and 3.28 μm features occupy a broadly similar spatial zone, which is characterised by an unresolved core responsible for most of the emission, and an extended and considerably weaker halo. Grain properties required to excite the 4.28 microns line, the nature of the 3.28 μm emission, and its relation to the source structure are discussed
Satellite Galaxies and Fossil Groups in the Millennium Simulation
We use a semianalytic galaxy catalogue constructed from the Millennium
Simulation to study the satellites of isolated galaxies in the LCDM cosmogony.
This sample (~80,000$ bright primaries, surrounded by ~178,000 satellites)
allows the characterization, with minimal statistical uncertainty, of the
dynamical properties of satellite/primary galaxy systems in a LCDM universe. We
find that, overall, the satellite population traces the dark matter rather
well: its spatial distribution and kinematics may be approximated by an NFW
profile with a mildly anisotropic velocity distribution. Their spatial
distribution is also mildly anisotropic, with a well-defined ``anti-Holmberg''
effect that reflects the misalignment between the major axis and angular
momentum of the host halo. The isolation criteria for our primaries picks not
only galaxies in sparse environments, but also a number of primaries at the
centre of ''fossil'' groups. We find that the abundance and luminosity function
of these unusual systems are in reasonable agreement with the few available
observational constraints. We recover the expected L_{host} \sigma_{sat}^3
relation for LCDM models for truly-isolated primaries. Less strict primary
selection, however, leads to substantial modification of the scaling relation.
Our analysis also highlights a number of difficulties afflicting studies that
rely on blind stacking of satellite systems to constrain the mean halo mass of
the primary galaxies.Comment: 18 pages, 14 figures, MNRAS in press. Accepted version with minor
changes. Version with high resolution figures available at:
http://www.astro.uvic.ca/~lsales/SatPapers/SatPapers.htm
Linear Cosmological Structure Limits on Warm Dark Matter
I consider constraints from observations on a cutoff scale in clustering due
to free streaming of the dark matter in a warm dark matter cosmological model
with a cosmological constant. The limits are derived in the framework of a
sterile neutrino warm dark matter universe, but can be applied to gravitinos
and other models with small scale suppression in the linear matter power
spectrum. With freedom in all cosmological parameters including the free
streaming scale of the sterile neutrino dark matter, limits are derived using
observations of the fluctuations in the cosmic microwave background, the 3D
clustering of galaxies and 1D clustering of gas in the Lyman-alpha (Ly-alpha)
forest in the Sloan Digital Sky Survey (SDSS), as well as the Ly-alpha forest
in high-resolution spectroscopic observations. In the most conservative case,
using only the SDSS main-galaxy 3D power-spectrum shape, the limit is m_s >
0.11 keV; including the SDSS Ly-alpha forest, this limit improves to m_s > 1.7
keV. More stringent constraints may be placed from the inferred matter power
spectrum from high-resolution Ly-alpha forest observations, which has
significant systematic uncertainties; in this case, the limit improves to m_s >
3.0 keV (all at 95% CL).Comment: 6 pages, 4 figures; v2: matches PRD version, with note added
regarding astro-ph/060243
Linear Optical CNOT Gate in the Coincidence Basis
We describe the operation and tolerances of a non-deterministic, coincidence
basis, quantum CNOT gate for photonic qubits. It is constructed solely from
linear optical elements and requires only a two-photon source for its
demonstration.Comment: Submitted to Physical Review
Wilson line approach to gravity in the high energy limit
We examine the high energy (Regge) limit of gravitational scattering using a
Wilson line approach previously used in the context of non-Abelian gauge
theories. Our aim is to clarify the nature of the Reggeization of the graviton
and the interplay between this Reggeization and the so-called eikonal phase
which determines the spectrum of gravitational bound states. Furthermore, we
discuss finite corrections to this picture. Our results are of relevance to
various supergravity theories, and also help to clarify the relationship
between gauge and gravity theories.Comment: 33 pages, 5 figure
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A high resolution millimetre and submillimetre study of W3
The continuum bolometer receiver on the James Clerk Maxwell telescope has been used to map the dense core of the star formation region W3 with a spatial resolution of 15-20 arcsec. At 350 and 800 μm, the region appears as two principal peaks around the known IR sources IRS4 and IRS5, while at 1100 μm, a further peak is noted which is interpreted as being due to free-free emission around IRS2. Taking into account the free-free contribution to the intensity, the continuum dust emission from the region is found to be consistent with optically thin emission at all of the three wavelengths considered. Values for the dust optical depth, hydrogen column density, mass, and central density have been obtained for each of the main peaks
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