55,237 research outputs found
Slices of the Kerr ergosurface
The intrinsic geometry of the Kerr ergosurface on constant Boyer-Lindquist
(BL), Kerr, and Doran time slices is characterized. Unlike the BL slice, which
had been previously studied, the other slices (i) do not have conical
singularities at the poles (except the Doran slice in the extremal limit), (ii)
have finite polar circumference in the extremal limit, and (iii) for
sufficiently large spin parameter fail to be isometrically embeddable as a
surface of revolution above some latitude. The Doran slice develops an
embeddable polar cap for spin parameters greater than about 0.96.Comment: 13 pages, 6 figures; v.2: minor editing for clarification, references
added, typos fixed, version published in Classical and Quantum Gravit
Searching for sub-millisecond pulsars from highly polarized radio sources
Pulsars are among the most highly polarized sources in the universe. The NVSS
has catalogued 2 million radio sources with linear polarization measurements,
from which we have selected 253 sources, with polarization percentage greater
than 25%, as targets for pulsar searches. We believe that such a sample is not
biased by selection effects against ultra-short spin or orbit periods. Using
the Parkes 64m telescope, we conducted searches with sample intervals of 0.05
ms and 0.08 ms, sensitive to submillisecond pulsars. Unfortunately we did not
find any new pulsars.Comment: 2 pages 1 figure. To appear in "Young Neutron Stars and Their
Environments" (IAU Symposium 218, ASP Conference Proceedings), eds F. Camilo
and B. M. Gaensle
Imaginary-time formulation of steady-state nonequilibrium: application to strongly correlated transport
We extend the imaginary-time formulation of the equilibrium quantum many-body
theory to steady-state nonequilibrium with an application to strongly
correlated transport. By introducing Matsubara voltage, we keep the finite
chemical potential shifts in the Fermi-Dirac function, in agreement with the
Keldysh formulation. The formulation is applied to strongly correlated
transport in the Kondo regime using the quantum Monte Carlo method.Comment: 5 pages 3 figure
Skyrmion Generation by Current
Skyrmions, once a hypothesized field-theoretical object believed to describe
the nature of elementary particles, became common sightings in recent years
among several non-centrosymmetric metallic ferromagnets. For more practical
applications of Skyrmionic matter as carriers of information, thus realizing
the prospect of "Skyrmionics", it is necessary to have the means to create and
manipulate Skyrmions individually. We show through extensive simulation of the
Landau-Lifshitz-Gilbert equation that a circulating current imparted to the
metallic chiral ferromagnetic system can create isolated Skyrmionic spin
texture without the aid of external magnetic field.Comment: 8 pages, 5 figures, submitted to PR
Studying High Energy Final State Interactions by N/D Method
We discuss the final state interaction effects at high energies via a
multi-channel N/D method. We find that the 2 by 2 charge--exchange final state
interactions typically contribute an enhancement factor of a few times
in the meson decay amplitudes, both for the real and the
imaginary part. We also make some discussions on the elastic rescattering
effects.Comment: 10 pages, revte
Subdwarf B Stars from the ESO Supernova Ia Progenitor Survey -- Observation versus Theory
Original paper can be found at: http://www.astrosociety.org/pubs/cs/328.html--Copyright Astronomical Society of the PacificWe present the analysis of a high-quality sample of optical spectra for 76 sdB stars from the ESO Supernova Ia Progenitor Survey. Effective temperature, surface gravity, and photospheric helium abundance were derived from line profile fits. We demonstrate that our subsample of 52 single-lined sdB stars is a useful tool to compare observation and theory. The predictions of population synthesis models for close binary evolution are compared to our data. We show that the simulations cover the observed parameter range of sdBs, but fail to reproduce the observed distribution in detail
An improved solar wind electron-density model for pulsar timing
Variations in the solar wind density introduce variable delays into pulsar
timing observations. Current pulsar timing analysis programs only implement
simple models of the solar wind, which not only limit the timing accuracy, but
can also affect measurements of pulsar rotational, astrometric and orbital
parameters. We describe a new model of the solar wind electron density content
which uses observations from the Wilcox Solar Observatory of the solar magnetic
field. We have implemented this model into the tempo2 pulsar timing package. We
show that this model is more accurate than previous models and that these
corrections are necessary for high precision pulsar timing applications.Comment: Accepted by ApJ, 13 pages, 4 figure
Quantum State Discrimination with General Figures of Merit
We solve the problem of quantum state discrimination with "general
(symmetric) figures of merit" for an even number of symmetric quantum bits with
use of the no-signaling principle. It turns out that conditional probability
has the same form for any figure of merit. Optimal measurement and
corresponding conditional probability are the same for any monotonous figure of
merit.Comment: 5 pages, 2 figure
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