17,120 research outputs found
Singularity free cosmological solutions of Einstein-Maxwell equations
We report on a new two-parameter class of cosmological solutions to the
Einstein-Maxwell equations. The solutions have everywhere regular curvature
invariants. We prove that the solutions are geodesically complete and globally
hyperbolic.Comment: 8 pages,latex; v2 some typos correcte
Killing spinor space-times and constant-eigenvalue Killing tensors
A class of Petrov type D Killing spinor space-times is presented, having the
peculiar property that their conformal representants can only admit Killing
tensors with constant eigenvalues.Comment: 11 pages, submitted to CQ
A new form of the Kerr solution
A new form of the Kerr solution is presented. The solution involves a time
coordinate which represents the local proper time for free-falling observers on
a set of simple trajectories. Many physical phenomena are particularly clear
when related to this time coordinate. The chosen coordinates also ensure that
the solution is well behaved at the horizon. The solution is well suited to the
tetrad formalism and a convenient null tetrad is presented. The Dirac
Hamiltonian in a Kerr background is also given and, for one choice of tetrad,
it takes on a simple, Hermitian form.Comment: 8 pages, LaTeX, no figures. Corrected and improved version. To appear
in Phys. Rev.
Gravitating superconducting strings with timelike or spacelike currents
We construct gravitating superconducting string solutions of the U(1)_{local}
x U(1)_{global} model solving the coupled system of Einstein and matter field
equations numerically. We study the properties of these solutions in dependence
on the ratio between the symmetry breaking scale and the Planck mass. Using the
macroscopic stability conditions formulated by Carter, we observe that the
coupling to gravity allows for a new stable region that is not present in the
flat space-time limit. We match the asymptotic metric to the Kasner metric and
show that the relations between the Kasner coefficients and the energy per unit
length and tension suggested previously are well fulfilled for symmetry
breaking scale much smaller than the Planck mass. We also study the solutions
to the geodesic equation in this space-time. While geodesics in the exterior
space-time of standard cosmic strings are just straight lines, test particles
experience a force in a general Kasner space-time and as such bound orbits are
possible.Comment: 16 pages including 14 figure
Non-Leptonic Decays of B Mesons and Strong Coupling Constants
Non-leptonic decays of B mesons into two mesons or meson resonances are
studied on the basis of two versions of simple pole-dominance models involving
scalar, vector, pseudoscalar and axial-vector poles. The results are compared
with those obtained from the usual factorization model and used to obtain
information on strong coupling constants between B meson and one light or one
charmed meson, respectively. These coupling constants are compared to results
from various QCD sum rule calculations.Comment: Latex file 35 pages, including 3 figure
Is Context-aware Reasoning = Case-based Reasoning?
The purpose of this paper is to explore the similarities and differences and then argue for the potential synergies between two methodologies, namely Context-aware Reasoning and Case-based Reasoning, that are amongst the tools which can be used for intelligent environment (IE) system development. Through a case study supported by a review of the literature, we argue that context awareness and case based reasoning are not equal and are complementary methodologies to solve a domain specific problem, rather, the IE development paradigm must build a cooperation between these two approaches to overcome the individual drawbacks and to maximise the success of the IE systems
Electrovac -waves
New exact solutions of the Einstein-Maxwell field equations that describe
-waves are presented
Changes in Polarization Position Angle across the Eclipse in the Double Pulsar System
We investigate the changes in polarization position angle in radiation from
pulsar A around the eclipse in the Double Pulsar system PSR J0737-3039A/B at
the 20 cm and 50 cm wavelengths using the Parkes 64-m telescope. The changes
are ~2\sigma\ during and shortly after the eclipse at 20 cm but less
significant at 50 cm. We show that the changes in position angle during the
eclipse can be modelled by differential synchrotron absorption in the eclipse
regions. Position angle changes after the eclipse are interpreted as Faraday
rotation in the magnetotail of pulsar B. Implied charge densities are
consistent with the Goldreich-Julian density, suggesting that the particle
energies in the magnetotail are mildly relativistic.Comment: Accepted for publication in The Astrophysical Journal Letter
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