7,798 research outputs found
Wormholes, naked singularities and universes of ghost radiation
Both the static and homogeneous metrics describing the spherically symmetric
gravitational field of a crossflow of incoming and outgoing null dust streams
are generalized for the case of the two-component ghost radiation. Static
solutions represent either naked singularities or the wormholes recently found
by Hayward. The critical value of the parameter separating the two
possibilities is given. The wormhole is allowed to have positive mass. The
homogeneous solutions are open universes.Comment: 5 pages, 10 figures, minor changes to match the published versio
Gravitational radiation reaction in compact binary systems: Contribution of the quadrupole-monopole interaction
The radiation reaction in compact spinning binaries on eccentric orbits due
to the quadrupole-monopole interaction is studied. This contribution is of
second post-Newtonian order. As result of the precession of spins the magnitude
of the orbital angular momentum is not conserved. Therefore a proper
characterization of the perturbed radial motion is provided by the energy
and angular average . As powerful computing tools, the generalized
true and eccentric anomaly parametrizations are introduced. Then the secular
losses in energy and magnitude of orbital angular momentum together with the
secular evolution of the relative orientations of the orbital angular momentum
and spins are found for eccentric orbits by use of the residue theorem. The
circular orbit limit of the energy loss agrees with Poisson's earlier result.Comment: accepted for publication in Phys. Rev.
Brane-world cosmology with black strings
We consider the simplest scenario when black strings / cigars penetrate the
cosmological brane. As a result, the brane has a Swiss-cheese structure, with
Schwarzschild black holes immersed in a
Friedmann-Lema\^{\i}tre-Robertson-Walker brane. There is no dark radiation in
the model, the cosmological regions of the brane are characterized by a
cosmological constant and flat spatial sections. Regardless of the
value of , these brane-world universes forever expand and forever
decelerate. The totality of source terms in the modified Einstein equation sum
up to a dust, establishing a formal equivalence with the general relativistic
Einstein-Straus model. However in this brane-world scenario with black strings
the evolution of the cosmological fluid strongly depends on . For
it has positive energy density and negative pressure
and at late times it behaves as in the Einstein-Straus model. For (not too
high) positive values of the cosmological evolution begins with
positive and negative , but this is followed by an epoch with both
and positive. Eventually, becomes negative, while stays
positive. A similar evolution is present for high positive values of , however in this case the evolution ends in a pressure singularity,
accompanied by a regular behaviour of the cosmic acceleration. This is a novel
type of singularity appearing in brane-worlds.Comment: 6 pages, 4 figures; expanded version, references added, to appear in
Physical Review
On the validity of the 5-dimensional Birkhoff theorem: The tale of an exceptional case
The 5-dimensional (5d) Birkhoff theorem gives the class of 5d vacuum
space-times containing spatial hypersurfaces with cosmological symmetries. This
theorem is violated by the 5d vacuum Gergely-Maartens (GM) space-time, which is
not a representant of the above class, but contains the static Einstein brane
as embedded hypersurface. We prove that the 5d Birkhoff theorem is still
satisfied in a weaker sense: the GM space-time is related to the degenerated
horizon metric of certain black-hole space-times of the allowed class. This
result resembles the connection between the Bertotti-Robinson space-time and
the horizon region of the extremal Reissner-Nordstrom space-time in general
relativity.Comment: 13 pages; v2: title amended, to be published in Classical and Quantum
Gravit
Metal-rich or misclassified? The case of four RR Lyrae stars
We analysed the light curve of four, apparently extremely metal-rich
fundamental-mode RR Lyrae stars. We identified two stars, MT Tel and ASAS
J091803-3022.6 as RRc (first-overtone) pulsators that were misclassified as
RRab ones in the ASAS survey. In the case of the other two stars, V397 Gem and
ASAS J075127-4136.3, we could not decide conclusively, as they are outliers in
the period-Fourier-coefficient space from the loci of both classes, but their
photometric metallicities also favour the RRc classification.Comment: 5 pages, 2 figures, published in IBVS:
http://ibvs.konkoly.hu/cgi-bin/IBVS?617
Super-energy tensor for space-times with vanishing scalar curvature
A four-index tensor is constructed with terms both quadratic in the Riemann
tensor and linear in its second derivatives, which has zero divergence for
space-times with vanishing scalar curvature. This tensor reduces in vacuum to
the Bel-Robinson tensor. Furthermore, the completely timelike component
referred to any observer is positive, and zero if and only if the space-time is
flat (excluding some unphysical space-times). We also show that this tensor is
the unique that can be constructed with these properties. Such a tensor does
not exist for general gravitational fields. Finally, we study this tensor in
several examples: the Friedmann-Lema\^{\i}tre-Robertson-Walker space-times
filled with radiation, the plane-fronted gravitational waves, and the Vaidya
radiating metric.Comment: 13 pages, LaTeX 2.09. To be published in Journal of Mathematical
Physic
- âŠ