24 research outputs found
The holographic bound in the scalar-tensor and gravities
The holographic bound has been extended to the different theory of gravities
such as scalar-tensor gravity and gravity according to the Noether
charge definition of the entropy for a black hole surface. We have introduced
some popular examples of the flat FRW cosmology in order to investigate
holographic bound in scalar-tensor and gravity. Using the holographic
bound, we put an additional constraint on the scalar-tensor gravity and
gravity parameters. We also discuss about the transformation from Jordan frame
to Einstein frame.Comment: accepted in European Physical Journal C (epjc), a section added to
the pape
Radiation from the LTB black hole
Does a dynamical black hole embedded in a cosmological FRW background emit
Hawking radiation where a globally defined event horizon does not exist? What
are the differences to the Schwarzschild black hole? What about the first law
of black hole mechanics? We face these questions using the LTB cosmological
black hole model recently published. Using the Hamilton-Jacobi and radial null
geodesic-methods suitable for dynamical cases, we show that it is the apparent
horizon which contributes to the Hawking radiation and not the event horizon.
The Hawking temperature is calculated using the two different methods giving
the same result. The first law of LTB black hole dynamics and the thermal
character of the radiation is also dealt with.Comment: 9 pages, revised version, Europhysics Letter 2012 97 2900
The spherical symmetry Black hole collapse in expanding universe
The spherical symmetry Black holes are considered in expanding background.
The singularity line and the marginally trapped tube surface behavior are
discussed. In particular, we address the conditions whether dynamical horizon
forms for these cosmological black holes. We also discuss about the
cosmological constant effect on these black hole and the redshift of the light
which comes from the marginally trapped tube surface.Comment: 7 pages, 3 figures. Accepted for publication in International Journal
of Modern Physics D (IJMPD). arXiv admin note: text overlap with
arXiv:gr-qc/0308033 and arXiv:gr-qc/030611
Cosmological LTB Black Hole in a Quintom Universe
We study cosmological Lemaitre-Tolman-Bondi (LTB) black hole thermodynamics
immersed in a quintom universe. We investigate some thermodynamic aspects of
such a black hole in detail. We apply two methods of treating particles'
tunneling from the apparent horizons and calculate the black hole's temperature
in each method; the results of which are the same. In addition, by considering
specific time slices in cosmic history, we study the thermodynamic features of
this black hole in these specific cosmic epochs. Also, we discuss the
information loss problem and the remnant content of the cosmological black hole
in different cosmic epochs in this context. We show that approximately in all
cosmic history, the temperature of the black hole's apparent horizon is more
than the temperature of the cosmological apparent horizon
On the time dependent Schwarzschild - de Sitter spacetime
An imperfect cosmic fluid with energy flux is analyzed. Even though its
energy density is positive, the pressure due to the fact
that the metric is asymptotically de Sitter. The kinematical quantities for a
nongeodesic congruence are computed. The scalar expansion is time independent
but divergent at the singularity . Far from the central mass and
for a cosmic time , the heat flux does not depend on
Newton's constant .Comment: 8 pages, no figures, Sections 3 and 5 enlarged, one reference adde
Do we know the mass of a black hole? Mass of some cosmological black hole models
Using a cosmological black hole model proposed recently, we have calculated
the quasi-local mass of a collapsing structure within a cosmological setting
due to different definitions put forward in the last decades to see how similar
or different they are. It has been shown that the mass within the horizon
follows the familiar Brown-York behavior. It increases, however, outside the
horizon again after a short decrease, in contrast to the Schwarzschild case.
Further away, near the void, outside the collapsed region, and where the
density reaches the background minimum, all the mass definitions roughly
coincide. They differ, however, substantially far from it. Generically, we are
faced with three different Brown-York mass maxima: near the horizon, around the
void between the overdensity region and the background, and another at
cosmological distances corresponding to the cosmological horizon. While the
latter two maxima are always present, the horizon mass maxima is absent before
the onset of the central singularity.Comment: 11 pages, 8 figures, revised version, accepted in General Relativity
and Gravitatio
Complete solutions to the metric of spherically collapsing dust in an expanding spacetime with a cosmological constant
We present semi-analytical solutions to the background equations describing
the Lema\^itre-Tolman-Bondi (LTB) metric as well as the homogeneous Friedmann
equations, in the presence of dust, curvature and a cosmological constant
Lambda. For none of the presented solutions any numerical integration has to be
performed. All presented solutions are given for expanding and collapsing
phases, preserving continuity in time and radius. Hence, these solutions
describe the complete space time of a collapsing spherical object in an
expanding universe. In the appendix we present for completeness a solution of
the Friedmann equations in the additional presence of radiation, only valid for
the Robertson-Walker metric.Comment: 23 pages, one figure. Numerical module for evaluation of the
solutions released at
http://web.physik.rwth-aachen.de/download/valkenburg/ColLambda/ Matches
published version, published under Open Access. Note change of titl
A concrete anti-de Sitter black hole with dynamical horizon having toroidal cross-sections and its characteristics
We propose a special solution of Einstein equations in the general Vaidya form representing a dynamical black hole having horizon cross-sections with toroidal topology. The concrete model enables us to study for the first time dynamical horizons with toroidal topology, its area law, and the question of matter flux inside the horizon, without using a cut-and-paste technology to construct the solution