1,254 research outputs found
Thermodynamics of Quasi-Topological Cosmology
In this paper, we study thermodynamical properties of the apparent horizon in
a universe governed by quasi-topological gravity. Our aim is twofold. First, by
using the variational method we derive the general form of Friedmann equation
in quasi-topological gravity. Then, by applying the first law of thermodynamics
on the apparent horizon, after using the entropy expression associated with the
black hole horizon in quasi-topological gravity, and replacing the horizon
radius, , with the apparent horizon radius, , we derive
the corresponding Friedmann equation in quasi-topological gravity. We find that
these two different approaches yield the same result which show the profound
connection between the first law of thermodynamics and the gravitational field
equations of quasi-topological gravity. We also study the validity of the
generalized second law of thermodynamics in quasi-topological cosmology. We
find that, with the assumption of the local equilibrium hypothesis, the
generalized second law of thermodynamics is fulfilled for the universe
enveloped by the apparent horizon for the late time cosmology.Comment: 8 pages, no figure, Phys. Lett B, in press (2013
Thermodynamical study of FRW universe in Quasi-Topological Theory
By applying the unified first law of thermodynamics on the apparent horizon
of FRW universe, we get the entropy relation for the apparent horizon in
quasi-topological gravity theory. Throughout the paper, the results of
considering the Hayward-Kodama and Cai-Kim temperatures are also addressed. Our
study shows that whenever, there is no energy exchange between the various
parts of cosmos, we can get an expression for the apparent horizon entropy in
quasi-topological gravity, which is in agreement with other attempts followed
different approaches. The effects of a mutual interaction between the various
parts of cosmos on the apparent horizon entropy as well as the validity of
second law of thermodynamics in quasi-topological gravity are also perused.Comment: The text has been revised and some new references are adde
Venomous Animals; Are They Important in Iran?
Many reports have indicated the medical importance of animal poisons in Iran. The significance numbers of Iranians are injured from high endemic to sporadic, by venomous snakes, scorpions, wasps, bees, fire and velvet ants, spiders and backswimmer bugs, so their nuisance prevention is an important task
Thermodynamics of Rotating Charged Black Branes in Third Order Lovelock Gravity and the Counterterm Method
We generalize the quasilocal definition of the stress energy tensor of
Einstein gravity to the case of third order Lovelock gravity, by introducing
the surface terms that make the action well-defined. We also introduce the
boundary counterterm that removes the divergences of the action and the
conserved quantities of the solutions of third order Lovelock gravity with zero
curvature boundary at constant and . Then, we compute the charged
rotating solutions of this theory in dimensions with a complete set of
allowed rotation parameters. These charged rotating solutions present black
hole solutions with two inner and outer event horizons, extreme black holes or
naked singularities provided the parameters of the solutions are chosen
suitable. We compute temperature, entropy, charge, electric potential, mass and
angular momenta of the black hole solutions, and find that these quantities
satisfy the first law of thermodynamics. We find a Smarr-type formula and
perform a stability analysis by computing the heat capacity and the determinant
of Hessian matrix of mass with respect to its thermodynamic variables in both
the canonical and the grand-canonical ensembles, and show that the system is
thermally stable. This is commensurate with the fact that there is no
Hawking-Page phase transition for black objects with zero curvature horizon.Comment: 19 pages, 1 figure, a few references added, typos correcte
Counterterms for Static Lovelock Solutions
In this paper, we introduce the counterterms that remove the non-logarithmic
divergences of the action in third order Lovelock gravity for static
spacetimes. We do this by defining the cosmological constant in such a way that
the asymptotic form of the metric have the same form in Lovelock and Einstein
gravities. Thus, we employ the counterterms of Einstein gravity and show that
the power law divergences of the action of Lovelock gravity for static
spacetimes can be removed by suitable choice of coefficients. We find that the
dependence of these coefficients on the dimension in Lovelock gravity is the
same as in Einstein gravity. We also introduce the finite energy-momentum
tensor and employ these counterterms to calculate the finite action and mass of
static black hole solutions of third order Lovelock gravity. Next, we calculate
the thermodynamic quantities and show that the entropy calculated through the
use of Gibbs-Duhem relation is consistent with the obtained entropy by Wald's
formula. Furthermore, we find that in contrast to Einstein gravity in which
there exists no uncharged extreme black hole, third order Lovelock gravity can
have these kind of black holes. Finally, we investigate the stability of static
charged black holes of Lovelock gravity in canonical ensemble and find that
small black holes show a phase transition between very small and small black
holes, while the large ones are stable.Comment: arXiv admin note: text overlap with arXiv:1008.0102 by other author
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