Thermodynamical model for nonextremal black p-brane

@article{Ohshima2007ThermodynamicalMF,
  title={Thermodynamical model for nonextremal black p-brane},
  author={Ken-ichi Ohshima},
  journal={Physical Review D},
  year={2007},
  volume={76},
  pages={104011}
}
  • K. Ohshima
  • Published 31 December 2006
  • Mathematics
  • Physical Review D
We show that the correct entropy, temperature (and absorption probability) of nonextremal black p-brane can be reproduced by a certain thermodynamical model when maximizing its entropy. We show that the form of the model is related to the geometrical similarity of nonextremal and near extremal black p-brane at near horizon region, and argue about the appropriateness of the model. 

References

SHOWING 1-10 OF 52 REFERENCES

Entropy and temperature of black 3-branes.

We consider slightly nonextremal black 3-branes of type IIB supergravity and show that their Bekenstein-Hawking entropy agrees, up to a mysterious factor, with an entropy derived by counting non-BPS

Action Integrals and Partition Functions in Quantum Gravity

One can evaluate the action for a gravitational field on a section of the complexified spacetime which avoids the singularities. In this manner we obtain finite, purely imaginary values for the

Threebrane Absorption and Emission from a Brane-Antibrane System

We show that a previously proposed model based on a D3-brane--anti-D3-brane system at finite temperature can reproduce the low-frequency absorption and emission probabilities of the black threebrane

Higher-dimensional resolution of dilatonic black-hole singularities

We show that the four-dimensional extreme dilaton black hole with dilaton coupling constant can be interpreted as a completely non-singular, non-dilatonic, black p-brane in (4+p) dimensions provided

Quasinormal modes for nonextreme Dp-branes and thermalizations of super-Yang-Mills theories

The nonextreme Dp-brane solutions in type II supergravity (in the near-horizon limit) are expected to be dual to (p+1)-dimensional noncompact supersymmetric Yang-Mills theories at finite temperature.

Particle creation by black holes

AbstractIn the classical theory black holes can only absorb and not emit particles. However it is shown that quantum mechanical effects cause black holes to create and emit particles as if they were

Thermodynamics of black holes in anti-de Sitter space

The Einstein equations with a negative cosmological constant admit black hole solutions which are asymptotic to anti-de Sitter space. Like black holes in asymptotically flat space, these solutions

Erratum: Action and entropy of extreme and nonextreme black holes

  • Teitel'boim
  • Physics
    Physical review. D, Particles and fields
  • 1995
The Hamiltonian actions for extreme and nonextreme black holes are compared and contrasted and a simple derivation of the lack of entropy of extreme black holes is given. In the nonextreme case the

Microscopic origin of the Bekenstein-Hawking entropy

...