Thermodynamic structure of field equations near apparent horizon for radiating black holes - INSPIRE

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Thermodynamic structure of field equations near apparent horizon for radiating black holes

Uma Papnoi
(
- Jamia Millia Islamia
)
,
Megan Govender
(
- KwaZulu Natal U.
)
,
Sushant G. Ghosh
(
- Jamia Millia Islamia and
- KwaZulu Natal U.
)

Oct 31, 2014

10 pages

Published in:

Mod.Phys.Lett.A 29 (2014) 34, 1450188

Published: Oct 31, 2014

e-Print:

1411.2323 [gr-qc]

DOI:

10.1142/S0217732314501880

View in:

ADS Abstract Service

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Abstract: (World Scientific)

We study the intriguing analogy between gravitational dynamics of the horizon and thermodynamics for the case of nonstationary radiating spherically symmetric black holes both in four dimensions and higher dimensions. By defining all kinematical parameters of nonstationary radiating black holes in terms of null vectors, we demonstrate that it is possible to interpret the Einstein field equations near the apparent horizon in the form of a thermodynamical identity T dS = dE+P dV.

04.30.-w
04.50.Gh
Black hole
thermodynamics
higher dimensions
dimension: 4
symmetry: rotation
black hole: thermodynamics
radiation: Hawking
horizon

References(28)

Figures(0)

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