New Formulation of the First Law of Black Hole Thermodynamics: A Stringy Analogy

Details New Formulation of the First Law of Black Hole Thermodynamics: A Stringy Analogy New Formulation of the First Law of Black Hole Thermodynamics: A Stringy Analogy

2004-05-06

arxiv.org/abs/gr-qc/0405029v2

Phys.Lett. B608 (2005) 251-257

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

5 pages, no figure, revtex 4, one reference added and typesetting errors corrected

Scientific paper

10.1016/j.physletb.2005.01.018

We consider the first laws of thermodynamics for a pair of systems made up of the two horizons of a Kerr-Newman black hole. These two systems are constructed in such a way that we only demand their ``horizon areas'' to be the sum and difference of that of the outer and inner horizons of their prototype. Remarkably, these two copies bear a striking resemblance to the right- and left-movers in string theory and D-brane physics. Our reformulation of the first law of black hole thermodynamics can be thought of as an analogy of thermodynamics of effective string or D-brane models.

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