Casimir effect and thermodynamics of horizon instabilities

Details Casimir effect and thermodynamics of horizon instabilities Casimir effect and thermodynamics of horizon instabilities

2004-03-30

arxiv.org/abs/hep-th/0403281v2

Phys.Rev. D70 (2004) 044015

Physics

High Energy Physics

High Energy Physics - Theory

1 + 14 pages. LaTeX. 1 figure. Minor addition and references added

Scientific paper

10.1103/PhysRevD.70.044015

We propose a dual thermodynamic description of a classical instability of generalised black hole spacetimes. From a thermodynamic perspective, the instability is due to negative compressibility in regions where the Casimir pressure is large. The argument indicates how the correspondence between thermodynamic and classical instability for horizons may be extended to cases without translational invariance.

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