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Classical and thermodynamical aspects of black holes with conformally coupled scalar field hair · arXivDesk

gr-qc/0408046Aug 16, 200419 pages, 8 figures, talk given at the `Workshop on Dynamics and Thermodynamics of Black Holes and Naked Singularities', Milan, May 2004

Classical and thermodynamical aspects of black holes with conformally coupled scalar field hair

Elizabeth Winstanley

General Relativity and Quantum Cosmology

arXiv PDF

Abstract

We discuss the existence, stability and classical thermodynamics of four-dimensional, spherically symmetric black hole solutions of the Einstein equations with a conformally coupled scalar field. We review the solutions existing in the literature with zero, positive and negative cosmological constant. We also outline new results on the thermodynamics of these black holes when the cosmological constant is non-zero.

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Researchers working in gr-qc and adjacent areas.

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The paper addresses: Classical and thermodynamical aspects of black holes with conformally coupled scalar field hair.
We discuss the existence, stability and classical thermodynamics of four-dimensional, spherically symmetric black hole solutions of the Einstein equations with a conformally coupled scalar field.

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Author comment: 19 pages, 8 figures, talk given at the `Workshop on Dynamics and Thermodynamics of Black Holes and Naked Singularities', Milan, May 2004