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

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dc.creatorWinstanley, Elizabeth
dc.date2004-08-16
dc.date.accessioned2026-07-07T03:28:55Z
dc.date.available2026-07-07T03:28:55Z
dc.descriptionWe 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.
dc.description19 pages, 8 figures, talk given at the `Workshop on Dynamics and Thermodynamics of Black Holes and Naked Singularities', Milan, May 2004
dc.identifierhttps://arxiv.org/abs/gr-qc/0408046
dc.identifierhttp://arxiv.org/abs/gr-qc/0408046
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35016
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleClassical and thermodynamical aspects of black holes with conformally coupled scalar field hair
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