On how energy conservation might prevent black hole explosions and violations of the third law

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dc.contributor	Universitat Politècnica de Catalunya. Departament de Física Aplicada
dc.contributor	Universitat Politècnica de Catalunya. DF - Dinàmica No Lineal de Fluids
dc.contributor.author	Torres Herrera, Ramon
dc.contributor.author	Fayos Vallés, Francisco
dc.date	2013-11-12
dc.identifier.citation	Torres, R.; Fayos, F. On how energy conservation might prevent black hole explosions and violations of the third law. "International journal of modern physics D", 12 Novembre 2013, vol. 23, núm. 1, p. 1450009-1-1450009-15.
dc.identifier.citation	0218-2718
dc.identifier.citation	10.1142/S0218271814500096
dc.identifier.uri	http://hdl.handle.net/2117/21837
dc.language.iso	eng
dc.relation	http://www.worldscientific.com/doi/abs/10.1142/S0218271814500096
dc.rights	Attribution-NonCommercial-NoDerivs 3.0 Spain
dc.rights	info:eu-repo/semantics/openAccess
dc.rights	http://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subject	Àrees temàtiques de la UPC::Física
dc.subject	Black holes (Astronomy)
dc.subject	Black Holes
dc.subject	Hawking radiation
dc.subject	Black Hole Thermodynamics
dc.subject	Third Law
dc.subject	Forats negres (Astronomia)
dc.title	On how energy conservation might prevent black hole explosions and violations of the third law
dc.type	info:eu-repo/semantics/draft
dc.type	info:eu-repo/semantics/article
dc.description.abstract	Preprint of an article published in International journal of modern physics D, 23, 1, 2013, 1450009-1 - 1450009-15 10.1142/S0218271814500096 © copyright World Scientific Publishing Company http://www.worldscientific.com/worldscinet/ijmpd
dc.description.abstract	We claim that imposing energy conservation to the emission of Hawking radiation and to the modeling of black hole (BH) evaporation might prevent BH explosions as well as violations of the third law of BH thermodynamics. This is specifically shown for the general class of spherically symmetric quantum BHs described by an effective quantum vacuum invariant under boosts in the radial direction. No assumptions are made with regard to the specific framework from which the quantum BHs are derived.

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