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Einstein-Planck Formula, Equivalence Principle, and Black Hole Radiance

Repositori DSpace/Manakin

dc.contributor.author	Fabbri, Alessandro
dc.contributor.author	Navarro Salas, José
dc.date.accessioned	2014-03-29T10:30:55Z
dc.date.available	2014-03-29T10:30:55Z
dc.date.issued	2005
dc.identifier.citation	Fabbri, Alessandro Navarro Salas, José 2005 Einstein-Planck Formula, Equivalence Principle, and Black Hole Radiance International Journal of Modern Physics D 14 12 2213 2218
dc.identifier.uri	http://hdl.handle.net/10550/33781
dc.description.abstract	The presence of gravity implies corrections to the Einstein-Planck formula E = hν. This gives hope that the divergent blueshift in frequency, associated to the presence of a black hole horizon, could be smoothed out for the energy. Using simple arguments based on Einstein's equivalence principle, we show that this is only possible if a black hole emits, in a first approximation, not just a single particle, but thermal radiation.
dc.relation.ispartof	International Journal of Modern Physics D, 2005, vol. 14, num. 12, p. 2213-2218
dc.subject	Astrofísica
dc.subject	Camps, Teoria quàntica de
dc.subject	Gravitació
dc.title	Einstein-Planck Formula, Equivalence Principle, and Black Hole Radiance
dc.type	journal article	es_ES
dc.date.updated	2014-03-29T10:30:55Z
dc.identifier.doi	10.1142/S0218271805007966
dc.identifier.idgrec	035533
dc.rights.accessRights	open access	es_ES
dc.identifier.url	10.1142/S0218271805007966