Trace anomaly and black holes evaporation

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dc.creatorCanfora, F.
dc.creatorVilasi, G.
dc.date2003-02-10
dc.date2003-05-05
dc.date.accessioned2026-07-07T03:27:38Z
dc.date.available2026-07-07T03:27:38Z
dc.descriptionA model is proposed to describe a transition from a Schwarzschild black hole of mass $M_{0}$ to a Schwarzschild black hole of mass $M_{1}$ $\leq M_{0}$. The basic equations are derived from the non-vacuum Einstein field equations taking a source representing a null scalar field with a nonvanishing trace anomaly. It is shown that the nonvanishing trace anomaly of the scalar field prevents a complete evaporation.
dc.identifierhttps://arxiv.org/abs/gr-qc/0302036
dc.identifierhttp://arxiv.org/abs/gr-qc/0302036
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34505
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleTrace anomaly and black holes evaporation
dc.typetext

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