Hawking Radiation in Trace Anomaly Free Frames

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dc.creatorSalehi, H.
dc.creatorMirabotalebi, S.
dc.date2004-02-16
dc.date.accessioned2026-07-07T03:28:28Z
dc.date.available2026-07-07T03:28:28Z
dc.descriptionWe have used the results of renormalization of a two-dimensional quantum stress tensor to develop a conformally invariant dynamical model. The model requires the consideration of those conformal frames in which there exists a correspondence between the trace anomaly and a cosmological constant. We apply this model to a two dimensional-Schwarzschild (-de Sitter) spacetime to show that in these conformal frames one may achieve Hawking radiation without recourse to the trace anomaly .
dc.description7 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0402074
dc.identifierhttp://arxiv.org/abs/gr-qc/0402074
dc.identifierGen.Rel.Grav. 34 (2002) 23-30
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34845
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHawking Radiation in Trace Anomaly Free Frames
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