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dc.contributor.authorFayos Vallés, Francisco
dc.contributor.authorTorres Herrera, Ramon
dc.contributor.otherUniversitat Politècnica de Catalunya. Departament de Física Aplicada
dc.date.accessioned2013-11-12T10:50:37Z
dc.date.available2013-11-12T10:50:37Z
dc.date.created2011-09-01
dc.date.issued2011-09-01
dc.identifier.citationFayos, F.; Torres, R. An approach to evaporating stars and black holes. "Journal of physics: conference series", 01 Setembre 2011, vol. 314, p. 1-3.
dc.identifier.issn1742-6588
dc.identifier.urihttp://hdl.handle.net/2117/20582
dc.description.abstractMany models in which the object under study loses all its mass have appeared in the literature. No doubt, the most eminent examples are the models for evaporating black holes and for evaporating stars. Here we describe a semiclassical study of these evaporating models centered on the evaporating event itself. We pay special attention to the evaporating models as a means of avoiding singularities during the collapse. In case of any pre-existing non-spacelike curvature singularity, we show that these models tend to evaporate it.
dc.format.extent3 p.
dc.language.isoeng
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Spain
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subjectÀrees temàtiques de la UPC::Física
dc.subject.lcshBlack holes (Astronomy)
dc.titleAn approach to evaporating stars and black holes
dc.typeArticle
dc.subject.lemacForats negres (Astronomia)
dc.contributor.groupUniversitat Politècnica de Catalunya. DF - Dinàmica No Lineal de Fluids
dc.identifier.doi10.1088/1742-6596/314/1/012127
dc.description.peerreviewedPeer Reviewed
dc.relation.publisherversionhttp://iopscience.iop.org/1742-6596/314/1/012127/
dc.rights.accessOpen Access
local.identifier.drac12722923
dc.description.versionPostprint (published version)
local.citation.authorFayos, F.; Torres, R.
local.citation.publicationNameJournal of physics: conference series
local.citation.volume314
local.citation.startingPage1
local.citation.endingPage3


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