Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3243
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dc.contributor.authorNityananda, R.-
dc.contributor.authorNarayan, R.-
dc.date.accessioned2007-07-10T07:44:35Z-
dc.date.available2007-07-10T07:44:35Z-
dc.date.issued1981-03-
dc.identifier.citationPhysics Letters A, 1981, Vol.82, p1-3en
dc.identifier.issn0375-9601-
dc.identifier.urihttp://hdl.handle.net/2289/3243-
dc.descriptionRestricted Access.en
dc.description.abstractIt has recently been proposed that the Hawking picture of previous termblack hole evaporationnext term breaks down when the back reaction of the emitted radiation is included. Our reanalysis shows that the equation for the evolution of the horizon has well-behaved solutions which closely follow the Hawking picture.en
dc.format.extent216840 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherElsevier B.V.en
dc.relation.urihttp://dx.doi.org/10.1016/0375-9601(81)90384-4en
dc.rights1981 Elsevier B.V.en
dc.titleValidity of the quasistatic approximation in the theory of black hole evaporationen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

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