Validity of the quasistatic approximation in the theory of black hole evaporation

dc.contributor.author	Nityananda, R.
dc.contributor.author	Narayan, R.
dc.date.accessioned	2007-07-10T07:44:35Z
dc.date.available	2007-07-10T07:44:35Z
dc.date.issued	1981-03
dc.description	Restricted Access.	en
dc.description.abstract	It 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.extent	216840 bytes
dc.format.mimetype	application/pdf
dc.identifier.citation	Physics Letters A, 1981, Vol.82, p1-3	en
dc.identifier.issn	0375-9601
dc.identifier.uri	http://hdl.handle.net/2289/3243
dc.language.iso	en	en
dc.publisher	Elsevier B.V.	en
dc.relation.uri	http://dx.doi.org/10.1016/0375-9601(81)90384-4	en
dc.rights	1981 Elsevier B.V.	en
dc.title	Validity of the quasistatic approximation in the theory of black hole evaporation	en
dc.type	Article	en

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