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http://hdl.handle.net/2289/3243
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DC Field | Value | Language |
---|---|---|
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.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.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.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 |
Appears in Collections: | Research Papers (TP) |
Files in This Item:
File | Description | Size | Format | |
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1981 PL-A V82 p1.pdf Restricted Access | Restricted Access | 211.76 kB | Adobe PDF | View/Open Request a copy |
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