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dc.contributor.author | Nugayev R. | |
dc.date.accessioned | 2018-09-14T20:04:47Z | |
dc.date.available | 2018-09-14T20:04:47Z | |
dc.date.issued | 1983 | |
dc.identifier.issn | 0004-640X | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/132101 | |
dc.description.abstract | The results of various calculations of the Casimir effect and of the effect of particle creation by accelerated mirrors are applied to the case of a collapse-formed black hole, which in consequence produces black-body radiation. Its temperature coincides exactly with Hawking's result. The difference between the vacuum expectation values of the energy-momentum tensors of scalar and electromagnetic fields near the horizon is found. Further investigation of expanding spheres in flat-space-time should disclose where the radiation is being created and what happens near the horizon. © 1983 D. Reidel Publishing Co. | |
dc.relation.ispartofseries | Astrophysics and Space Science | |
dc.title | An outline of approach linking black-hole-evaporation with quantum-field effects in flat spacetime | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 1 | |
dc.relation.ispartofseries-volume | 91 | |
dc.collection | Публикации сотрудников КФУ | |
dc.relation.startpage | 53 | |
dc.source.id | SCOPUS0004640X-1983-91-1-SID33947697055 |