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 |
|