dc.contributor.author |
Nugayev R. |
|
dc.date.accessioned |
2018-09-14T20:15:06Z |
|
dc.date.available |
2018-09-14T20:15:06Z |
|
dc.date.issued |
1985 |
|
dc.identifier.issn |
0369-3554 |
|
dc.identifier.uri |
https://dspace.kpfu.ru/xmlui/handle/net/132268 |
|
dc.description.abstract |
The application of quantum-field flat-space-time results to a black hole reveals the domain and the mechanism of particle creation. The Hawking radiation is «squeezed out» by the tail of gravitational-field potential barrier in the [1.5 Rg, ∞] region. Its black-body spectrum is due to the interaction of virtual particles with the «cavity» formed by the potential barrier. © 1985 Società Italiana di Fisica. |
|
dc.relation.ispartofseries |
Il Nuovo Cimento B Series 11 |
|
dc.subject |
PACS. 97.60 Late stages of stellar evolution (including black holes) |
|
dc.title |
Particle creation by a black hole as a consequence of quantum-field effects in flat space-time |
|
dc.type |
Article |
|
dc.relation.ispartofseries-issue |
1 |
|
dc.relation.ispartofseries-volume |
86 |
|
dc.collection |
Публикации сотрудников КФУ |
|
dc.relation.startpage |
90 |
|
dc.source.id |
SCOPUS03693554-1985-86-1-SID51649153416 |
|