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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 |