Показать сокращенную информацию
dc.contributor.author | Khusnutdinov N. | |
dc.date.accessioned | 2018-09-17T20:46:27Z | |
dc.date.available | 2018-09-17T20:46:27Z | |
dc.date.issued | 2003 | |
dc.identifier.issn | 0556-2821 | |
dc.identifier.uri | https://dspace.kpfu.ru/xmlui/handle/net/134030 | |
dc.description.abstract | Smooth-throat wormholes are treated as possessing quantum fluctuation energy with a scalar massive field as its source. The heat kernel coefficients of the Laplace operator are calculated in the background of the arbitrary-profile throat wormhole with the help of the zeta-function approach. Two specific profiles are considered. Some arguments are given that wormholes may exist. It serves as a solution of semiclassical Einstein equations in the range of specific values of the length, a certain radius of the wormhole's throat, and a constant of nonminimal connection. © 2003 The American Physical Society. | |
dc.relation.ispartofseries | Physical Review D | |
dc.title | Semiclassical wormholes | |
dc.type | Article | |
dc.relation.ispartofseries-issue | 12 | |
dc.relation.ispartofseries-volume | 67 | |
dc.collection | Публикации сотрудников КФУ | |
dc.source.id | SCOPUS05562821-2003-67-12-SID0043130201 |