Semiclassical wormholes

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

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Коллекция содержит публикации сотрудников Казанского федерального (до 2010 года Казанского государственного) университета, проиндексированные в БД Scopus, начиная с 1970г.