Vacuum fluctuations of twisted fields in the spacetime of a cosmic string

dc.contributorInstituto de Fisica Teorica
dc.date.accessioned2022-04-29T08:42:50Z
dc.date.accessioned2022-12-20T03:09:58Z
dc.date.available2022-04-29T08:42:50Z
dc.date.available2022-12-20T03:09:58Z
dc.date.created2022-04-29T08:42:50Z
dc.date.issued1990-01-01
dc.identifierPhysical Review D, v. 41, n. 12, p. 3846-3847, 1990.
dc.identifier0556-2821
dc.identifierhttp://hdl.handle.net/11449/230943
dc.identifier10.1103/PhysRevD.41.3846
dc.identifier2-s2.0-0040432795
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/5411077
dc.description.abstractA twisted scalar field conformally coupled to gravitation is used to calculate the vacuum stress-energy tensor in the background spacetime generated by an infinite straight gauge cosmic string. The result found has an absolute numerical value close to the one obtained with a nontwisted conformal scalar field, but their signs are opposite. © 1990 The American Physical Society.
dc.languageeng
dc.relationPhysical Review D
dc.sourceScopus
dc.titleVacuum fluctuations of twisted fields in the spacetime of a cosmic string
dc.typeArtículos de revistas


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