Hawking radiation via gravitational anomalies in nonspherical topologies

Papantonopoulos, E; Skamagoulis, P

dc.contributor.author	Papantonopoulos, E	en
dc.contributor.author	Skamagoulis, P	en
dc.date.accessioned	2014-03-01T01:30:50Z
dc.date.available	2014-03-01T01:30:50Z
dc.date.issued	2009	en
dc.identifier.issn	1550-7998	en
dc.identifier.uri	https://dspace.lib.ntua.gr/xmlui/handle/123456789/19641
dc.subject	Hawking Radiation	en
dc.subject	Negative Curvature	en
dc.subject	Scalar Field	en
dc.subject	Black Hole	en
dc.subject.classification	Astronomy & Astrophysics	en
dc.subject.classification	Physics, Particles & Fields	en
dc.subject.other	BLACK-HOLES	en
dc.subject.other	COVARIANT ANOMALIES	en
dc.subject.other	BOUNDARY-CONDITIONS	en
dc.subject.other	PSEUDOSPHERE	en
dc.subject.other	HORIZONS	en
dc.subject.other	CREATION	en
dc.title	Hawking radiation via gravitational anomalies in nonspherical topologies	en
heal.type	journalArticle	en
heal.identifier.primary	10.1103/PhysRevD.79.084022	en
heal.identifier.secondary	http://dx.doi.org/10.1103/PhysRevD.79.084022	en
heal.identifier.secondary	084022	en
heal.language	English	en
heal.publicationDate	2009	en
heal.abstract	We study the method of calculating Hawking radiation via gravitational anomalies in gravitational backgrounds of constant negative curvature. We apply the method to topological black holes and also to topological black holes conformally coupled to a scalar field. © 2009 The American Physical Society.	en
heal.publisher	AMER PHYSICAL SOC	en
heal.journalName	Physical Review D - Particles, Fields, Gravitation and Cosmology	en
dc.identifier.doi	10.1103/PhysRevD.79.084022	en
dc.identifier.isi	ISI:000266408500084	en
dc.identifier.volume	79	en
dc.identifier.issue	8	en