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Tachyon field quantization and Hawking radiation

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dc.contributor.author Chiou-Lahanas, C en
dc.contributor.author Diamandis, GA en
dc.contributor.author Georgalas, BC en
dc.contributor.author Maintas, XN en
dc.contributor.author Papantonopoulos, E en
dc.date.accessioned 2014-03-01T01:11:31Z
dc.date.available 2014-03-01T01:11:31Z
dc.date.issued 1995 en
dc.identifier.issn 0556-2821 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/11678
dc.subject Hawking Radiation en
dc.subject Scalar Curvature en
dc.subject Scalar Field en
dc.subject Thermal Radiation en
dc.subject Black Hole en
dc.subject.classification Astronomy & Astrophysics en
dc.subject.classification Physics, Particles & Fields en
dc.subject.other 2-DIMENSIONAL STRING THEORY en
dc.subject.other NONLINEAR SIGMA-MODEL en
dc.subject.other BLACK-HOLE en
dc.subject.other HAIR en
dc.title Tachyon field quantization and Hawking radiation en
heal.type journalArticle en
heal.identifier.primary 10.1103/PhysRevD.52.5877 en
heal.identifier.secondary http://dx.doi.org/10.1103/PhysRevD.52.5877 en
heal.language English en
heal.publicationDate 1995 en
heal.abstract We quantize the tachyon field in a static two-dimensional dilaton gravity black hole background, and we calculate the Hawking radiation rate. We find that the thermal radiation flux, due to the tachyon field, is larger than the conformal matter one. We also find that massive scalar fields which do not couple to the dilaton do not give any contribution to the thermal radiation up to terms quadratic in the scalar curvature. © 1995 The American Physical Society. en
heal.publisher AMERICAN PHYSICAL SOC en
heal.journalName Physical Review D en
dc.identifier.doi 10.1103/PhysRevD.52.5877 en
dc.identifier.isi ISI:A1995TF80200052 en
dc.identifier.volume 52 en
dc.identifier.issue 10 en
dc.identifier.spage 5877 en
dc.identifier.epage 5882 en


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