1995
DOI: 10.1103/physrevd.52.5877
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Tachyon field quantization and Hawking radiation

Abstract: AbstactWe 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.

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Cited by 13 publications
(18 citation statements)
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“…In this work we consider solutions of two-dimensional dilaton gravity with R 2 term which can be viewed as backreaction term from quantization of matter. Of course this term has interest by itself considered as R 2 gravity but we emphasize its quantum origin and the fact that, in the semiclassical approximation, it does not contribute to the Hawking radiation [2]. We confirm the static solutions found in [3] working in the conformal gauge and using light-cone coordinates.…”
Section: Time Dependencesupporting
confidence: 75%
“…In this work we consider solutions of two-dimensional dilaton gravity with R 2 term which can be viewed as backreaction term from quantization of matter. Of course this term has interest by itself considered as R 2 gravity but we emphasize its quantum origin and the fact that, in the semiclassical approximation, it does not contribute to the Hawking radiation [2]. We confirm the static solutions found in [3] working in the conformal gauge and using light-cone coordinates.…”
Section: Time Dependencesupporting
confidence: 75%
“…Hence, Φ is identified with the Hawking flux of the MTZ black hole, which is a (3+1)-dimensional topological black hole conformally coupled to a scalar field. 6 Robinson-Wilczek Method with a Scalar Field Non-minimally Coupled to the Black Hole Background…”
Section: Hawking Radiation From a Tbh Conformally Coupled To A Scalar...mentioning
confidence: 99%
“…The part S f ree is the free part of the action. The second term is 6) and describes the interactions of the scalar field. The third term is…”
Section: Robinson-wilczek Methods With a Scalar Field Non-minimallymentioning
confidence: 99%
See 1 more Smart Citation
“…Таким образом, проблема нахождения амплитуды рассеяния сводится к вычислению достаточно сложного функционального интеграла (6).…”
Section: амплитуда упругого рассеянияunclassified