Hawking radiation via higher-spin gauge anomalies

Satoshi Iso, Takeshi Morita, and Hiroshi Umetsu
Phys. Rev. D 77, 045007 – Published 4 February 2008

Abstract

We give a higher-spin generalization of the anomaly method for the Hawking radiation from black holes. In the paper [S. Iso, T. Morita, and H. Umetsu, arXiv:0710.0453.] higher-spin generalizations of the gauge (and gravitational) anomalies in d=2 were obtained. By applying these anomalies to black hole physics, we derive the higher moments of the Hawking fluxes. We also give a higher-spin generalization of the trace anomaly method by Christensen and Fulling [S. Christensen and S. Fulling, Phys. Rev. D 15, 2088 (1977).].

  • Received 9 October 2007

DOI:https://doi.org/10.1103/PhysRevD.77.045007

©2008 American Physical Society

Authors & Affiliations

Satoshi Iso1,*, Takeshi Morita2,†, and Hiroshi Umetsu3,‡

  • 1Institute of Particle and Nuclear Studies, High Energy Accelerator Research Organization (KEK), Oho 1-1, Tsukuba, Ibaraki 305-0801, Japan
  • 2Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502, Japan
  • 3Okayama Institute for Quantum Physics, Kyoyama 1-9-1, Okayama 700-0015, Japan

  • *satoshi.iso@kek.jp
  • Present address: Department of Theoretical Physics, Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India. mtakeshi@yukawa.kyoto-u.ac.jp, takeshi@theory.tifr.res.in
  • hiroshi_umetsu@pref.okayama.jp

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Issue

Vol. 77, Iss. 4 — 15 February 2008

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