Fluxes of higher-spin currents and Hawking radiation from charged black holes

Satoshi Iso, Takeshi Morita, and Hiroshi Umetsu
Phys. Rev. D 76, 064015 – Published 13 September 2007

Abstract

This is an extended version of the previous paper [S. Iso, T. Morita, and H. Umetsu, Phys. Rev. D 75, 124004 (2007).]. Quantum fields near horizons can be described in terms of an infinite set of two-dimensional conformal fields. We first generalize the method of Christensen and Fulling to charged black holes to derive fluxes of energy and charge. These fluxes can be obtained by employing a conformal field theory technique. We then apply this technique to obtain the fluxes of higher-spin currents and show that the thermal distribution of Hawking radiation from a charged black hole can be completely reproduced by investigating transformation properties of the higher-spin currents under conformal and gauge transformations.

  • Received 29 May 2007

DOI:https://doi.org/10.1103/PhysRevD.76.064015

©2007 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
  • mtakeshi@yukawa.kyoto-u.ac.jp
  • hiroshi_umetsu@pref.okayama.jp

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Issue

Vol. 76, Iss. 6 — 15 September 2007

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