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      Massive Complex Scalar Field in a Kerr-Sen Black Hole Background: Exact Solution of Wave Equation and Hawking Radiation

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          Abstract

          The separated radial part of a massive complex scalar wave equation in the Kerr-Sen geometry is shown to satisfy the generalized spheroidal wave equation which is, in fact, a confluent Heun equation up to a multiplier. The Hawking evaporation of scalar particles in the Kerr-Sen black hole background is investigated by the Damour-Ruffini-Sannan's method. It is shown that quantum thermal effect of the Kerr-Sen black hole has the same characteras that of the Kerr-Newman black hole.

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          Author and article information

          Journal
          10 July 2001
          Article
          10.1063/1.1539899
          gr-qc/0107037
          90252026-f099-4cd4-9e0f-63891b1ae802
          History
          Custom metadata
          J.Math.Phys. 44 (2003) 1084-1088
          Revtex, 5 pages, no figure, submitted to Phys. Rev. D
          gr-qc

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