Entropy of the Kerr Black Hole Arising from Rarita-Schwinger field

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Abstract

Using the Newman-Penrose formalism and the brick wall model the entropy of a Kerr black hole due to a massless Rarita-Schwinger field is calculated. The dependence of the subleading correction with the spin is analyzed and the differences with previously published results are discussed.

Original languageEnglish
Pages (from-to)59-68
Number of pages10
JournalGeneral Relativity and Gravitation
Volume35
Issue number1
DOIs
StatePublished - Jan 2003
Externally publishedYes

Keywords

  • Black hole
  • Brick wall model
  • Entropy
  • Rarita-Schwinger field

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