Area spectrum of the D-dimensional de Sitter spacetime

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Abstract

The determination of the quantum area spectrum of a black hole horizon by means of its asymptotic quasinormal frequencies has been explored recently. We believe that for D-dimensional de Sitter horizon we must study if the idea works. Thus taking into account the local description of the thermodynamics of horizons proposed by Padmanabhan and the results of Hod, Kunstatter, and Maggiore we study the area spectrum of the D-dimensional de Sitter horizon.

Original languageEnglish
Pages (from-to)85-88
Number of pages4
JournalPhysics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics
Volume682
Issue number1
DOIs
StatePublished - 23 Nov 2009
Externally publishedYes

Keywords

  • Area spectrum
  • Bekenstein-Hawking entropy
  • Quasinormal modes
  • de Sitter horizon

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