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New coordinates for de Sitter space and de Sitter radiation

2002/04/30 by Maulik Parikh, Maulik K. Parikh · 9 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Quantum Electrodynamics and Casimir Effect #gr-qc #hep-th

paper · pdf · doi:10.1016/s0370-2693(02)02701-6

published as Phys.Lett.B546:189-195,2002 · LaTeX, 10 pages; v2. references added; v3. minor sign errors fixed, reference added, journal version

openalex publication_date 2002/10/01 · arxiv created 2002/10/02 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/02

Abstract

We introduce a simple coordinate system covering half of de Sitter space. The new coordinates have several attractive properties: the time direction is a Killing vector, the metric is smooth at the horizon, and constant-time slices are just flat Euclidean space. We demonstrate the usefulness of the coordinates by calculating the rate at which particles tunnel across the horizon. When self-gravitation is taken into account, the resulting tunneling rate is only approximately thermal. The effective temperature decreases through the emission of radiation.

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