With the use of the Newman-Penrose spin coefficients, the radial part of the electrom equation in the de Sitter-Schwarzschild space is separated, and the transmission coefftcient is calculated when the metric is specialized to the de Sitter case. Two different solutions of the radial equation are gi
โฆ LIBER โฆ
Density fluctuation in the de Sitter universe
โ Scribed by N Banerjee; S Mallik
- Publisher
- Elsevier Science
- Year
- 1991
- Tongue
- English
- Weight
- 919 KB
- Volume
- 205
- Category
- Article
- ISSN
- 0003-4916
No coin nor oath required. For personal study only.
โฆ Synopsis
A scalar Higgs field theory in de Sitter space-time has been investigated using the real time formulation of Semenoff and Weiss. We calculate the two-point function at late times and use it to obtain a general expression for the amplitude of fluctuation in energy density on scales which come out of the de Sitter horizon.
cc' 1991 Academic Press, Inc.
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