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Author Danielsson, Ulf H.
Source arXiv.org
Content type Text
File Format PDF
Date of Submission 2002-05-22
Language English
Subject Domain (in DDC) Computer science, information & general works ♦ Natural sciences & mathematics ♦ Physics
Subject Keyword High Energy Physics - Theory ♦ physics:hep-th
Abstract A family of de Sitter vacua introduced in hep-th/0203198 as plausible initial conditions for inflation, are discussed from the point of view of de Sitter holography. The vacua are argued to be physically acceptable and the inflationary picture provides a physical interpretation of a subfamily of de Sitter invariant vacua. Some speculations on the issue of vacuum choice and the connection between the CMBR and holography are also provided.
Description Reference: JHEP 0207 (2002) 040
Educational Use Research
Learning Resource Type Article
Page Count 16


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