Kaluza-Klein-Casimir cosmology with decoupled heavy modes

E. I. Guendelman

doi:10.1016/0370-2693(88)90076-7

Kaluza-Klein-Casimir cosmology with decoupled heavy modes

E. I. Guendelman

Department of Physics

Research output: Contribution to journal › Article › peer-review

5 Scopus citations

Abstract

In a cosmological setting, Kaluza-Klein heavy modes can decouple. One can then treat them as "dust" in a 4D effective picture, even when these particles are massless from a higher dimensional point of view. We find cosmological solutions with decoupled heavy modes considering toroidal compactification for the extra dimensions and also the Casimir effect induced by the compactification.

Original language	English
Pages (from-to)	39-41
Number of pages	3
Journal	Physics Letters B
Volume	201
Issue number	1
DOIs	https://doi.org/10.1016/0370-2693(88)90076-7
State	Published - 28 Jan 1988

ASJC Scopus subject areas

Nuclear and High Energy Physics

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abstract = "In a cosmological setting, Kaluza-Klein heavy modes can decouple. One can then treat them as {"}dust{"} in a 4D effective picture, even when these particles are massless from a higher dimensional point of view. We find cosmological solutions with decoupled heavy modes considering toroidal compactification for the extra dimensions and also the Casimir effect induced by the compactification.",

author = "Guendelman, {E. I.}",

note = "Funding Information: I want to thank Professor J. Bekenstein and M. Schiffer for conversations and R. Shaanan for typing this paper. This research has been supported in part by the Fund for Basic Research administered by the Israel Academy of Sciences.",

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N2 - In a cosmological setting, Kaluza-Klein heavy modes can decouple. One can then treat them as "dust" in a 4D effective picture, even when these particles are massless from a higher dimensional point of view. We find cosmological solutions with decoupled heavy modes considering toroidal compactification for the extra dimensions and also the Casimir effect induced by the compactification.

AB - In a cosmological setting, Kaluza-Klein heavy modes can decouple. One can then treat them as "dust" in a 4D effective picture, even when these particles are massless from a higher dimensional point of view. We find cosmological solutions with decoupled heavy modes considering toroidal compactification for the extra dimensions and also the Casimir effect induced by the compactification.

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Kaluza-Klein-Casimir cosmology with decoupled heavy modes

Abstract

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