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Trapping the Kaluza-Klein scalar

Journal Article · · General Relativity and Gravitation; (United States)
DOI:https://doi.org/10.1007/BF00762293· OSTI ID:5439382
The Kaluza-Klein unified theory predicts the existence of a Brans-Dicke type scalar field with {omega} = 0. Solar system experiments do, however, imply that gravitational scalar fields must be suppressed either by a very weak coupling to matter ({omega} > 500) or a self-interaction. Here the consequences of a self-interaction potential of the Kaluza-Klein scalar are investigated. By suppressing the scalar field in this way, the one-body metric reduces to the Schwarzschild solution. The cosmologies of the scalar-tensor model are, however, very different from cosmologies of Einstein's theory, since here the time evolution of the cosmic scale-factor is determined only by the initial conditions. These may be chosen so that the theory is compatible with the hypothesis of primordial nucleosynthesis.
OSTI ID:
5439382
Journal Information:
General Relativity and Gravitation; (United States), Journal Name: General Relativity and Gravitation; (United States) Vol. 23:3; ISSN 0001-7701; ISSN GRGVA
Country of Publication:
United States
Language:
English