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Time variation of G and α within models with extra dimensions

P Lorén-Aguilar1, E García-Berro1,2, J Isern2,3 and Yu A Kubyshin4,5

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We derive the formulae for the time variation of the gravitational 'constant' G and of the fine structure 'constant' α in various models with extra dimensions and analyse their consistency with the available observational data for distant supernovae. We find that the reported variation of α translates into a small variation of G that makes distant supernovae to appear brighter, in contrast to recent observations of high z supernovae. The significance of these results within the framework of some cosmological scenarios is also discussed. We find, however, that the magnitude of the effect is not large enough to safely discard the models with extra dimensions studied here.


PACS

04.50.-h Higher-dimensional gravity and other theories of gravity

98.80.-k Cosmology

97.60.Bw Supernovae

MSC

83F05 Cosmology

83E15 Kaluza-Klein and other higher-dimensional theories

Subjects

Gravitation and cosmology

Astrophysics and astroparticles

Dates

Issue 18 (21 September 2003)

Received 26 February 2003, in final form 30 May 2003

Published 20 August 2003



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