A Time Varying Strong Coupling Constant as a Model of Inflationary Universe

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dc.creatorChamoun, N.
dc.creatorLandau, S. J.
dc.creatorVucetich, H.
dc.date2000-09-13
dc.date2004-09-17
dc.date.accessioned2026-07-25T17:53:03Z
dc.descriptionWe consider a scenario where the strong coupling constant was changing in the early universe. We attribute this change to a variation in the colour charge within a Bekenstein-like model. Treating the vacuum gluon condensate $<G^2>$ as a free paramete r, we could generate inflation with the required properties to solve the fluctuation and other standard cosmology problems. A possible approach to end the inflation is suggested.
dc.description11 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0009204
dc.identifierhttp://arxiv.org/abs/astro-ph/0009204
dc.identifier.urihttps://dspace.dare.co.zw/handle/123456789/51547
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleA Time Varying Strong Coupling Constant as a Model of Inflationary Universe
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