A model to explain varying Lambda , G and sigma super(2) simultaneously

Models with varying cosmic parameters, which were earlier regarded constant, are getting attention. However, different models are usually invoked to explain the evolution of different parameters. We argue that whatever physical process is responsible for the evolution of one parameter, should also b...

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Bibliographic Details
Published inGeneral relativity and gravitation Vol. 37; no. 7; pp. 1305 - 1311
Main Author Vishwakarma, R G
Format Journal Article
LanguageEnglish
Published 01.07.2005
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Summary:Models with varying cosmic parameters, which were earlier regarded constant, are getting attention. However, different models are usually invoked to explain the evolution of different parameters. We argue that whatever physical process is responsible for the evolution of one parameter, should also be responsible for the evolution of others. This means that the different parameters are coupled together somehow. Based on this guiding principle, we investigate a Bianchi type I model with variable Lambda and G, in which Lambda , G and the shear parameter sigma super(2), all are coupled. It is interesting that the resulting model reduces to the FLRW model for large t with G approaching a constant.
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ISSN:0001-7701
1572-9532
DOI:10.1007/s10714-005-0113-0