Solutions to Cosmological Problems with Energy Conservation and Varying c, G and Lambda

Abstract

The flatness and cosmological constant problems are solved with varying speed of light c, gravitational coupling strength G and cosmological parameter Lambda, by explicitly assuming energy conservation of observed matter. The present solution to the flatness problem is the same as the previous solution in which energy conservation was absent.

5 pages, Replaced with LaTex file with minor changes

References in corpus (1)

• Supergravity, D-brane Probes and thermal super Yang-Mills: a comparison

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