arXiv · gr-qc/9907003
Cosmological models with variable constants
Abstract
The behavior of the constants, G,c,h,a,e,m and Lambda, considering them as variable, in the framework of a flat cosmological model with FRW symmetries described by a bulk viscous fluid and considering mechanisms of adiabatic matter creation are investigated. Within two models; one with radiation predominance and another of matter predominance, this behavior are studied.
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J. A. Belinchon. 1999-11-19. Cosmological models with variable constants. https://doi.org/10.1023/a%3A1003644614145
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