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.

15 pages. submitted to IJTP

References in corpus (1)

• Cosmological models with bulk viscosity in presence of adiabatic matter creation and with G, c and Lambda variables

Cited by in corpus (5)

• The minimally extended Varying Speed of Light (meVSL)
• Quantization of Gravitational System and its Cosmological Consequences
• A Theory of time-varying Constants
• Revisiting Varying Speed of Light in Cosmology: Insights from the Friedmann-Lemaître-Robertson-Walker Metric
• Perturbation Theory in the Minimally Extended Varying Speed of Light (meVSL) Model