Cosmological model with Ω_M-dependent cosmological constant
classification
🌌 astro-ph
keywords
cosmologicalconstantmodelproportionalscalarstress-energytensorcosmical
read the original abstract
The idea here is to set the cosmical constant $\lambda$ proportional to the scalar of the stress-energy tensor of the ordinary matter. We investigate the evolution of the scale factor in a cosmological model in which the cosmological constant is proportional to the scalar of the stress-energy tensor.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.