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New Solutions for Evolution of the Scale Factor with a Variable Cosmological Term

High Energy Physics - Theory 2007-05-23 v1

Abstract

The cosmological term is assumed to be a function of time such as Λ=Ba2\Lambda =Ba^{-2} where a(t) means the scale factor of standard cosmology. Analytical solutions for radiation dominated epoch and open universe are found. For closed universe, k=+1, and for flat universe, k=0, we show a numerical solution. In general the scenario of Big Bang is preserved in our case for the Friedmann-Robertson-Walker cosmology.

Keywords

Cite

@article{arxiv.hep-th/0006174,
  title  = {New Solutions for Evolution of the Scale Factor with a Variable Cosmological Term},
  author = {Carlos Pinheiro and F. C. Khanna},
  journal= {arXiv preprint arXiv:hep-th/0006174},
  year   = {2007}
}

Comments

1 figure can be asked to the authors, 7 pages, AMStex

R2 v1 2026-07-22T14:58:40.577Z