Dec 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phla..142..338b&link_type=abstract
Physics Letters A, Volume 142, Issue 6-7, p. 338-340.
Physics
2
Scientific paper
We solve the Einstein equations, considering a non-null cosmological constant, non-null tricurvature, a large variety of equations of state represented by p = αρ (α = const), for a perfect fluid and the Robertson-Walker metric. Though some of the formulae obtained were already identified as solutions of particular cases, it is the first time that the general case is being solved. We find also that the specific equation of state only matters for the early phase of the universe.
Samuel Berman Marcelo
Som Murari M.
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