R-W cosmological models with zero-mass scalar fields for different equations of state

Details R-W cosmological models with zero-mass scalar fields for different equations of state R-W cosmological models with zero-mass scalar fields for different equations of state

Nov 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.138..217r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 138, no. 1, Nov. 1987, p. 217-219.

Statistics

Computation

3

Charge Distribution, Cosmology, Equations Of State, Hubble Constant, Klein-Gordon Equation, Astronomical Models, Computational Astrophysics

Scientific paper

Spatially-flat cosmological models with interacting perfect fluid and
zero-mass scalar field have been obtained under different equations of
state and in presence of the scalar charge density associated with the
Klein-Gordon equation assuming a special law of variation for the
Hubble's parameter.

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