Spatially flat R-W cosmological model with massive scalar field

Details Spatially flat R-W cosmological model with massive scalar field Spatially flat R-W cosmological model with massive scalar field

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.161..181v&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 161, no. 1, Nov. 1989, p. 181-184.

Physics

3

Astronomical Models, Cosmology, Scalars, Field Theory (Physics), Hubble Constant, Klein-Gordon Equation, Mass, Relativistic Effects

Scientific paper

An exact solution for the spatially flat Robertson-Walker (R-W) cosmological model with massive scalar field is obtained, using Einstein's field equations in the presence of a cosmological constant. This solution varies in the sense that the Hubble parameter is epoch-dependent while it is epoch-independent in the solution obtained by Rao et al. (1976).

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