Solutions to the Friedmann equations with the Lambda-term for a dust-radiation universe

Details Solutions to the Friedmann equations with the Lambda-term for a dust-radiation universe Solutions to the Friedmann equations with the Lambda-term for a dust-radiation universe

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983azh....60..648k&link_type=abstract

(Astronomicheskii Zhurnal, vol. 60, July-Aug. 1983, p. 648-655) Soviet Astronomy (ISSN 0038-5301), vol. 27, July-Aug. 1983, p. 3

Astronomy and Astrophysics

Astronomy

Astronomical Models, Cosmic Dust, Cosmology, Universe, Constants, Radiation, Roots Of Equations

Scientific paper

The Friedmann equations with a Lambda term for a universe comprising dustlike matter and radiation are solved analytically, extending the investigation of Kharbediya (1976). The metric is written in conformal form in comoving coordinates, expressing the real time terms of the parameteric time for all signs of the space curvature and of Lambda. The solutions are expressed as elementary functions for type A1 or A2 models and as elliptical functions for type M1, M2, or O1 models.

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