A plane symmetric cosmological model in Lyra manifold

Details A plane symmetric cosmological model in Lyra manifold A plane symmetric cosmological model in Lyra manifold

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.123...49r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 123, no. 1, June 1986, p. 49-52.

Astronomy and Astrophysics

Astrophysics

24

Astronomical Models, Cosmology, Lyra Constellation, Riemann Manifold, Flux Density, Ideal Fluids, Pressure Distribution, Space-Time Functions, Stellar Gravitation

Scientific paper

A non-static plane-symmetric cosmological model in Lyra's manifold is
obtained when the source of the gravitational field is a perfect fluid
with pressure equal to energy density. Some properties of the model have
also been discussed.

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