Evolution of inhomogeneous plane-symmetric cosmological models

Details Evolution of inhomogeneous plane-symmetric cosmological models Evolution of inhomogeneous plane-symmetric cosmological models

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978ncimb..44..372t&link_type=abstract

Nuovo Cimento, Sezione B, vol. 44B, Apr. 11, 1978, p. 372-380.

Physics

19

Astronomical Models, Cosmology, Einstein Equations, Space-Time Functions, Cosmic Dust, Density Distribution, Field Theory (Physics), Geodesy

Scientific paper

As models for the investigation of a plane-symmetric system and its evolution, solutions of Einstein's equations for dust with plane symmetry are studied. A new solution is found for a particular case; the solution depends on one arbitrary function which evolves to the open Robertson-Walker model as t approaches infinity. The function density on an initial spacelike hypersurface is an arbitrary function of z.

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