Inhomogeneities in a Friedmann universe

Details Inhomogeneities in a Friedmann universe Inhomogeneities in a Friedmann universe

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987stin...8911672t&link_type=abstract

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Physics

Cosmology, Einstein Equations, Inhomogeneity, Universe, Anisotropy, Density Distribution, Spheres, Symmetry, Time Dependence

Scientific paper

One of the outstanding problems in cosmology is the growth of inhomogeneities, which are characterized by an anisotropic pressure and density distribution. Following a method developed by McVittie (1967, 1968) it has been possible to find time-dependent spherically symmetric solutions of Einstein's field equations containing an arbitrary pressure and density distribution which connect smoothly to a Friedmann universe for any desired equation of state.

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