Expressions for linearized perturbations in ideal-fluid cosmological models

Details Expressions for linearized perturbations in ideal-fluid cosmological models Expressions for linearized perturbations in ideal-fluid cosmological models

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phrvd..38.2399r&link_type=abstract

Physical Review D (Particles and Fields), Volume 38, Issue 8, 15 October 1988, pp.2399-2414

Mathematics

Logic

17

Scientific paper

We present closed-form solutions of the relativistic linear perturbation equations (in synchronous gauge) that govern the evolution of inhomogeneities in homogeneous, spatially flat, ideal-fluid, cosmological models. These expressions, which are valid for irregularities on any scale, allow one to analytically interpolate between the known approximate solutions which are valid at early times and at late times.

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