Singularity-free decaying-vacuum cosmologies: Evolution of density perturbations

Details Singularity-free decaying-vacuum cosmologies: Evolution of density perturbations Singularity-free decaying-vacuum cosmologies: Evolution of density perturbations

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvd..46.5675a&link_type=abstract

Physical Review D (Particles, Fields, Gravitation, and Cosmology), Volume 46, Issue 12, 15 December 1992, pp.5675-5677

Physics

5

Scientific paper

We discuss the growth of matter inhomogeneities in decaying-vacuum
cosmologies of an earlier paper. We find that linear density
perturbations evolve essentially as in the k=0 standard model.

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