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The horizon problem in Friedmann-Robertson-Walker cosmology

✍ Scribed by Sofiane Cliallane-Tlemsani

Publisher
Springer US
Year
1993
Tongue
English
Weight
379 KB
Volume
25
Category
Article
ISSN
0001-7701

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We consider one-soliton perturbations of a flat Fricdmann-Robertson-Walker (FRW) cosmological model, with an ideal fluid with pressure equal to the cmrgy density (stiff fluid), in the case when the "pok trajactory" parameter is negative. introducing thenby singularitics along certain null h ypersurf