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Phase transitions in cosmological models: Temperature vs. curvature

✍ Scribed by H. Fleming; V. L. R. da Silveira

Book ID
112922644
Publisher
Springer-Verlag,Italian Physical Society
Year
1980
Weight
266 KB
Volume
58
Category
Article
ISSN
0369-3554

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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