Primordial black holes, phase transitions, and the fate of the universe

Details Primordial black holes, phase transitions, and the fate of the universe Primordial black holes, phase transitions, and the fate of the universe

2000-03-05

arxiv.org/abs/astro-ph/0003062v1

Astronomy and Astrophysics

Astrophysics

3 pages LaTeX (prcrc.sty), 0 figures, pompous title, in Proceedings of the 3rd International Symposium on Sources and Detectio

Scientific paper

Phase transitions in the early universe are prime settings for the production of primordial black holes, since they can break the relatively quiescent homogeneity and isotropy of Friedmann-Robertson-Walker (FRW) cosmologies. These epochs of "symmetry breaking," moreover, can affect the subsequent development of spacetime by changing the evolution of some FRW parameters, including the present age and density of the universe. We discuss the relative importance of such effects on constraining mechanisms of black hole formation.

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