Cosmological fluctuations produced near a singularity

Details Cosmological fluctuations produced near a singularity Cosmological fluctuations produced near a singularity

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980mnras.192..663z&link_type=abstract

Monthly Notices of the Royal Astronomical Society, vol. 192, Sept. 1980, p. 663-667.

Mathematics

430

Cosmology, Field Theory (Physics), Galactic Evolution, Perturbation Theory, Singularity (Mathematics), Einstein Equations, Equations Of State, Metric Space, Radioactive Decay, Universe

Scientific paper

The perturbations of a uniform Friedmannian universe, leading to galaxy formation, are explained by the strings, formed during the symmetry loss of vacuum of a complex Higgs field with mass characteristic of grand unification. Difficulties are pointed out inherent to phase transition, particle decay and black hole evaporation as sources of growing perturbations.

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