Initial monopole density in an inflationary Universe

Details Initial monopole density in an inflationary Universe Initial monopole density in an inflationary Universe

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001cqgra..18.3019d&link_type=abstract

Classical and Quantum Gravity, Volume 18, Issue 15, pp. 3019-3024 (2001).

Mathematics

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1

Scientific paper

Non-equilibrium dynamics leading to the formation of topological defects
in a symmetry-breaking phase transition is studied. In a spatially flat
inflationary Universe an initial number density of monopoles as a
function of metric characteristic is estimated.

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