Clustering of cosmological defects at the time of formation

Details Clustering of cosmological defects at the time of formation Clustering of cosmological defects at the time of formation

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phlb..260...27l&link_type=abstract

Physics Letters B, Volume 260, Issue 1-2, p. 27-31.

Physics

11

Scientific paper

A simple model for the formation of global monopoles is considered. It is shown that they naturally form in clusters, with monopoles adjacent to antimonopoles, and vice-versa. The strong attraction between pole and antipole causes the clusters to collapse very rapidly, leading to the annihilation of most (62% in our model) of the original defects within a time τ, where τ is of the order of the correlation length.

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