Two-point correlation function of cosmic-string loops

Details Two-point correlation function of cosmic-string loops Two-point correlation function of cosmic-string loops

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvl..63.1334b&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 63, Sept. 25, 1989, p. 1334-1337.

Physics

10

Cosmology, Galactic Clusters, Center Of Mass, Correlation, Galactic Evolution

Scientific paper

The two-point correlations of cosmic-string loops are studied with numerical simulations of the evolution of a cosmic-string network in an expanding universe. It is found that the initial positions of loops that are chopped off the network have a correlation function that is quite similar to the highest estimates of the Abell-cluster correlation function, but these correlations are rapidly washed out by the motion of the loops. The implications for the cosmic-string galaxy-formation scenario are briefly discussed.

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