Formation of large-scale structure from cosmic strings and massive neutrinos

Details Formation of large-scale structure from cosmic strings and massive neutrinos Formation of large-scale structure from cosmic strings and massive neutrinos

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989phrvl..62..379s&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 62, Jan. 23, 1989, p. 379-382. Research supported by NASA and NSF.

Statistics

Computation

46

Astronomical Models, Computational Astrophysics, Cosmology, Neutrinos, String Theory, Dark Matter, Galactic Evolution, Gravitation Theory, Particle Mass

Scientific paper

Numerical simulations of large-scale structure formation from cosmic strings and massive neutrinos are described. The linear power spectrum in this model resembles the cold-dark-matter power spectrum. Galaxy formation begins early, and the final distribution consists of isolated density peaks embedded in a smooth background, leading to a natural bias in the distribution of luminous matter. The distribution of clustered matter has a filamentary appearance with large voids.

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