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  • 1
    Publication Date: 2011-08-19
    Description: 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.
    Keywords: ASTROPHYSICS
    Type: Physical Review Letters (ISSN 0031-9007); 62; 379-382
    Format: text
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