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Cosmic strings with self-interacting hot dark matter
Authors:P. P. Avelino,&   J. P. M. de Carvalho
Affiliation:Centro de Astrofísica da Univ. do Porto, Rua do Campo Alegre 823, 4150 Porto, Portugal,;Dep. de Matemática Aplicada da Faculdade de Ciências da Univ. do Porto, Rua das Taipas 135, 4050 Porto, Portugal
Abstract:We compute the linear power spectrum of cosmic-string-seeded fluctuations in the context of neutrinos with a strong self-interaction and show that it is very similar to that obtained in the context of 'normal' neutrinos. We compare our results with observational data and show that for any value of the cosmological parameters h and Ω0 the interacting hot dark matter power spectrum requires a scale-dependent biasing parameter.
Keywords:cosmic strings    galaxies: clusters: general — dark matter — large-scale structure of Universe
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