Abstract
Formation and evolution of the large-scale structure of galaxy distribution in unstable dark matter (UDM) models are discussed. Epoch of galaxy formation which for stable neutrino models (m = 30 eV) was too late (z = 0.5 – 1) for UDM models (m = 50 – 100 eV) goes to z = 3 if products of decays are relativistic at present or at least to z= 7 – 10 if the products are nonrelativistic.
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© 1989 Kluwer Academic Publishers
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Klypin, A.A., Doroshkevich, A.A. (1989). Galaxy Formation in Unstable Dark Matter Models. In: Frenk, C.S., Ellis, R.S., Shanks, T., Heavens, A.F., Peacock, J.A. (eds) The Epoch of Galaxy Formation. NATO ASI Series, vol 264. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0919-9_37
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DOI: https://doi.org/10.1007/978-94-009-0919-9_37
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