Massive Neutrinos and the Large-Scale Structure of the Universe

J. R. Bond, G. Efstathiou, and J. Silk
Phys. Rev. Lett. 45, 1980 – Published 15 December 1980
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Abstract

If neutrinos dominate the mass density of the Universe, they play a critical role in the gravitational instability theory of galaxy formation. For neutrinos of mass 30m30 eV, a maximum Jeans mass Mνm4×1015m302M is derived. On smaller scales, neutrino fluctuations are damped, and the growth of baryon fluctuations is greatly inhibited. Structures on scales >Mνm may collapse, forming galaxies as in Zel'dovich's "pancake" theory.

  • Received 9 July 1980

DOI:https://doi.org/10.1103/PhysRevLett.45.1980

©1980 American Physical Society

Authors & Affiliations

J. R. Bond, G. Efstathiou, and J. Silk

  • Astronomy Department, University of California, Berkeley, California 94720

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Issue

Vol. 45, Iss. 24 — 15 December 1980

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