Simulation of gravitational superclustering of massive neutrinos

Details Simulation of gravitational superclustering of massive neutrinos Simulation of gravitational superclustering of massive neutrinos

Mar 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982phrvl..48..894m&link_type=abstract

Physical Review Letters, vol. 48, Mar. 29, 1982, p. 894-896.

Physics

45

Computerized Simulation, Cosmology, Gravitational Effects, Neutrinos, Particle Mass, Particle Motion, Galactic Evolution, Perturbation Theory

Scientific paper

Results of a numerical simulation of large-scale, plane, symmetric gravitational clustering of massive neutrinos are presented. It is shown that neutrinos may cluster in galactic halos in the adiabatic scenario of galaxy formation. The population of test particles exhibits very little phase mixing, suggesting that the scale of galactic halos may be set by the neutrino mass.

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