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Embedding of Galactic Systems in Extended Neutrino Clouds

Published online by Cambridge University Press:  04 August 2017

R. Cowsik
Affiliation:
Tata Institute of Fundamental Research, Homi Bhabha Road, BOMBAY 400 005, India
P. Ghosh
Affiliation:
Tata Institute of Fundamental Research, Homi Bhabha Road, BOMBAY 400 005, India

Abstract

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In an expanding universe neutrinos of mass 10eV form condensates with typical mass 1016 M and size ∼0.5 Mpc. Visible matter like galaxies and stars are embedded in these and assuming a Maxwellian distribution and collisionless nature of these systems we solve the self consistent Poisson-Vlasov equations. These solutions correctly predict the profiles of luminosity of clusters of galaxies, dwarf, elliptic and spiral galaxies as well as their rotation curves; the embedding picture is supported by M∼R33 relation for astronomical systems as below.

Type
Research Article
Copyright
Copyright © Reidel 1987