Formation of Neutrino Stars from Cosmological Background Neutrinos

Details Formation of Neutrino Stars from Cosmological Background Neutrinos Formation of Neutrino Stars from Cosmological Background Neutrinos

2006-09-20

arxiv.org/abs/astro-ph/0609564v1

Astronomy and Astrophysics

Astrophysics

15 pages, 7 figures

Scientific paper

We study hydrodynamic evolution of cosmological background neutrinos. By using a spherically symmetric Newtonian hydrodynamic code, we calculate the time evolution of the density profiles of neutrino matter in cluster and galactic scales. We discuss the possible observational consequences of such evolution and the resulting density profiles of the degenerate neutrino `stars' in galaxies and clusters.

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