Formation of Neutrino Stars from Cosmological Background Neutrinos

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dc.creatorChan, M. H.
dc.creatorChu, M. -C.
dc.date2006-09-20
dc.date.accessioned2026-07-07T07:23:18Z
dc.date.available2026-07-07T07:23:18Z
dc.descriptionWe 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.
dc.description15 pages, 7 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0609564
dc.identifierhttp://arxiv.org/abs/astro-ph/0609564
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/115929
dc.subjectAstrophysics
dc.titleFormation of Neutrino Stars from Cosmological Background Neutrinos
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