The Dynamics of the Formation of Degenerate Heavy Neutrino Stars

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dc.creatorBilic, Neven
dc.creatorLindebaum, Robert J.
dc.creatorTupper, Gary B.
dc.creatorViollier, Raoul D.
dc.date2000-08-16
dc.date2001-07-27
dc.date.accessioned2026-07-07T01:54:56Z
dc.date.available2026-07-07T01:54:56Z
dc.descriptionThrough reformulating the cold, self-gravitating fermion gas as a Bose condensate by identifying their mutual Thomas-Fermi limits, the dissipationless formation of a heavy neutrino star in gravitational collapse is numerically demonstrated. Such stars offer an alternative to supermassive black holes for the compact dark objects at the centers of galaxies.
dc.description4 pages, 2 figures, Minor changes only
dc.identifierhttps://arxiv.org/abs/astro-ph/0008230
dc.identifierhttp://arxiv.org/abs/astro-ph/0008230
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1484
dc.subjectAstrophysics
dc.titleThe Dynamics of the Formation of Degenerate Heavy Neutrino Stars
dc.typetext

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