The Dynamics of the Formation of Degenerate Heavy Neutrino Stars
classification
🌌 astro-ph
keywords
formationheavyneutrinostarsalternativeblackbosecenters
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Through 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.
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