Self-gravitating fermions in general relativity show phase transitions from a gas to a condensed fermion ball, with a further collapse to a black hole above the Oppenheimer-Volkoff limit.
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Gravitational phase transitions and instabilities of self-gravitating fermions in general relativity
Self-gravitating fermions in general relativity show phase transitions from a gas to a condensed fermion ball, with a further collapse to a black hole above the Oppenheimer-Volkoff limit.