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Gravitational Collapse with Torsion and Universe in a Black Hole

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arxiv 2307.12190 v1 pith:XJRQZXJY submitted 2023-07-23 gr-qc astro-ph.CO

classification gr-qcastro-ph.CO
keywords universetorsionblackgravitationalholecollapsecreationcycle
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abstract

We consider gravitational collapse of a sphere of a fluid with torsion generated by spin, which forms a black hole. We use the Tolman metric and the Einstein$-$Cartan field equations with a relativistic spin fluid as a source. We show that gravitational repulsion of torsion prevents a singularity, replacing it with a nonsingular bounce. Quantum particle creation during contraction prevents shear from overcoming torsion. Particle creation during expansion can generate a finite period of inflation and produce large amounts of matter. The resulting closed universe on the other side of the event horizon may have several bounces. Such a universe is oscillatory, with each cycle larger than the preceding cycle, until it reaches a size at which dark energy dominates and expands indefinitely. Our universe might have therefore originated from a black hole existing in another universe.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Reheating chiral dynamos with spin-0 and massive spin-1 torsions via chiral asymmetry

    astro-ph.CO 2025-02 reject novelty 4.0 of 10

    Adding a constant torsion trace to the chiral dynamo equation produces exponential magnetic growth with a sign set by torsion chirality, but the supporting equations and headline field strengths are not reliable.

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