Gravitational collapse of a fluid with torsion into a universe in a black hole

Abstract

We consider gravitational collapse of a spherically symmetric sphere of a fluid with spin and torsion into 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 and replaces it with a nonsingular bounce. Quantum particle production during contraction helps torsion to dominate over shear. Particle production during expansion can generate a finite period of inflation and produce enormous 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 in size than the previous cycle, until it reaches the cosmological size and expands indefinitely. Our universe might have therefore originated from a black hole.

8 pages; published version

References in corpus (4)

• Cosmology with torsion: An alternative to cosmic inflation
• Matter-antimatter asymmetry and dark matter from torsion
• Collapse and dispersal of a homogeneous spin fluid in Einstein-Cartan theory
• The Shape of Bouncing Universes

Cited by in corpus (5)

• Imprints of dark matter on the structural properties of minimally deformed compact stars
• Completely Deformed Complexity-free Anisotropic Fluid Sphere
• Conundrum of regular black holes with nonlinear electromagnetic fields
• General-relativistic wave$-$particle duality with torsion
• Master equations governing the coupling between spin-currents and gravity