Big bounce and inflation from spin and torsion, N. Poplawski
Room: 100
616-10 Beechwood Pl
London, ON
Department of Physics and Astronomy
PHYSICS & ASTRONOMY COLLOQUIUM
Dr. Nikodem Poplawski
Department of Mathematics and Physics
University of New Haven, CT
“Big bounce and inflation from spin and torsion”
ABSTRACT
The conservation law for the total (orbital plus spin) angular momentum of a Dirac particle in the presence of gravity requires that spacetime is not only curved, but also has a nonzero torsion. The coupling between the spin and torsion in the Einstein–Cartan theory of gravity generates gravitational repulsion at extremely high densities, which prevents a singularity in a black hole and may create there a new, closed, baby universe undergoing one or more nonsingular bounces. We show that quantum particle production caused by an extremely high curvature near a bounce creates enormous amounts of matter and can generate a finite period of inflation. Our scenario has only one parameter, does not depend significantly on the initial conditions, does not involve hypothetical scalar fields, avoids eternal inflation, and predicts plateau-like inflation that is supported by the Planck observations of the cosmic microwave background. This scenario suggests that our Universe may have originated from a nonsingular bounce in a black hole existing in another universe.