Polymer quantization of a self-gravitating thin shell

Jonathan Ziprick, Jack Gegenberg, and Gabor Kunstatter
Phys. Rev. D 94, 104076 – Published 30 November 2016

Abstract

We study the quantum mechanics of self-gravitating thin shell collapse by solving the polymerized Wheeler-DeWitt equation. We obtain the energy spectrum and solve the time-dependent equation using numerics. In contradistinction to the continuum theory, we are able to consistently quantize the theory for super-Planckian black holes, and find two choices of boundary conditions which conserve energy and probability, as opposed to one in the continuum theory. Another feature unique to the polymer theory is the existence of negative energy stationary states that disappear from the spectrum as the polymer scale goes to 0. In both theories the probability density is positive semidefinite only for the space of positive energy stationary states. Dynamically, we find that an initial Gaussian probability density develops regions of negative probability as the wave packet approaches R=0 and bounces. This implies that the bouncing state is a sum of both positive and negative eigenstates.

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  • Received 27 September 2016

DOI:https://doi.org/10.1103/PhysRevD.94.104076

© 2016 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Jonathan Ziprick*

  • Department of Mathematics and Statistics, University of New Brunswick, Fredericton, New Brunswick E3B 5A3, Canada

Jack Gegenberg

  • Department of Mathematics and Statistics and Department of Physics, University of New Brunswick, Fredericton, New Brunswick E3B 5A3, Canada

Gabor Kunstatter

  • Department of Physics and Winnipeg Institute for Theoretical Physics, University of Winnipeg, Winnipeg, Manitoba R3B 2E9, Canada

  • *jziprick@unb.ca
  • geg@unb.ca
  • g.kunstatter@uwinnipeg.ca

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Issue

Vol. 94, Iss. 10 — 15 November 2016

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