Lorentzian quantum cosmology

Job Feldbrugge, Jean-Luc Lehners, and Neil Turok
Phys. Rev. D 95, 103508 – Published 16 May 2017

Abstract

We argue that the Lorentzian path integral is a better starting point for quantum cosmology than its Euclidean counterpart. In particular, we revisit the minisuperspace calculation of the Feynman path integral for quantum gravity with a positive cosmological constant. Instead of rotating to Euclidean time, we deform the contour of integration over metrics into the complex plane, exploiting Picard-Lefschetz theory to transform the path integral from a conditionally convergent integral into an absolutely convergent one. We show that this procedure unambiguously determines which semiclassical saddle point solutions are relevant to the quantum mechanical amplitude. Imposing “no-boundary” initial conditions, i.e., restricting attention to regular, complex metrics with no initial boundary, we find that the dominant saddle contributes a semiclassical exponential factor which is precisely the inverse of the famous Hartle-Hawking result.

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  • Received 22 March 2017

DOI:https://doi.org/10.1103/PhysRevD.95.103508

© 2017 American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Job Feldbrugge1,*, Jean-Luc Lehners2,†, and Neil Turok1,‡

  • 1Perimeter Institute, 31 Caroline Street N, Waterloo, Ontario N2L 2Y5, Canada
  • 2Max-Planck-Institute for Gravitational Physics (Albert-Einstein-Institute), 14476 Potsdam, Germany

  • *jfeldbrugge@perimeterinstitute.ca
  • jlehners@aei.mpg.de
  • nturok@perimeterinstitute.ca

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Issue

Vol. 95, Iss. 10 — 15 May 2017

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