Real no-boundary wave function in Lorentzian quantum cosmology

J. Diaz Dorronsoro, J. J. Halliwell, J. B. Hartle, T. Hertog, and O. Janssen
Phys. Rev. D 96, 043505 – Published 7 August 2017

Abstract

It is shown that the standard no-boundary wave function has a natural expression in terms of a Lorentzian path integral with its contour defined by Picard-Lefschetz theory. The wave function is real, satisfies the Wheeler-DeWitt equation and predicts an ensemble of asymptotically classical, inflationary universes with nearly-Gaussian fluctuations and with a smooth semiclassical origin.

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  • Received 23 June 2017

DOI:https://doi.org/10.1103/PhysRevD.96.043505

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

Authors & Affiliations

J. Diaz Dorronsoro1,*, J. J. Halliwell2,†, J. B. Hartle3,‡, T. Hertog1,§, and O. Janssen4,∥

  • 1Institute for Theoretical Physics, KU Leuven, 3001 Leuven, Belgium
  • 2Blackett Laboratory, Imperial College, London SW7 2BZ, United Kingdom
  • 3Department of Physics, UCSB, Santa Barbara, California 93106, USA
  • 4Center for Cosmology and Particle Physics, NYU, New York, New York 10003, USA

  • *juan.diaz@fys.kuleuven.be
  • j.halliwell@imperial.ac.uk
  • hartle@physics.ucsb.edu
  • §thomas.hertog@fys.kuleuven.be
  • opj202@nyu.edu

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Issue

Vol. 96, Iss. 4 — 15 August 2017

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