Power-law inflation satisfies Penrose’s Weyl curvature hypothesis

Guido D’Amico and Nemanja Kaloper
Phys. Rev. D 106, 103503 – Published 7 November 2022

Abstract

Based on entropy considerations and the arrow of time Penrose argued that the Universe must have started in a special initial singularity with vanishing Weyl curvature. This is often interpreted to be at odds with inflation. Here we argue just the opposite, that Penrose’s persuasions are in fact consistent with inflation. Using the example of power law inflation, we show that inflation begins with a past null singularity, where Weyl tensor vanishes when the metric is initially exactly conformally flat. This initial state precisely obeys Penrose’s conditions. The initial null singularity breaks T-reversal spontaneously and picks the arrow of time. It can be regulated and interpreted as a creation of a universe from nothing, initially fitting in a bubble of Planckian size when it materializes. Penrose’s initial conditions are favored by the initial O(4) symmetry of the bubble, selected by extremality of the regulated Euclidean action. The predicted observables are marginally in tension with the data, but they can fit if small corrections to power law inflation kick in during the last 60e-folds.

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  • Received 2 October 2022
  • Accepted 20 October 2022

DOI:https://doi.org/10.1103/PhysRevD.106.103503

© 2022 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsParticles & Fields

Authors & Affiliations

Guido D’Amico1,* and Nemanja Kaloper2,†

  • 1Dipartimento di SMFI dell’, Università di Parma and INFN, Gruppo Collegato di Parma, Italy
  • 2QMAP, Department of Physics and Astronomy, University of California Davis, California 95616, USA

  • *damico.guido@gmail.com
  • kaloper@physics.ucdavis.edu

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Issue

Vol. 106, Iss. 10 — 15 November 2022

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