Stabilizing the Planck mass shortly after inflation

Carsten van de Bruck, Adam Christopherson, and Mathew Robinson
Phys. Rev. D 91, 123503 – Published 3 June 2015

Abstract

We consider a model of the early Universe which consists of two scalar fields: the inflaton and a second field which drives the stabilization of the Planck mass (or gravitational constant). We show that the nonminimal coupling of this second field to the Ricci scalar sources a nonadiabatic pressure perturbation. By performing a fully numerical calculation, we find, in turn, that this boosts the amplitude of the primordial power spectrum after inflation.

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  • Received 15 April 2015

DOI:https://doi.org/10.1103/PhysRevD.91.123503

© 2015 American Physical Society

Authors & Affiliations

Carsten van de Bruck1,*, Adam Christopherson2,†, and Mathew Robinson1,‡

  • 1Consortium for Fundamental Physics, School of Mathematics and Statistics, University of Sheffield, Hounsfield Road, Sheffield S3 7RH, United Kingdom
  • 2Department of Physics, University of Florida, Gainesville, Florida 32611, USA

  • *C.vandeBruck@sheffield.ac.uk
  • achristopherson@ufl.edu
  • app11mrr@sheffield.ac.uk

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Issue

Vol. 91, Iss. 12 — 15 June 2015

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