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Critical geometry of a thermal big bang

Niayesh Afshordi and João Magueijo
Phys. Rev. D 94, 101301(R) – Published 18 November 2016
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Abstract

We explore the space of scalar-tensor theories containing two nonconformal metrics, and find a discontinuity pointing to a “critical” cosmological solution. Due to the different maximal speeds of propagation for matter and gravity, the cosmological fluctuations start off inside the horizon even without inflation, and will more naturally have a thermal origin (since there is never vacuum domination). The critical model makes an unambiguous, nontuned prediction for the spectral index of the scalar fluctuations: nS=0.96478(64). Considering also that no gravitational waves are produced, we have unveiled the most predictive model on offer. The model has a simple geometrical interpretation as a probe 3-brane embedded in an EAdS2×E3 geometry.

  • Received 10 March 2016

DOI:https://doi.org/10.1103/PhysRevD.94.101301

© 2016 American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
Gravitation, Cosmology & Astrophysics

Authors & Affiliations

Niayesh Afshordi

  • Perimeter Institute for Theoretical Physics, 31 Caroline Street North, Waterloo, Ontario N2L 2Y5, Canada and Department of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1, Canada

João Magueijo

  • Theoretical Physics, Blackett Laboratory, Imperial College, London SW7 2BZ, United Kingdom

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Issue

Vol. 94, Iss. 10 — 15 November 2016

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