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Duality invariant cosmology to all orders in α

Olaf Hohm and Barton Zwiebach
Phys. Rev. D 100, 126011 – Published 10 December 2019

Abstract

While the classification of α corrections of string inspired effective theories remains an unsolved problem, we show how to classify duality invariant α corrections for purely time-dependent (cosmological) backgrounds. We determine the most general duality invariant theory to all orders in α for the metric, b-field, and dilaton. The resulting Friedmann equations are studied when the spatial metric is a time-dependent scale factor times the Euclidean metric and the b-field vanishes. These equations can be integrated perturbatively to any order in α. We construct nonperturbative solutions and display duality invariant theories featuring string-frame de Sitter vacua.

  • Received 14 June 2019

DOI:https://doi.org/10.1103/PhysRevD.100.126011

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsParticles & Fields

Authors & Affiliations

Olaf Hohm1 and Barton Zwiebach2

  • 1Institute for Physics, Humboldt University Berlin, Zum Großen Windkanal 6, D-12489 Berlin, Germany
  • 2Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA

Article Text

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Issue

Vol. 100, Iss. 12 — 15 December 2019

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