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Hydrogen Burning in Low Mass Stars Constrains Scalar-Tensor Theories of Gravity

Jeremy Sakstein
Phys. Rev. Lett. 115, 201101 – Published 10 November 2015

Abstract

The most general scalar-tensor theories of gravity predict a weakening of the gravitational force inside astrophysical bodies. There is a minimum mass for hydrogen burning in stars that is set by the interplay of plasma physics and the theory of gravity. We calculate this for alternative theories of gravity and find that it is always significantly larger than the general relativity prediction. The observation of several low mass red dwarf stars therefore rules out a large class of scalar-tensor gravity theories and places strong constraints on the cosmological parameters appearing in the effective field theory of dark energy.

  • Figure
  • Received 26 June 2015

DOI:https://doi.org/10.1103/PhysRevLett.115.201101

© 2015 American Physical Society

Authors & Affiliations

Jeremy Sakstein*

  • Institute of Cosmology and Gravitation, University of Portsmouth, Portsmouth PO1 3FX, United Kingdom

  • *jeremy.sakstein@port.ac.uk

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Issue

Vol. 115, Iss. 20 — 13 November 2015

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