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Implications of the Neutron Star Merger GW170817 for Cosmological Scalar-Tensor Theories

Jeremy Sakstein and Bhuvnesh Jain
Phys. Rev. Lett. 119, 251303 – Published 18 December 2017
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Abstract

The LIGO and VIRGO Collaborations have recently announced the detection of gravitational waves from a neutron star–neutron star merger (GW170817) and the simultaneous measurement of an optical counterpart (the γ-ray burst GRB 170817A). The close arrival time of the gravitational and electromagnetic waves limits the difference in speed of photons and gravitons to be less than about 1 part in 1015. This has three important implications for cosmological scalar-tensor gravity theories that are often touted as dark energy candidates and alternatives to the Λ cold dark matter model. First, for the most general scalar-tensor theories—beyond Horndeski models—three of the five parameters appearing in the effective theory of dark energy can now be severely constrained on astrophysical scales; we present the results of combining the new gravity wave results with galaxy cluster observations. Second, the combination with the lack of strong equivalence principle violations exhibited by the supermassive black hole in M87 constrains the quartic galileon model to be cosmologically irrelevant. Finally, we derive a new bound on the disformal coupling to photons that implies that such couplings are irrelevant for the cosmic evolution of the field.

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  • Received 18 October 2017

DOI:https://doi.org/10.1103/PhysRevLett.119.251303

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & Astrophysics

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Reining in Alternative Gravity

Published 18 December 2017

Theorists have tightly constrained alternative theories of gravity using the recent joint detection of gravitational waves and light from a neutron star merger.

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Authors & Affiliations

Jeremy Sakstein* and Bhuvnesh Jain

  • Department of Physics and Astronomy, Center for Particle Cosmology, University of Pennsylvania, 209 South 33rd Street, Philadelphia, Pennsylvania 19104, USA

  • *sakstein@physics.upenn.edu
  • bjain@physics.upenn.edu

See Also

Strong Constraints on Cosmological Gravity from GW170817 and GRB 170817A

T. Baker, E. Bellini, P. G. Ferreira, M. Lagos, J. Noller, and I. Sawicki
Phys. Rev. Lett. 119, 251301 (2017)

Dark Energy after GW170817 and GRB170817A

Paolo Creminelli and Filippo Vernizzi
Phys. Rev. Lett. 119, 251302 (2017)

Dark Energy After GW170817: Dead Ends and the Road Ahead

Jose María Ezquiaga and Miguel Zumalacárregui
Phys. Rev. Lett. 119, 251304 (2017)

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Vol. 119, Iss. 25 — 22 December 2017

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