The speed of Galileon gravity

We analyse the speed of gravitational waves in coupled Galileon models with an equation of state ωphgr=−1 now and a ghost-free Minkowski limit. We find that the gravitational waves propagate much faster than the speed of light unless these models are small perturbations of cubic Galileons and the Ga...

Full description

Bibliographic Details
Main Authors: Brax, Philippe, Burrage, Clare, Davis, Anne-Christine
Format: Article
Published: IOPScience 2016
Subjects:
Online Access:https://eprints.nottingham.ac.uk/42092/
_version_ 1848796416688783360
author Brax, Philippe
Burrage, Clare
Davis, Anne-Christine
author_facet Brax, Philippe
Burrage, Clare
Davis, Anne-Christine
author_sort Brax, Philippe
building Nottingham Research Data Repository
collection Online Access
description We analyse the speed of gravitational waves in coupled Galileon models with an equation of state ωphgr=−1 now and a ghost-free Minkowski limit. We find that the gravitational waves propagate much faster than the speed of light unless these models are small perturbations of cubic Galileons and the Galileon energy density is sub-dominant to a dominant cosmological constant. In this case, the binary pulsar bounds on the speed of gravitational waves can be satisfied and the equation of state can be close to -1 when the coupling to matter and the coefficient of the cubic term of the Galileon Lagrangian are related. This severely restricts the allowed cosmological behaviour of Galileon models and we are forced to conclude that Galileons with a stable Minkowski limit cannot account for the observed acceleration of the expansion of the universe on their own. Moreover any sub-dominant Galileon component of our universe must be dominated by the cubic term. For such models with gravitons propagating faster than the speed of light, the gravitons become potentially unstable and could decay into photon pairs. They could also emit photons by Cerenkov radiation. We show that the decay rate of such speedy gravitons into photons and the Cerenkov radiation are in fact negligible. Moreover the time delay between the gravitational signal and light emitted by explosive astrophysical events could serve as a confirmation that a modification of gravity acts on the largest scales of the Universe.
first_indexed 2025-11-14T19:47:38Z
format Article
id nottingham-42092
institution University of Nottingham Malaysia Campus
institution_category Local University
last_indexed 2025-11-14T19:47:38Z
publishDate 2016
publisher IOPScience
recordtype eprints
repository_type Digital Repository
spelling nottingham-420922020-05-04T17:42:48Z https://eprints.nottingham.ac.uk/42092/ The speed of Galileon gravity Brax, Philippe Burrage, Clare Davis, Anne-Christine We analyse the speed of gravitational waves in coupled Galileon models with an equation of state ωphgr=−1 now and a ghost-free Minkowski limit. We find that the gravitational waves propagate much faster than the speed of light unless these models are small perturbations of cubic Galileons and the Galileon energy density is sub-dominant to a dominant cosmological constant. In this case, the binary pulsar bounds on the speed of gravitational waves can be satisfied and the equation of state can be close to -1 when the coupling to matter and the coefficient of the cubic term of the Galileon Lagrangian are related. This severely restricts the allowed cosmological behaviour of Galileon models and we are forced to conclude that Galileons with a stable Minkowski limit cannot account for the observed acceleration of the expansion of the universe on their own. Moreover any sub-dominant Galileon component of our universe must be dominated by the cubic term. For such models with gravitons propagating faster than the speed of light, the gravitons become potentially unstable and could decay into photon pairs. They could also emit photons by Cerenkov radiation. We show that the decay rate of such speedy gravitons into photons and the Cerenkov radiation are in fact negligible. Moreover the time delay between the gravitational signal and light emitted by explosive astrophysical events could serve as a confirmation that a modification of gravity acts on the largest scales of the Universe. IOPScience 2016-03-04 Article PeerReviewed Brax, Philippe, Burrage, Clare and Davis, Anne-Christine (2016) The speed of Galileon gravity. Journal of Cosmology and Astroparticle Physics, 2016 (03). 004/1-004/17. ISSN 1475-7516 dark energy theory gravitational waves / theory modified gravity http://iopscience.iop.org/article/10.1088/1475-7516/2016/03/004/meta doi:10.1088/1475-7516/2016/03/004 doi:10.1088/1475-7516/2016/03/004
spellingShingle dark energy theory
gravitational waves / theory
modified gravity
Brax, Philippe
Burrage, Clare
Davis, Anne-Christine
The speed of Galileon gravity
title The speed of Galileon gravity
title_full The speed of Galileon gravity
title_fullStr The speed of Galileon gravity
title_full_unstemmed The speed of Galileon gravity
title_short The speed of Galileon gravity
title_sort speed of galileon gravity
topic dark energy theory
gravitational waves / theory
modified gravity
url https://eprints.nottingham.ac.uk/42092/
https://eprints.nottingham.ac.uk/42092/
https://eprints.nottingham.ac.uk/42092/