The speed of Galileon gravity
TLDR
In this article, the authors analyzed the speed of gravitational waves in coupled Galileon models with an equation of state ωphgr=−1 now and a ghost-free Minkowski limit.Abstract:
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.read more
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Journal ArticleDOI
Strong Constraints on Cosmological Gravity from GW170817 and GRB 170817A.
TL;DR: It is shown that the detection of an electromagnetic counterpart to the gravitational-wave signal from the merger of two neutron stars allows for stringent constraints on general scalar-tensor and vector-Tensor theories, while allowing for an independent bound on the graviton mass in bimetric theories of gravity.
Journal ArticleDOI
Dark Energy after GW170817 and GRB170817A
TL;DR: The observation of GW170817 and its electromagnetic counterpart implies that gravitational waves travel at the speed of light, with deviations smaller than a few×10−15, and it is shown that the deduced relations among operators do not introduce further tuning of the models, since they are stable under quantum corrections.
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Tests of chameleon gravity
Clare Burrage,Jeremy Sakstein +1 more
TL;DR: A review of the state-of-the-art searches for screened scalars coupled to matter can be found in this article, where the authors summarize the results of these searches and discuss the future prospects for constraining screened modified gravity models further using upcoming and planned experiments.
Journal ArticleDOI
Galileon gravity in light of ISW, CMB, BAO and H 0 data
Janina J. Renk,Miguel Zumalacárregui,Miguel Zumalacárregui,Francesco Montanari,Alexandre Barreira +4 more
TL;DR: Cosmological models with Galileon gravity are an alternative to the standard ACDM paradigm with testable predictions at the level of its self-accelerating solutions for the expansion history as discussed by the authors.
Journal ArticleDOI
Dark Energy in Light of Multi-Messenger Gravitational-Wave Astronomy
TL;DR: Ezquiaga and Zumalacarregui as mentioned in this paper reviewed the different ways in which Gravitational Wave (GW) can be used to test gravity and models for late-time cosmic acceleration.
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