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Horndeski gravity without screening in binary pulsars

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arxiv 1811.05393 v1 pith:4QX3SLE4 submitted 2018-11-13 astro-ph.HE gr-qc

P.I.Dyadina , N.A.Avdeev , S.O.Alexeyev This is my paper · ORCID
classification astro-ph.HEgr-qc
keywords gravitybinaryhorndeskipulsarswithoutadditionbinariesbrans-dicke
verification ladder T0 review T1 audit T2 compute T3 formal
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We test the subclasses of Horndeski gravity without Vainshtein mechanism in the strong field regime of binary pulsars. We find the rate of energy losses via the gravitational radiation predicted by such theories and compare our results with observational data from quasi-circular binaries PSR J1738+0333, PSR J0737-3039, PSR J1012+5307. In addition, we consider few specific cases: the hybrid metric-Palatini f(R)-gravity and massive Brans-Dicke theory.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter

    hep-th 2023-05 unverdicted novelty 6.0 of 10

    Computes 1PN conservative dynamics for gravitational/EM/Proca fields and 2PN for scalar, plus radiation effects from axion-photon coupling at high PN orders in binary black hole systems with dark matter.

  2. Probing Massive Scalar Fields from a Pulsar in a Stellar Triple System

    gr-qc 2019-08 conditional novelty 6.0 of 10

    PSR J0337 timing bounds on equivalence-principle violation are translated into new constraints on massive scalar, axion, and dark-matter-mediator fifth forces, with the strongest limits on massive Brans-Dicke gravity ...

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