pith. sign in

arxiv: 1811.05393 · v1 · pith:4QX3SLE4new · submitted 2018-11-13 · 🌌 astro-ph.HE · gr-qc

Horndeski gravity without screening in binary pulsars

P.I.Dyadina , N.A.Avdeev , S.O.Alexeyev This is my paper
classification 🌌 astro-ph.HE gr-qc
keywords gravitybinaryhorndeskipulsarswithoutadditionbinariesbrans-dicke
0
0 comments X
read the original abstract

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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

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

  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

    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.