pith. machine review for the scientific record. sign in

arxiv: 1711.06661 · v2 · submitted 2017-11-17 · 🌌 astro-ph.CO · gr-qc· hep-th

Recognition: unknown

Vainshtein mechanism after GW170817

Authors on Pith no claims yet
classification 🌌 astro-ph.CO gr-qchep-th
keywords theoryorderhorndeskimechanismtheoriesvainshteinequationsgravitational
0
0 comments X
read the original abstract

The almost simultaneous detection of gravitational waves and a short gamma-ray burst from a neutron star merger has put a tight constraint on the difference between the speed of gravity and light. In the four-dimensional scalar-tensor theory with second order equations of motion, the Horndeski theory, this translates into a significant reduction of the viable parameter space of the theory. Recently, extensions of Horndeski theory, which are free from Ostrogradsky ghosts despite the presence of higher order derivatives in the equations of motion, have been identified and classified exploiting the degeneracy criterium. In these new theories, the fifth force mediated by the scalar field must be suppressed in order to evade the stringent Solar System constraints. We study the Vainshtein mechanism in the most general degenerate higher order scalar-tensor theory in which light and gravity propagate at the same speed. We find that the Vainshtein mechanism generally works outside a matter source but it is broken inside matter, similarly to beyond Horndeski theories. This leaves interesting possibilities to test these theories that are compatible with gravitational wave observations using astrophysical objects.

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 2 Pith papers

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

  1. A Master Equation for Screening in Luminal Horndeski Gravity

    gr-qc 2026-05 unverdicted novelty 7.0

    A master screening equation is derived for luminal Horndeski gravity that recovers Vainshtein and Chameleon mechanisms and introduces Phaedrus screening with screening radius scaling linearly with source mass.

  2. Spherical collapse and cluster number counts in DHOST theories that pass the constraints from gravitational waves

    astro-ph.CO 2026-05 unverdicted novelty 4.0

    In DHOST theories consistent with GW observations, deviations from GR suppress high-redshift galaxy cluster abundance relative to ΛCDM when using spherical collapse and analytic mass functions matched to eROSITA data.