REVIEW 1 cited by
No Run Gravity
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
abstract
Considering the dark energy/gravity landscape if next generation surveys of galaxies, cosmic microwave background radiation, and gravitational waves do not find clear modification of gravity, we develop No Run Gravity as a counterexample to the conclusion that this would imply general relativity with an expansion history described by an equation of state $w(z)$. No Run Gravity is a cubic Horndeski theory with a constant Planck mass, no gravitational slip, and no modification of gravitational waves, but a rich phenomenology beyond $w(z)$. We calculate the evolution of gravitational strength, sound speed, and cosmic growth within the theory and project sensitivities for upcoming DESI redshift space distortion data.
Forward citations
Cited by 1 Pith paper
-
A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events
Simulated bright siren events show LVK-era detections will not competitively constrain Horndeski gravity parameters, while one year of Einstein Telescope observations could detect αM ≠ 0 at over 3σ.
Discussion (0). Continue with ORCID to comment.