The Effect of Modified Gravity on the Odds of the Bound Violations of the Turn-Around Radii
Jounghun Lee (Seoul Nat'l Univ.), Baojiu Li (Durham Univ.)

TL;DR
This study investigates how modified gravity theories influence the likelihood of galaxy groups exceeding the expected turn-around radius, revealing that stronger fifth forces increase the probability of bound violations, thus providing a new way to test gravity models.
Contribution
The paper demonstrates that modified gravity models significantly increase the odds of bound violations in galaxy groups compared to standard GR, offering a novel diagnostic for gravity theories.
Findings
Modified gravity increases the probability of bound violations.
A 4-sigma difference was detected between MG and GR models.
Odds of violations correlate with the strength of the fifth force.
Abstract
The turn-around radii of the galaxy groups show the imprint of a long battle between their self-gravitational forces and the accelerating space. The standard CDM cosmology based on the general relativity (GR) predicts the existence of an upper bound on the expectation value of the turn-around radius which is rarely violated by individual galaxy groups. We speculate that a deviation of the gravitational law from GR on the cosmological scale could cause an appreciable shift of the mean turn-around radius to higher values and make the occurrence of the bound violation more probable. Analyzing the data from high-resolution N-body simulations for two specific models with modified gravity (MG) and the standard GR+CDM cosmology, we determine the turn-around radii of the massive Rockstar groups from the peculiar motions of the galactic halos located in the bound zone where the…
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