Modified Gravity and the Black Hole Mass Gap
Maria C. Straight, Jeremy Sakstein, and Eric J. Baxter

TL;DR
This paper introduces the black hole mass gap as a new method to test modified gravity theories, showing how fifth forces affect stellar evolution and black hole formation, and applying this to LIGO/Virgo data to constrain gravity modifications.
Contribution
It develops a novel approach using the black hole mass gap to constrain modified gravity theories and demonstrates its application with real gravitational wave data.
Findings
Modified gravity can explain GW190521 as an unscreened galaxy event.
A 7% bound on the difference in gravitational constant was obtained from LIGO/Virgo data.
Black hole mass gap predictions can constrain fifth forces in gravity theories.
Abstract
We pioneer the black hole mass gap as a powerful new tool for constraining modified gravity theories. These theories predict fifth forces that alter the structure and evolution of population-III stars, exacerbating the pair-instability. This results in the formation of lighter astrophysical black holes and lowers both the upper and lower edges of the mass gap. These effects are explored using detailed numerical simulations to derive quantitative predictions that can be used as theoretical inputs for Bayesian data analysis. We discuss detection strategies in light of current and upcoming data as well as complications that may arise due to environmental screening. To demonstrate the constraining power of the mass gap, we present a novel test of the strong equivalence principle where we apply our results to an analysis of the first ten LIGO/Virgo binary black hole merger events to obtain a…
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