Probing modified gravity via the mass-temperature relation of galaxy clusters
Amir Hammami, David F. Mota

TL;DR
This paper explores how the mass-temperature relation of galaxy clusters can test modified gravity theories, revealing significant deviations from standard gravity predictions especially in less massive clusters, using cosmological simulations.
Contribution
It demonstrates that the mass-temperature relation can distinguish certain modified gravity models from Einstein's gravity, especially in less massive galaxy clusters, through cosmological simulations.
Findings
Modified gravity models alter the mass-temperature relation significantly.
Screened modified gravities show deviations mainly in less massive clusters.
Gas mass-temperature relation exhibits even larger deviations than thermal mass-temperature.
Abstract
We propose that the mass-temperature relation of galaxy clusters is a prime candidate for testing gravity theories beyond Einstein's general relativity, for modified gravity models with universal coupling between matter and the scalar field. For non-universally coupled models we discover that the impact of modified gravity can remain hidden from the mass-temperature relation. Using cosmological simulations, we find that in modified gravity the mass-temperature relation varies significantly from the standard gravity prediction of . To be specific, for symmetron models with a coupling factor of we find a lower limit to the power law as ; and for f(R) gravity we compute predictions based on the model parameters. We show that the mass-temperature relation, for screened modified gravities, is significantly different from that of standard…
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