Extended Gravity Constraints at Different Scales

We review a set of the possible ways to constrain extended gravity models at Galaxy clusters scales (the regime of dark energy explanations and comparison with ACDM), for black hole shadows, gravitational wave astronomy, binary pulsars, the Solar system and a Large Hadron Collider (consequences for high-energy physics at TeV scale). The key idea is that modern experimental and observational precise data provide us with the chance to go beyond general relativity.

Automated summary

This paper reviews the possible ways to constrain extended gravity models at the scale of galaxy clusters, exploring their implications for various astrophysical phenomena and high-energy physics at the TeV scale. It highlights the significance of modern experimental and observational precise data in pushing the boundaries of our understanding beyond general relativity.