“…Here, we use galaxy clusters in testing for variations in α. Galaxy clusters are the most massive, gravitationally collapsed objects in the universe and have proved to be wonderful laboratories for studying cosmology, structure formation, galaxy evolution, neutrino mass, graviton mass, various modified gravity theories etc [29][30][31]. In the past two decades, a large number of galaxy clusters have been discovered upto very high redshifts thanks to multi-wavelength surveys in optical, X-ray, and Sunyaev-Zeldovich (SZ, hereafter) at mm wavelengths which have mapped out large-area contiguous regions of the universe.…”