L. Campanelli; G.L. Fogli; T. Kahniashvili; A. Marrone; Bharat Ratra
(2013-04-22)
We use data onmassive galaxy clusters (Mcluster>
8 × 1014h
−1M within a comoving radius of Rcluster =
1.5h
−1 Mpc) in the redshift range 0.05 z 0.83 to place
constraints, simultaneously, on the nonrelativistic ...