Possible Observational Signatures of RMOND

Modified Newtonian Dynamics (MOND) nicely accounts for the observed universal galactic acceleration scale, but the basic version of MOND cannot account for the cosmic microwave background (CMB) and matter power spectrum observational data. However, a relativistic MOND (RMOND) theory like Skordis and Zlosnik’s can. In this talk, I discuss possible observational signatures from this RMOND theory, including gravitational wave signatures.