Cosmological dynamics of relativistic MOND

In this paper, we investigate the recently proposed relativistic theory for MOND using phase space analysis. Unlike its precedent theory, namely TeVeS, is claimed to agree with observed Cosmic Microwave Background and matter power spectra. We convert background cosmological equations of a set first-order autonomous equations. Then explore corresponding critical points their physical meaning. This method powerful in sense that behavior model diagnosed independently magnitude free parameters theory. show has viable sequence epochs. Although specific initial conditions, mimics standard model; it provides richer structure as far cosmology concerned. implies further investigations are required see if contributes addressing current tensions.