General relativity and its Newtonian weak field limit are not sufficient to explain the observed
phenomenology in the Universe, from the formation of large-scale structures to the dynamics …

Dark matter phenomena in rotationally supported galaxies exhibit a characteristic
acceleration scale of g†≈ 1.2× 10− 10 ms− 2. Whether this acceleration is a manifestation of …

Recently, the discovery of the radial acceleration relation (RAR) in galaxies has been
regarded as an indirect support of alternative theories of gravity such as modified Newtonian …

We carry out a test of the radial acceleration relation (RAR) for galaxy clusters from two
different catalogs compiled in literature, as an independent cross-check of two recent …

We propose a complementary and fast approach to study galaxy rotation curves directly from
the sample data, instead of individual fits. With this approach, some relevant tests can be …

Milgrom's modified Newtonian dynamics (MOND) can explain well the mass discrepancy
problem in galaxy without invoking dark matter. The MOND theory predicts a universal …

We carry out a test of the radial acceleration relation (RAR) for a sample of 10 dynamically
relaxed and cool-core galaxy clusters imaged by the Chandra X-ray telescope, which was …

The radial acceleration relation (RAR) shows a strong correlation between two accelerations
associated with galaxy rotation curves. The relation between these accelerations is given by …

The application of Bayesian techniques to astronomical data is generally non-trivial because
the fitting parameters can be strongly degenerated and the formal uncertainties are …

The dark matter halo surface density, given by the product of the dark matter core radius (rc)
and core density (ρ c) has been shown to be a constant for a wide range of isolated galaxy …