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The distribution of dark matter in galaxies
Paolo Salucci
The distribution of the non-luminous matter in galaxies of different luminosity and Hubble type is much more than a proof of the existence of dark particles governing the structure…
The Radial Acceleration Relation (RAR): the crucial cases of Dwarf Discs and of Low Surface Brightness galaxies
Chiara Di Paolo, Paolo Salucci, Jean Philippe Fontaine
McGaugh et al. (2016) have found, in a large sample of disc systems, a tight nonlinear relationship between the total radial accelerations and their components arisen fro…
The Dark Side Properties of Galaxies Requires (viable) Modifications to the Verlinde's Emergent Gravity Theory
Gauri Sharma, Paolo Salucci
Dark Matter is an unknown entity in the Universe. Although several fields of astrophysics \& cosmology are trying to endorse this elusive matter, however, its nature remains an ope…
Dark Matter in Galaxies: evidences and challenges
Paolo Salucci
The evidence of the phenomenon for which, in galaxies, the gravitating mass is distributed differently than the luminous mass, increases as new data become available. Furthermore,…
Kinematics of Spiral galaxies as a Portal to the Nature of Dark Matter
Paolo Salucci
The gravitational field of Spiral galaxies is well traced by their rotation curves. Only recently it has become of extreme interest that the latter form a family ruled by two param…
The universal rotation curve of low surface brightness galaxies IV: the interrelation between dark and luminous matter
Chiara Di Paolo, Paolo Salucci, Adnan Erkurt
We investigate the properties of the baryonic and the dark matter components in low surface brightness (LSB) disc galaxies, with central surface brightness in the B band $μ_0 \geq…