Issues in the Investigations of the Dark Matter Phenomenon in Galaxies: Parcere Personis, Dicere de Vitiis
arXiv:2502.11872 · doi:10.3390/universe11020067
Abstract
It is always more evident that the kinematics of galaxies provide us with unique information on the Nature of the dark particles and on the properties of the galaxy Dark Matter (DM) halos. However, in investigating this topic, we have to be very careful about certain issues related to the assumptions that we take or to the practices that we follow. Here, we critically discuss such issues, that, today, result of fundamental importance, in that we have realized that the Nature of the DM will be not provided by The Theory but, has to be inferred by reverse engineering the observational scenario.
arXiv comment13 pages 5 Figures Comments welcome. In print on Universe
References in corpus (26)
- A Universal Density Profile from Hierarchical Clustering
- Cold and Fuzzy Dark Matter
- Small-Scale Challenges to the CDM Paradigm
- Halos and galaxies in the standard cosmological model: results from the Bolshoi simulation
- Analytical Models For Galactic Nuclei
- The cored distribution of dark matter in spiral galaxies
- Dark Matter Scaling Relations
- A constant dark matter halo surface density in galaxies
- Sterile Neutrino Dark Matter
- The Universal Rotation Curve of Spiral Galaxies. II The Dark Matter Distribution out to the Virial Radius
- The distribution of dark matter in galaxies
- Strongly baryon-dominated disk galaxies at the peak of galaxy formation ten billion years ago
- Dwarf galaxies in CDM and SIDM with baryons: observational probes of the nature of dark matter
- The universal rotation curve of dwarf disk galaxies
- Template Rotation Curves for Disk Galaxies
- The constant density region of the dark halos of spiral galaxies
- Density profiles of dark matter haloes on Galactic and Cluster scales
- The Radial Tully-Fisher relation for spiral galaxies I
- Indefinitely Flat Circular Velocities and the Baryonic Tully-Fisher Relation from Weak Lensing
- Phase space mass bound for fermionic dark matter from dwarf spheroidal galaxies
- The universal rotation curve of low surface brightness galaxies IV: the interrelation between dark and luminous matter
- Constraining Non-local Gravity by S2 star orbits
- Constraints on Yukawa gravity parameters from observations of bright stars
- The Quest for the Nature of the Dark Matter: The Need of a New Paradigm
- Empirical velocity profiles for galactic rotation curves
- Dark matter halos of luminous AGNs from galaxy-galaxy lensing with the HSC Subaru Strategic Program