Occam's Razor and a Three-Family Ultralight Fermionic Dark Matter Model
astro-ph.GA, hep-ph
Submitted: 2026-10-05
Updated: 2026-10-05
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
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- Fermionic warm dark matter produces galaxy cores in the observed scales because of quantum mechanics
- Cores in Dwarf Galaxies from Fermi Repulsion
- Models of dark matter halos based on statistical mechanics: II. The fermionic King model
- Modeling dark matter halos with self-interacting fermions: A polytropic approach
- How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves
- General-relativistic structure of two-component quantum dark fermion stars
- Bayesian analysis for rotational curves with $\ell$-boson stars as a dark matter component
- The nuMSM, leptonic asymmetries, and properties of singlet fermions
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