Is MOND an Emergent Effective Law of a Complex Dark Matter Sector?
gr-qc, astro-ph.CO
Submitted: 2026-08-24
Updated: 2026-08-24
Terminology
Sources
- Dark Matter Self-interactions and Small Scale Structure
- Ruling Out Bosonic Repulsive Dark Matter in Thermal Equilibrium
- Dark halo microphysics and massive black hole scaling relations in galaxies
- Self-interacting dark matter solves the final parsec problem of supermassive black hole mergers
- Dark Matter Halos as Particle Colliders: A Unified Solution to Small-Scale Structure Puzzles from Dwarfs to Clusters
- Formation and Evolution of the Self-Interacting Dark Matter Halos
- Galaxy stability within a self-interacting dark matter halo
- Polytropic dark halos of elliptical galaxies
- Dark matter concentrations in galactic nuclei according to polytropic models
- Galactic Halos of Fluid Dark Matter
- Evidence for Dark Matter Self-Interactions via Collisionless Shocks in Cluster Mergers
- Self-Interacting Dark Matter
- Observational evidence for self-interacting cold dark matter
- Cores in Dwarf Galaxies from Dark Matter with a Yukawa Potential
- Dark Matter and Dark Radiation
- Repulsive Dark Matter
- Dark Fluid: a complex scalar field to unify dark energy and dark matter
- Probing the cold nature of dark matter
- When Dark Matter Heats Up: A Model-Independent Search for Non-Cold Behavior
- An Analytic Scale-dependent Dark Matter Profile and the Baryonic Tully-Fisher Relation
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