Dark Matter Superfluidity
arXiv:2109.10928 · doi:10.21468/SciPostPhysLectNotes.42
Abstract
In these lectures I describe a theory of dark matter superfluidity developed in the last few years. The dark matter particles are axion-like, with masses of order eV. They Bose-Einstein condense into a superfluid phase in the central regions of galaxy halos. The superfluid phonon excitations in turn couple to baryons and mediate a long-range force (beyond Newtonian gravity). For a suitable choice of the superfluid equation of state, this force reproduces the various galactic scaling relations embodied in Milgrom's law. Thus the dark matter and modified gravity phenomena represent different phases of a single underlying substance, unified through the rich and well-studied physics of superfluidity.
arXiv comment21 pages, 1 figure, Submitted to SciPost Physics Lecture Notes, Les Houches Summer School Series. v2: corrected typos and added references
References in corpus (73)
- Planck 2013 results. XVI. Cosmological parameters
- Theory of Bose-Einstein condensation in trapped gases
- Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
- Theory of ultracold Fermi gases
- Cold and Fuzzy Dark Matter
- Ultralight scalars as cosmological dark matter
- Small-Scale Challenges to the CDM Paradigm
- Relativistic gravitation theory for the MOND paradigm
- Too big to fail? The puzzling darkness of massive Milky Way subhaloes
- Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions
- Modified Newtonian Dynamics as an Alternative to Dark Matter
- The Radial Acceleration Relation in Rotationally Supported Galaxies
- Dynamical Friction in a Gaseous Medium
- Emergent Gravity and the Dark Universe
- Can dark matter be a Bose-Einstein condensate?
- The non-gravitational interactions of dark matter in colliding galaxy clusters
- Mass-radius relation of Newtonian self-gravitating Bose-Einstein condensates with short-range interactions: I. Analytical results
- A Vast Thin Plane of Co-rotating Dwarf Galaxies Orbiting the Andromeda Galaxy
- Bose-Einstein Condensation of Dark Matter Axions
- The unexpected diversity of dwarf galaxy rotation curves
- The Baryonic Tully-Fisher Relation of Gas Rich Galaxies as a Test of LCDM and MOND
- Late time Cosmological Phase Transition and Galactic Halo as Bose-liquid
- Fluid Dark Matter
- One Law To Rule Them All: The Radial Acceleration Relation of Galaxies
- General coordinate invariance and conformal invariance in nonrelativistic physics: Unitary Fermi gas
- Repulsive Dark Matter
- The VPOS: a vast polar structure of satellite galaxies, globular clusters and streams around the Milky Way
- Dynamical Friction and the Distribution of Dark Matter in Barred Galaxies
- The distribution of dark matter in galaxies
- Large Scale Structure in Bekenstein's theory of relativistic Modified Newtonian Dynamics
- The small scatter of the baryonic Tully-Fisher relation
- Do Dark Matter Axions Form a Condensate with Long-Range Correlation?
- BCS-BEC Crossover and the Unitary Fermi Gas
- Theory of Dark Matter Superfluidity
- Understanding the shape and diversity of dwarf galaxy rotation curves in LCDM
- Field-theoretical formulations of MOND-like gravity
- Angular Momentum and Vortex Formation in Bose-Einstein-Condensed Cold Dark Matter Haloes
- On the Proof of Dark Matter, the Law of Gravity and the Mass of Neutrinos
- Bose-Einstein condensation of dark matter solves the core/cusp problem
- Fitting the radial acceleration relation to individual SPARC galaxies
- An extensive study of dynamical friction in dwarf galaxies: the role of stars, dark matter, halo profiles and MOND
- The mass distribution of the Fornax dSph: constraints from its globular cluster distribution
- The Relation between Stellar and Dynamical Surface Densities in the Central Regions of Disk Galaxies
- X-ray Group and cluster mass profiles in MOND: Unexplained mass on the group scale
- Dark Matter Superfluidity and Galactic Dynamics
- Gravitational polarization and the phenomenology of MOND
- The globular cluster NGC 2419: a crucible for theories of gravity
- The mass discrepancy acceleration relation in a CDM context
- Model of Dark Matter and Dark Energy Based on Gravitational Polarization
- An Alternative to Particle Dark Matter
- Cold Dark Matter with MOND Scaling
- The scatter, residual correlations and curvature of the SPARC baryonic Tully-Fisher relation
- Phenomenological consequences of superfluid dark matter with baryon-phonon coupling
- Dark matter as a Bose--Einstein Condensate: the relativistic non-minimally coupled case
- Dark Matter via Massive (bi-)Gravity
- Another Path for the Emergence of Modified Galactic Dynamics from Dark Matter Superfluidity
- Low-energy effective field theory for finite-temperature relativistic superfluids
- Galaxy Clusters in the Context of Superfluid Dark Matter
- Finite temperature effects in Bose-Einstein Condensed dark matter halos
- Unified Superfluid Dark Sector
- Reconciling MOND and dark matter?
- Dynamical Friction in Superfluids
- A Realistic Cosmology Without Cold Dark Matter
- The Radial Acceleration Relation (RAR): the crucial cases of Dwarf Discs and of Low Surface Brightness galaxies
- Dipolar Dark Matter with Massive Bigravity
- The Equation of State of Dark Matter Superfluids
- The Milky Way's rotation curve with superfluid dark matter
- Strong lensing with superfluid dark matter
- Evidences for Collisional Dark Matter In Galaxies?
- Chance and Chandra (and repulsive dark matter)
- MOND: time for a change of mind?
- Lessons from the Local Group (and beyond) on dark matter
- A Dark Matter Superfluid
Cited by in corpus (7)
- A statistical investigation of the mass discrepancy-acceleration relation
- Unified Superfluid Dark Sector
- A Universe Without Dark Energy: Cosmic Acceleration from Dark Matter-Baryon Interactions
- The Equation of State of Dark Matter Superfluids
- Baryon-Interacting Dark Matter: heating dark matter and the emergence of galaxy scaling relations
- Science from an Ultra-Deep, High-Resolution Millimeter-Wave Survey
- CMB-HD: An Ultra-Deep, High-Resolution Millimeter-Wave Survey Over Half the Sky