Pattern dark matter and galaxy scaling relations
arXiv:2101.08372 · doi:10.1140/epjs/s11734-021-00196-9
Abstract
We argue that a natural explanation for a variety of robust galaxy scaling relations comes from the perspective of pattern formation and self-organization as a result of symmetry breaking. We propose a simple Lagrangian model that combines a conventional model for normal matter in a galaxy with a conventional model for stripe pattern formation in systems that break continuous translation invariance. We show that the energy stored in the pattern field acts as an effective dark matter. Our theory reproduces the gross features of elliptic galaxies as well as disk galaxies (HSB and LSB) including their detailed rotation curves, the radial acceleration relation (RAR), and the Freeman law. We investigate the stability of disk galaxies in the context of our model and obtain scaling relations for the central dispersion for elliptical galaxies. A natural interpretation of our results is that (1) `dark matter' is potentially a collective, emergent phenomenon and not necessarily an as yet undiscovered particle, and (2) MOND is an effective theory for the description of a self-organized complex system rather than a fundamental description of nature that modifies Newton's second law.
arXiv comment41 Pages, 12 figures, 2 Appendices. Additional references and small changes to the text
References in corpus (43)
- The Structure of Cold Dark Matter Halos
- Quantum Gravity at a Lifshitz Point
- Observational evidence for self-interacting cold dark matter
- Cold and Fuzzy Dark Matter
- Relativistic gravitation theory for the MOND paradigm
- Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions
- The Baryonic Tully-Fisher Relation
- The Connection between Galaxies and their Dark Matter Halos
- The Radial Acceleration Relation in Rotationally Supported Galaxies
- A healthy extension of Horava gravity
- Emergent Gravity and the Dark Universe
- The Formation of Disk Galaxies
- 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
- A constant dark matter halo surface density in galaxies
- One Law To Rule Them All: The Radial Acceleration Relation of Galaxies
- Theory of Dark Matter Superfluidity
- A new relativistic theory for Modified Newtonian Dynamics
- A comprehensive catalog of dark matter halo models for SPARC galaxies
- Galaxies appear simpler than expected
- Galaxy Selection and the Surface Brightness Distribution
- The MOND limit from space-time scale invariance
- Cores of Dark Matter Halos Correlate with Disk Scale Lengths
- Nonlocal metric formulations of MOND with sufficient lensing
- The origin of the mass discrepancy-acceleration relation in CDM
- Stability of disk galaxies in the modified dynamics
- The visible matter - dark matter coupling
- The Spatio-Temporal Structure of Spiral-Defect Chaos
- Simple Distribution Functions for Stellar Disks
- From lenticulars to blue compact dwarfs: the stellar mass fraction is regulated by disc gravitational instability
- From massive spirals to dwarf irregulars: a new set of tight scaling relations for cold gas and stars driven by disc gravitational instability
- The universal rotation curve of low surface brightness galaxies IV: the interrelation between dark and luminous matter
- The MOND Fundamental Plane
- Order out of Randomness : Self-Organization Processes in Astrophysics
- NIHAO XVIII: Origin of the MOND phenomenology of galactic rotation curves in a LCDM universe
- The Radial Acceleration Relation (RAR): the crucial cases of Dwarf Discs and of Low Surface Brightness galaxies
- Angular momentum and local gravitational instability in galaxy discs: does correlate with or ?
- Approximating Stellar Orbits: Improving on Epicycle Theory
- The quantum Gaussian well
- A variational theory for point defects in patterns
- Baryon-Interacting Dark Matter: heating dark matter and the emergence of galaxy scaling relations
- Pattern Universes
- Disk galaxies and their dark halos as self-organized patterns