Phenomenology of MOND and gravitational polarization
arXiv:1403.5963 · doi:10.1142/S2010194514602713
Abstract
The phenomenology of MOND (flat rotation curves of galaxies, baryonic Tully-Fisher relation, etc.) is a basic set of phenomena relevant to galaxy dynamics and dark matter distribution at galaxy scales. Still unexplained today, it enjoys a remarkable property, known as the dielectric analogy, which could have far-reaching implications. In the present paper we discuss this analogy in the framework of simple non-relativistic models. We show how a specific form of dark matter, made of two different species of particles coupled to different Newtonian gravitational potentials, could permit to interpret in the most natural way the dielectric analogy of MOND by a mechanism of gravitational polarization.
5 pages, 1 figure, to appear in the proceedings of the second Workshop on Antimatter and Gravity (WAG 2013)
References in corpus (7)
- Bimetric MOND gravity
- A Novel Test of the Modified Newtonian Dynamics with Gas Rich Galaxies
- Generalizing TeVeS Cosmology
- Gravitational polarization and the phenomenology of MOND
- Model of Dark Matter and Dark Energy Based on Gravitational Polarization
- Detecting a Lorentz-Violating Field in Cosmology
- Vector field models of modified gravity and the dark sector
Cited by in corpus (6)
- Galaxies as simple dynamical systems: observational data disfavor dark matter and stochastic star formation
- Dark Matter via Massive (bi-)Gravity
- The Third Law of Galactic Rotation
- Phenomenology of Dark Matter via a Bimetric Extension of General Relativity
- Antimatter gravity and the Universe
- Modified Baryonic Dynamics: two-component cosmological simulations with light sterile neutrinos