Galactic rotation curves inspired by a noncommutative-geometry background
arXiv:1011.1538 · doi:10.1007/s10714-011-1320-5
Abstract
This paper discusses the observed at rotation curves of galaxies in the context of noncommutative geometry. The energy density of such a geometry is diffused throughout a region due to the uncertainty encoded in the coordinate commutator. This intrinsic property appears to be sufficient for producing stable circular orbits, as well as attractive gravity, without the need for dark matter.
12 pages, 3 figures. Published in Gen.Rel.Grav. 44 (2012) 905-916
References in corpus (5)
Cited by in corpus (16)
- Possible existence of wormholes in the galactic halo region
- Searching for higher dimensional wormholes with noncommutative geometry
- Possibility of higher dimensional anisotropic compact star
- Nonommutative wormholes in gravity
- BTZ black holes inspired by noncommutative geometry
- Noncommutative geometry inspired wormholes with conformal motion
- Two diverse models of embedding class one
- Search of wormholes in different dimensional non-commutative inspired space-time with lorentzian distribution
- Quark matter as dark matter in modeling galactic halo
- On the stability of thin-shell wormholes in noncommutative geometry
- Fluid sphere: stability problem and dimensional constraint
- A new proposal for Galactic dark matter: Effect of f(T) gravity
- Noncommutative geometry inspired 3-dimensional charged black hole solution in an anti-de Sitter background space-time
- Accounting for some aspects of dark matter and dark energy via noncommutative geometry
- Noncommutative black hole in the Finslerian spacetime
- Revisiting galactic rotation curves given a noncommutative-geometry background