Galactic orbital motions in the Dark Matter, MOdified Newtonian Dynamics and MOdified Gravity scenarios
arXiv:0904.0219 · doi:10.1111/j.1365-2966.2009.15811.x
Abstract
We simultaneously integrate in a numerical way the equations of motion of both the Magellanic Clouds (MCs) in MOND, MOG and CDM for -1 <= t <= +1 Gyr to see if, at least in principle, it is possible to discriminate between them (Abridged version).
LaTex2e, 11 pages, 2 tables, 8 figures. Issues concerning the masses of MCs clarified. Integration time changed to -1 Gyr <= t <= +1 Gyr. To appear in Monthly Notices of the Royal Astronomical Society (MNRAS)
References in corpus (28)
- The Milky Way's Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars
- The RAVE Survey: Constraining the Local Galactic Escape Speed
- Are the Magellanic Clouds on their First Passage about the Milky Way?
- Detection of a 63 Degree Cold Stellar Stream in the Sloan Digital Sky Survey
- Is the SMC Bound to the LMC? The HST Proper Motion of the SMC
- Analysis of Rotation Curves in the framework of R^n gravity
- Dark matter vs. modifications of the gravitational inverse-square law. Results from planetary motion in the solar system
- The modified Newtonian dynamics-MOND-and its implications for new physics
- Confrontation of MOND with the rotation curves of early-type disc galaxies
- Insight into the baryon-gravity relation in galaxies
- Evolution of spiral galaxies in modified gravity
- Testing modified gravity with globular cluster velocity dispersions
- Fundamental parameter-free solutions in Modified Gravity
- MOND effects in the inner solar system
- Milky Way potentials in CDM and MOND. Is the Large Magellanic Cloud on a bound orbit?
- Escaping from MOND
- MOND habitats within the solar system
- Cosmological Structure Formation under MOND: a new numerical solver for Poisson's equation
- Solar system constraints on multi-field theories of modified dynamics
- Coincidences of Dark Energy with Dark Matter -- Clues for a Simple Alternative?
- Dynamical friction in modified Newtonian dynamics
- An Orbit Fit for the Grillmair Dionatos Cold Stellar Stream
- Vertical dynamics of disk galaxies in MOND
- Loss of mass and stability of galaxies in MOND
- The collision velocity of the bullet cluster in conventional and modified dynamics
- Evolution of spiral galaxies in modified gravity: II- Gas dynamics
- Spiral Galaxies Rotation Curves with a Logarithmic Corrected Newtonian Gravitational Potential
- On the MOND External Field Effect in the Solar System
Cited by in corpus (12)
- General relativistic polytropes with a repulsive cosmological constant
- Constraining the range of Yukawa gravity interaction from S2 star orbits
- Probing hybrid modified gravity by stellar motion around Galactic Centre
- Constraining Extended Gravity Models by S2 star orbits around the Galactic Centre
- Estimating the Parameters of Extended Gravity Theories with the Schwarzschild Precession of S2 Star
- High-energy scalarons in R^{2} gravity as a model for Dark Matter in galaxies
- Estimating the parameters of Hybrid Palatini gravity model with the Schwarzschild precession of S2, S38 and S55 stars: case of bulk mass distribution
- Observational Constraints on the Modified Gravity Model (MOG) Proposed by Moffat: Using the Magellanic System
- Probabilistic distributions of values for ultra-faint dwarf spheroidal galaxies: stochastic samplings of the IMF
- Constraining A String Gauge Field by Galaxy Rotation Curves and Perihelion Precession of Planets
- Dark matter halos modeled by polytropic spheres influenced by the relict cosmological constant and trapping polytropes forming supermassive black holes
- The Jeans theorem and the "Tolman-Oppenheimer-Volkov equation" in an exact wave solution of R^2 gravity