Experimental limits to the density of dark matter in the solar system
arXiv:astro-ph/9507051 · doi:10.1086/176669
Abstract
On the scales of galaxies and beyond there is evidence for unseen dark matter. In this paper we find the experimental limits to the density of dark matter bound in the solar system by studying its effect upon planetary motion.
9 pages, REVTeX, no figures
References in corpus (1)
Cited by in corpus (16)
- Relativistic effects and dark matter in the Solar system from observations of planets and spacecraft
- Dark matter vs. modifications of the gravitational inverse-square law. Results from planetary motion in the solar system
- Constraints on Dark Matter in the Solar System
- Orbital precession due to central-force perturbations
- Analysis of the Yukawa gravitational potential in gravity I: semiclassical periastron advance
- Formalism for testing theories of gravity using lensing by compact objects. III: Braneworld gravity
- Upper limits on density of dark matter in Solar system
- Exact expressions for the pericenter precession caused by some Dark Matter distributions and constraints on them from orbital motions in the Solar System, in the double pulsar and in the Galactic center
- Density of dark matter in Solar system and perihelion precession of planets
- Effect of Sun and Planet-Bound Dark Matter on Planet and Satellite Dynamics in the Solar System
- Influence of Dark Matter on Light Propagation in Solar System
- New Constraints on Dark Matter and Cosmic Neutrino Profiles through Gravity
- General formulae for the periapsis shift of a quasi-circular orbit in static spherically symmetric spacetimes and the active gravitational mass density
- Local dark matter searches with LISA
- Motion of Particles in Solar and Galactic Systems by Using Neumann Boundary Condition
- Probing Bosonic Overdensities with Optomechanical Sensing