Dark matter chaos in the Solar System - Université Toulouse 3 Accéder directement au contenu
Article Dans Une Revue Monthly Notice- Royal Astronomical Society -Letters- Année : 2013

Dark matter chaos in the Solar System

Résumé

We study the capture of galactic dark matter particles in the Solar System produced by rotation of Jupiter. It is shown that the capture cross section is much larger than the area of Jupiter orbit being inversely diverging at small particle energy. We show that the dynamics of captured particles is chaotic and is well described by a simple symplectic dark map. This dark map description allows to simulate the scattering and dynamics of $10^{14}$ dark matter particles during the life time of the Solar System and to determine dark matter density profile as a function of distance from the Sun. The mass of captured dark matter in the radius of Neptune orbit is estimated to be $2 \cdot 10^{15} g$. The radial density of captured dark matter is found to be approximately constant behind Jupiter orbit being similar to the density profile found in galaxies.

Dates et versions

hal-00748871 , version 1 (06-11-2012)

Identifiants

Citer

J. Lages, Dima Shepelyansky. Dark matter chaos in the Solar System. Monthly Notice- Royal Astronomical Society -Letters-, 2013, 430, pp.L25. ⟨10.1093/mnrasl/sls045⟩. ⟨hal-00748871⟩
156 Consultations
0 Téléchargements

Altmetric

Partager

Gmail Facebook X LinkedIn More