Power distributions for self-gravitating astrophysical systems based on nonextensive Tsallis kinetics
Sign Up to like & getrecommendations! Published in 2017 at "Solar System Research"
DOI: 10.1134/s0038094617020046
Abstract: The long-time development of self-gravitating gaseous astrophysical systems (in particular, the evolution of the protoplanet accretion disk) is mainly determined by relatively fast processes of the collision relaxation of particles. However, slower dynamical processes related… read more here.
Keywords: power; gravitating astrophysical; astrophysical systems; self gravitating ... See more keywords