The nonextensive parameter for the rotating astrophysical systems with power-law distributions
arXiv:1508.02290 · doi:10.1209/0295-5075/116/60005
Abstract
We study the nonextensive parameter for the rotating astrophysical systems with power-law distributions, including both the rotating self-gravitating system and the rotating space plasma. We extend the equation of nonextensive parameter to complex system with arbitrary force field, and derive a general equation of the q-parameter, most generally including both the rotating self-gravitating systems and the rotating space plasmas. At the same time, we reproduce the kappa-distribution in space plasmas and obtain equations of the kappa-parameter. We show that the q-parameter is related not only to the temperature gradient, the gravitational force and the electromagnetic force, but also to the inertial centrifugal force and Coriolis force. Thus the rotation introduces significant effect on nonextensivity in the systems. Several examples are given to illustrate the nonextensive effect introduced by the rotation.
11 pages, 56 references
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- Effect of magnetic field on transports of charged particles in the weakly ionized plasma with power-law q-distributions in nonextensive statistics
- The collision frequency of electron-neutral-particle in the weakly ionized plasma with the power-law velocity distribution
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- A nonextensive approach for understanding the van der Waals' equation
- The collision frequencies of charged particles in the complex plasmas with the non-Maxwellian velocity distributions