Nonequilibrium stationary states of 3D self-gravitating systems
arXiv:1409.2060 · doi:10.1103/PhysRevLett.113.100602
Abstract
Three dimensional self-gravitating systems do not evolve to thermodynamic equilibrium, but become trapped in nonequilibrium quasistationary states. In this Letter we present a theory which allows us to a priori predict the particle distribution in a final quasistationary state to which a self-gravitating system will evolve from an initial condition which is isotropic in particle velocities and satisfies a virial constraint 2K=-U, where K is the total kinetic energy and U is the potential energy of the system.
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- Numerical modeling of material points evolution in a system with gravity
- Intrinsic conformal order revealed in geometrically confined long-range repulsive particles
- Thermodynamic relation for the systems with inhomogeneous distribution of particles