We study the dynamics of N point particles with a gravitational interaction. The divergence of the microcanonical partition function prevents this system from reaching equilibrium. Assuming a random diffusion in phase space we deduce a scaling law involving time, which is numerically checked for 3 interacting masses in a quadratic nonsymmetrical potential. This random walk on the potential energy scale is studied in some detail and the results agree with the numerics
The evolution of closed gravitational systems is studied by means of $N$-body simulations. This, as ...
Fluctuations in the number of particles N within a small subvolume of a system of classical non-inte...
In this chapter the authors investigate the links among different scales, from a probabilistic point...
We consider the time-dependent distribution, $c(\bm{r},t)$, of $N \gg 1$ identical point-like random...
The statistical description of a system containing a large number of particles which interact via Ne...
21 pages, 16 figures, final version to match one to appear in Phys. Rev. E, minor changes to introdu...
We study, using numerical simulations, the dynamical evolution of self-gravitating point particles i...
In the gravitational evolution of a cold infinite particle distribution, two-body interactions can b...
11 pages, 11 figures, shortened introductory sections and other minor modifications, version to appe...
The evolution of material points interacting via gravitational force in 3D space was investigated. A...
Abstract: For the distribution of classical non-interacting particles we use Maxwell-Boltzmann’s sta...
We investigate the derivation of semilinear relaxation systems and scalar conservation laws from a c...
We are interested in a kinetic equation intended to describe the interactions of particles with thei...
This paper continues the study of a family of models studied earlier by the authors. Two particles ...
We discuss the statistical mechanics of a system of self-gravitating particles with an exc...
The evolution of closed gravitational systems is studied by means of $N$-body simulations. This, as ...
Fluctuations in the number of particles N within a small subvolume of a system of classical non-inte...
In this chapter the authors investigate the links among different scales, from a probabilistic point...
We consider the time-dependent distribution, $c(\bm{r},t)$, of $N \gg 1$ identical point-like random...
The statistical description of a system containing a large number of particles which interact via Ne...
21 pages, 16 figures, final version to match one to appear in Phys. Rev. E, minor changes to introdu...
We study, using numerical simulations, the dynamical evolution of self-gravitating point particles i...
In the gravitational evolution of a cold infinite particle distribution, two-body interactions can b...
11 pages, 11 figures, shortened introductory sections and other minor modifications, version to appe...
The evolution of material points interacting via gravitational force in 3D space was investigated. A...
Abstract: For the distribution of classical non-interacting particles we use Maxwell-Boltzmann’s sta...
We investigate the derivation of semilinear relaxation systems and scalar conservation laws from a c...
We are interested in a kinetic equation intended to describe the interactions of particles with thei...
This paper continues the study of a family of models studied earlier by the authors. Two particles ...
We discuss the statistical mechanics of a system of self-gravitating particles with an exc...
The evolution of closed gravitational systems is studied by means of $N$-body simulations. This, as ...
Fluctuations in the number of particles N within a small subvolume of a system of classical non-inte...
In this chapter the authors investigate the links among different scales, from a probabilistic point...