Statistical properties of classical gravitating particles in (2+1) dimensions

Details Statistical properties of classical gravitating particles in (2+1) dimensions Statistical properties of classical gravitating particles in (2+1) dimensions

2000-07-27

arxiv.org/abs/hep-th/0007218v1

Nucl.Phys. B596 (2001) 273-288

Physics

High Energy Physics

High Energy Physics - Theory

Latex2e (amssymb) file, 17 pages

Scientific paper

10.1016/S0550-3213(00)00705-7

We report the statistical properties of classical particles in (2+1) gravity as resulting from numerical simulations. Only particle momenta have been taken into account. In the range of total momentum where thermal equilibrium is reached, the distribution function and the corresponding Boltzmann entropy are computed. In the presence of large gravity effects, different extensions of the temperature turn out to be inequivalent, the distribution function has a power law high-energy tail and the entropy as a function of the internal energy presents a flex. When the energy approaches the open universe limit, the entropy and the mean value of the particle kinetic energy seem to diverge.

Affiliated with

Also associated with

No associations

Rating

Statistical properties of classical gravitating particles in (2+1) dimensions does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Statistical properties of classical gravitating particles in (2+1) dimensions, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Statistical properties of classical gravitating particles in (2+1) dimensions will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-719729