Statistical Mechanics of Self--Gravitating System : Cluster Expansion Method
arXiv:astro-ph/9808160 · doi:10.1016/S0375-9601(99)00422-3
Abstract
We study statistical mechanics of the self--gravitating system applying the cluster expansion method developed in solid state physics. By summing infinite series of diagrams, we derive a complex free energy whose imaginary part is related to the relaxation time of the system. Summation of another series yields two--point correlation function whose correlation length is essentially given by the Jeans wavelength of the system.
4 pages including 2 eps figures, RevTex