Fokker-Planck-Rosenbluth-Type Equations for Self-gravitating Systems in 1PN Approximation

Understand

We present two formulations of Fokker-Planck-Rosenbluth-type (FPR) equations for many-particle self-gravitating systems, with first order relativistic corrections in the post-Newtonian approach (1PN).

• The first starts from a covariant Fokker-Planck equation for a simple gas, introduced recently by G.
• Chacon-Acosta and G.
• Kremer (Phys.