Relativistic stochastic mechanics II: Reduced Fokker-Planck equation in curved spacetime
arXiv:2307.07805 · doi:10.1007/s10955-023-03205-4
Abstract
The general covariant Fokker-Planck equations associated with the two different versions of covariant Langevin equation in Part I of this series of work are derived, both lead to the same reduced Fokker-Planck equation for the non-normalized one particle distribution function (1PDF). The relationship between various distribution functions is clarified in this process. Several macroscopic quantities are introduced by use of the 1PDF, and the results indicate an intimate connection with the description in relativistic kinetic theory. The concept of relativistic equilibrium state of the heat reservoir is also clarified, and, under the working assumption that the Brownian particle should approach the same equilibrium distribution as the heat reservoir in the long time limit, a general covariant version of Einstein relation arises.
25 pages. Published version
References in corpus (6)
- Relativistic Brownian Motion
- One-dimensional nonrelativistic and relativistic Brownian motions: A microscopic collision model
- Relativistic Brownian motion: From a microscopic binary collision model to the Langevin equation
- Relativistic stochastic mechanics I: Langevin equation from observer's perspective
- Covariant transport equation and gravito-conductivity in generic stationary spacetimes
- Gravito-thermal transports, Onsager reciprocal relation and gravitational Wiedemann-Franz law
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- The Kramers escape rate of phase transitions for the 6-dimensional Gauss-Bonnet AdS black hole with triple phases
- Adiabatic Elimination in Relativistic Stochastic Mechanics