Abstract

The present work is concerned with the study of a generalized Langevin equation and its link to the physical theories of statistical mechanics and scale relativity. It is demonstrated that the form of the coefficients of the Langevin equation depends critically on the assumption of continuity of the reconstructed trajectory. This in turn demands for the fluctuations of the diffusion term to be discontinuous in time. This paper further investigates the connection between the scale-relativistic and stochastic mechanics approaches, respectively, with the study of the Burgers equation, which in this case appears as a stochastic geodesic equation for the drift. By further demanding time reversibility of the drift, the Langevin equation can also describe equivalent quantum-mechanical systems in a path-wise manner. The resulting statistical description obeys the Fokker–Planck equation of the probability density of the differential system, which can be readily estimated from simulations of the random paths. Based on the Fokker–Planck formalism, a new derivation of the transient probability densities is presented. Finally, stochastic simulations are compared to the theoretical results.

Highlights

  • The Langevin equation was introduced in order to describe the motion of a test particle subjected to a fluctuating force and a viscous drag [1]

  • This paper further investigates the connection between the scale-relativistic and stochastic mechanics approaches, respectively, with the study of the Burgers equation, which in this case appears as a stochastic geodesic equation for the drift

  • While this description can be achieved by fractional differ–integrals, or by multi-scale approaches [39], the present work focused on a local description

Read more

Summary

Introduction

The Langevin equation was introduced in order to describe the motion of a test particle subjected to a fluctuating force and a viscous drag [1]. The Langevin equation is fundamental for the stochastic interpretation of Quantum Mechanics (QM) [2] and it appears, in the form of a geodesic equation, in the scale relativity theory (SR) developed by Nottale [3]. The formal equations of stochastic mechanics were formulated at first by Fényes [19] and Weizel [20] and later taken up by Nelson [2] Following this interpretation, the trajectories of the configuration, described by a Markov stochastic process, are regarded as physically real. Nottale introduces a complex operator that he calls the scale derivative, which acts as a pseudo-derivative (see Section 4 for details).Using this tool, Nottale gives an informal derivation of the Schrödinger equation from the classical Newtonian equation of dynamics, via a quantization procedure that follows from an extension of Einstein’s relativity principle called the scale relativity principle

Stochastic Representation of Trajectories
Nelson’s Characterization
The Complex Velocity Operator in SR and SM Theories
The Real Stochastic Geodesic Equations
Path-Wise Separable Solutions
Stationary Drift Fields
Stationary Density Solutions
Asymptotic Density Solutions
The Complex Stochastic Geodesic Equations
Real-Valued and Complex Cole–Hopf Transformations
Exact Simulations
Free Diffusion
Particle in a Box
Discussion
Full Text
Published version (Free)

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call