Exact solution of the Fokker-Planck equation for isotropic scattering
Abstract
The Fokker-Planck (FP) equation ∂tf +μ ∂xf =∂μ(1 -μ2) ∂μf is solved analytically. Foremost among its applications, this equation describes the propagation of energetic particles through a scattering medium (in x - direction, with μ being the x - projection of particle velocity). The solution is found in terms of an infinite series of mixed moments of particle distribution, ⟨μjxk⟩. The second moment ⟨x2⟩ (j =0 , k =2 ) was obtained by G. I. Taylor (1920) in his classical study of random walk: ⟨x2⟩ =⟨x2⟩0+t /3 +[exp (-2 t ) -1 ] /6 (where t is given in units of an average time between collisions). It characterizes a spatial dispersion of a particle cloud released at t =0 , with √{⟨x2⟩0} being its initial width. This formula distills a transition from ballistic (rectilinear) propagation phase, ⟨x2⟩ -⟨x2⟩0≈t2/3 to a time-asymptotic, diffusive phase, ⟨x2⟩ -⟨x2⟩0≈t /3 . The present paper provides all the higher moments by a recurrence formula. The full set of moments is equivalent to the full solution of the FP equation, expressed in form of an infinite series in moments ⟨μjxk⟩. An explicit, easy-to-use approximation for a point source spreading of a pitch-angle averaged distribution f0(x ,t ) (starting from f0(x ,0 ) =δ (x ) , i.e., Green's function), is also presented and verified by a numerical integration of the FP equation.
- Publication:
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Physical Review D
- Pub Date:
- January 2017
- DOI:
- arXiv:
- arXiv:1610.01584
- Bibcode:
- 2017PhRvD..95b3007M
- Keywords:
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- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- 15 pages, 3 Figures, improved numerics, to appear in PRD