TY - JOUR
T1 - Brownian motion in a magnetic field and in the presence of additional external forces
AU - Jiménez-Aquino, J. I.
AU - Romero-Bastida, M.
AU - Pérez-Guerrero Noyola, A. C.
PY - 2008/6
Y1 - 2008/6
N2 - Our purpose in this paper is to solve exactly the Fokker-Planck-Kramers equation of a charged particle (heavy-ion) embedded in a fluid and under the influence of mechanical and electromagnetic forces. In this work the magnetic field is assumed to be constant and pointing along any direction of a Cartesian reference frame; the mechanical and electrical forces are both space-independent, but in general time-dependent. Our proposal relies upon two transformations of the Langevin equation associated with the charged particle's phase-space (r, u). The first one is a fixed rotation which transforms the (r, u)-coordinates into other (r′, u′)-coordinates, and makes it possible to re-orientate the magnetic field along an appropriate direction (say along the z′-axis). The second one is a time-dependent rotation which transforms the (r′, u′)-coordinates into other (r″, u′)-coordinates, in which the resulting Langevin equation strongly resembles that of ordinary Brownian motion in the presence of external forces. Under these circumstances, the Fokker-Planck-Kramers equation can immediately be solved in the (r″, u″) phase-space, following our methodology developed in Ref.
AB - Our purpose in this paper is to solve exactly the Fokker-Planck-Kramers equation of a charged particle (heavy-ion) embedded in a fluid and under the influence of mechanical and electromagnetic forces. In this work the magnetic field is assumed to be constant and pointing along any direction of a Cartesian reference frame; the mechanical and electrical forces are both space-independent, but in general time-dependent. Our proposal relies upon two transformations of the Langevin equation associated with the charged particle's phase-space (r, u). The first one is a fixed rotation which transforms the (r, u)-coordinates into other (r′, u′)-coordinates, and makes it possible to re-orientate the magnetic field along an appropriate direction (say along the z′-axis). The second one is a time-dependent rotation which transforms the (r′, u′)-coordinates into other (r″, u′)-coordinates, in which the resulting Langevin equation strongly resembles that of ordinary Brownian motion in the presence of external forces. Under these circumstances, the Fokker-Planck-Kramers equation can immediately be solved in the (r″, u″) phase-space, following our methodology developed in Ref.
KW - (FP) Fokker-Planck
KW - (FPK) Fokker-Planck-Kramers
UR - http://www.scopus.com/inward/record.url?scp=49249111852&partnerID=8YFLogxK
M3 - Artículo
SN - 1870-3542
VL - 54
SP - 81
EP - 86
JO - Revista Mexicana de Fisica E
JF - Revista Mexicana de Fisica E
IS - 1
ER -