2016
DOI: 10.1016/j.physa.2016.06.133
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Non-Markovian Brownian motion in a magnetic field and time-dependent force fields

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Cited by 24 publications
(18 citation statements)
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“…Equations similar to (2.1), i.e. Langevin equations with magnetic field, were studies at many places in application to plasma physics or stochastic systems [22,23,24,27,40,41,42,43]; see especially [25,44,45,46]. Our focus will be on implications of (2.1) for magnetobiology, i.e.…”
Section: Langevin Equationmentioning
confidence: 99%
See 1 more Smart Citation
“…Equations similar to (2.1), i.e. Langevin equations with magnetic field, were studies at many places in application to plasma physics or stochastic systems [22,23,24,27,40,41,42,43]; see especially [25,44,45,46]. Our focus will be on implications of (2.1) for magnetobiology, i.e.…”
Section: Langevin Equationmentioning
confidence: 99%
“…( 5.2) belongs to the class of linear oscillators driven subject to non-local friction and noise. Such systems were studied in [24,25,27,40,41,42,43,44,54,55,56,57]. We apply Fourier's transform to ζ and ξ in (5.2):…”
Section: The Anatomy Of Orbital Magnetismmentioning
confidence: 99%
“…There are several examples where the Brownian motion of the charged particle is found to occur in the condensed phase [2,17,[40][41][42][43]. It is to be noted here that although the study of the Brownian motion of charged particle in the presence of the magnetic field is getting strong attention in different contexts [3][4][5][6][7][8][9][10][11][12][44][45][46][47][48][49][50][51][52] but till now few studies have been reported considering the non-Markovian dynamics [8,9,11,[49][50][51][52]. Most of these studies with non-Markovian dynamics have been done based on the Langevin equation of motion.…”
Section: The Modelmentioning
confidence: 99%
“…The Fokker-Planck equation in the phase space also has been derived in a recent Ref. [52] using a characteristic function for a Brownian charged particle embedded in a memory thermal bath and under the action of force fields: a constant magnetic field and arbitrary timedependent force fields. Based on these methods it is very difficult to write the required Fokker-Planck equations in the energy space or the phase space for the present system where both coordinate and velocity dependent colored multiplicative noises appear.…”
Section: The Modelmentioning
confidence: 99%
“…Then contribution from the dissipative force is considered by the fourth term [1,4,5]. The next drift term may be identified as due to the magnetic force [1,6]. Although additional drift terms in the presence of a magnetic field do not appear for the Markovian dynamics [3,7] but the non-Markovian dynamics may modify the probability flux.…”
mentioning
confidence: 99%