1988
DOI: 10.1103/physreva.37.4026
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Charged particle in the presence of a variable magnetic field

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1988
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Cited by 25 publications
(12 citation statements)
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“…For time-independent spring forces in the presence of a time-independent magnetic field, [25,26] gave the analytic wave function and energy spectrum, which, in terms of the Heisenberg picture we consider in this paper, means that analytic solutions of (68) were found. For the time-dependent case, [27,28] found analytic wave function for an isotropic harmonic oscillator. For the general case, finding the analytic solution of (68) is not an easy task and it is beyond the analysis presented in this paper.…”
Section: Quantizationmentioning
confidence: 99%
“…For time-independent spring forces in the presence of a time-independent magnetic field, [25,26] gave the analytic wave function and energy spectrum, which, in terms of the Heisenberg picture we consider in this paper, means that analytic solutions of (68) were found. For the time-dependent case, [27,28] found analytic wave function for an isotropic harmonic oscillator. For the general case, finding the analytic solution of (68) is not an easy task and it is beyond the analysis presented in this paper.…”
Section: Quantizationmentioning
confidence: 99%
“…Instead, it can be modeled by two-dimensional time-dependent harmonic oscillator due to the existence of variable magnetic field B(t). Theoretical and experimental researches have been carried out extensively on the quantum properties of this system in the past several decades due to its importance not only in condensed matter physics but also in plasma physics [26][27][28][29][30][31][32][33][34][35][36]. Especially, the study of charged particle motion driven by external magnetic field is crucial in investigating magnetic confinement devices for fusion plasmas (whose subtopics are tokamaks, mirror machines, bumpy tori, and stellarators) and for space and astrophysical plasmas (whose subtopics are magnetospheric plasmas of earth and other planets like pulsar) [36].…”
Section: Introductionmentioning
confidence: 99%
“…These states were used to calculate the propagators, transition amplitudes and transition probabilities between energy levels corresponding to the initial and final asymptotic magnetic fields. Several other aspects of the problem, where solutions to Equation (3) were used, were considered later, e.g., in papers [11][12][13][14][15][16][17][18][19][20][21][22][23][24][25][26] for α = 0. In particular, the problem of squeezing in the time dependent magnetic field with α = 0 was considered in [14,16,17,19,26] with respect to the canonical pairs of variables.…”
Section: Introductionmentioning
confidence: 99%