Chaotic particle heating due to an obliquely propagating wave in a magnetized plasma

被引:2
|
作者
Correa da Silva, T. M. [1 ]
Pakter, R. [1 ]
Rizzato, F. B. [1 ]
de Sousa, M. C. [2 ]
Caldas, I. L. [2 ]
Steffens, F. M. [2 ]
机构
[1] Univ Fed Rio Grande do Sul, Inst Fis, Porto Alegre, RS, Brazil
[2] Univ Sao Paulo, Inst Fis, BR-01498 Sao Paulo, Brazil
来源
PHYSICAL REVIEW E | 2013年 / 88卷 / 01期
基金
巴西圣保罗研究基金会;
关键词
ACCELERATION; INSTABILITY; ELECTRONS; DYNAMICS;
D O I
10.1103/PhysRevE.88.013101
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
We study the dynamics of a relativistic charged particle in the presence of a uniform magnetic field and a stationary electrostatic wave that propagates at an arbitrary angle. The wave is considered as a series of periodic pulses which allows us to derive an exact map for the system. In particular, we investigate the heating process of an initially low-energy particle. It is found that abrupt changes in the maximum energy attained by the particle may occur as the angle between the wave propagation and the magnetic field varies. To determine what is the mechanism behind this phenomenon a reduced Hamiltonian that retains the important dynamical features is obtained. Using both Poincare plots and perturbation theory, we identify that a separatrix reconnection is the key mechanism for the abrupt change in particle response.
引用
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页数:7
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