抄録
A new particle acceleration process in a developing Alfvén turbulence in the course of successive parametric instabilities of a relativistic pair plasma is investigated by utilizing one-dimensional electromagnetic full particle code. Coherent wave-particle interactions result in efficient particle acceleration leading to a power-law-like energy distribution function. In the simulation, high-energy particles having large relativistic masses are preferentially accelerated as the turbulence spectrum evolves in time. The main acceleration mechanism is simultaneous relativistic resonance between a particle and two different waves. An analytical expression of maximum attainable energy in such wave-particle interactions is derived.
| 本文言語 | 英語 |
|---|---|
| ページ(範囲) | 1004-1012 |
| ページ数 | 9 |
| ジャーナル | Astrophysical Journal |
| 巻 | 692 |
| 号 | 2 |
| DOI | |
| 出版ステータス | 出版済み - 2月 20 2009 |
!!!All Science Journal Classification (ASJC) codes
- 天文学と天体物理学
- 宇宙惑星科学
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