TY - JOUR
T1 - Relativistic particle acceleration in developing Alfvén turbulence
AU - Matsukiyo, S.
AU - Hada, T.
N1 - Publisher Copyright:
© 2009 The American Astronomical Society. All rights reserved. Printed in the U.S.A.
PY - 2009/2/20
Y1 - 2009/2/20
N2 - 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.
AB - 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.
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U2 - 10.1088/0004-637X/692/2/1004
DO - 10.1088/0004-637X/692/2/1004
M3 - Article
AN - SCOPUS:84964839534
SN - 0004-637X
VL - 692
SP - 1004
EP - 1012
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 2
ER -