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A new analytic solution for 2nd-order Fermi acceleration
被引:10
作者:
Mertsch, Philipp
[1
]
机构:
[1] Univ Oxford, Rudolf Peierls Ctr Theoret Phys, Oxford OX1 3NP, England
来源:
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
|
2011年
/
12期
关键词:
particle acceleration;
cosmic ray theory;
STOCHASTIC PARTICLE-ACCELERATION;
COSMIC-RAY TRANSPORT;
ELECTRON ACCELERATION;
CHARGED PARTICLES;
BLACK-HOLE;
EMISSION;
EVOLUTION;
WAVES;
REACCELERATION;
TURBULENCE;
D O I:
10.1088/1475-7516/2011/12/010
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
A new analytic solution for 2nd-order Fermi acceleration is presented. In particular, we consider time-dependent rates for stochastic acceleration, diffusive and convective escape as well as a diabatic losses. The power law index q of the turbulence spectrum is unconstrained and can therefore account for Kolmogorov (q - 5/3) and Kraichnan (q - 3/2) turbulence, Bohm diffusion (q = 1) as well as the hard-sphere approximation (q = 2). This considerably improves beyond solutions known to date and will prove a useful tool for more realistic modelling of 2nd-order Fermi acceleration in a variety of astrophysical environments.
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页数:14
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