acceleration of particles;
cosmic rays;
shock waves;
D O I:
10.1086/375534
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We derive a relativistically covariant (although not manifestly so) equation for the distribution function of particles accelerated at shocks, which applies also to extremely relativistic shocks and arbitrarily anisotropic particle distributions. The theory is formulated for arbitrary pitch-angle scattering and reduces to the well-known case for small-angle scatterings via a Fokker-Planck approximation. The boundary conditions for the problem are completely reformulated introducing a physically motivated Green's function; the new formulation allows derivation of the particle spectrum both close and far away from the injection energy in an exact way, while it can be shown to reduce to a power law at large particle energies. The particle spectral index is also recovered in a novel way. Contact is made with the Newtonian treatment.
机构:
Stanford Univ, Dept Phys, Stanford, CA 94305 USA
Stanford Univ, KIPAC, Stanford, CA 94305 USA
Stanford Univ, Dept Appl Phys, Stanford, CA 94305 USAStanford Univ, Dept Phys, Stanford, CA 94305 USA
机构:
Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210034, Jiangsu, Peoples R China
Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Anhui, Peoples R ChinaChinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210034, Jiangsu, Peoples R China
Zhang, Yiran
Liu, Siming
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机构:
Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210034, Jiangsu, Peoples R China
Univ Sci & Technol China, Sch Astron & Space Sci, Hefei 230026, Anhui, Peoples R ChinaChinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210034, Jiangsu, Peoples R China