On particle acceleration around shocks. I.

被引:37
|
作者
Vietri, M [1 ]
机构
[1] Scuola Normale Super Pisa, I-56100 Pisa, Italy
关键词
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.
引用
收藏
页码:954 / 961
页数:8
相关论文
共 50 条
  • [31] Superbubbles and energetic particles in the Galaxy - I. Collective effects of particle acceleration
    Parizot, E
    Marcowith, A
    van der Swaluw, E
    Bykov, AM
    Tatischeff, V
    ASTRONOMY & ASTROPHYSICS, 2004, 424 (03) : 747 - 760
  • [32] MONTE-CARLO SIMULATIONS OF PARTICLE-ACCELERATION AT OBLIQUE SHOCKS
    BARING, MG
    ELLISON, DC
    JONES, FC
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 1994, 90 (02) : 547 - 552
  • [33] Numerical Simulations of Particle Acceleration at Interplanetary Quasi-perpendicular Shocks
    Kong, F. -J.
    Qin, G.
    Zhang, L. -H.
    ASTROPHYSICAL JOURNAL, 2017, 845 (01)
  • [34] Prospects for ultra-high-energy particle acceleration at relativistic shocks
    Huang, Zhi-Qiu
    Reville, Brian
    Kirk, John G.
    Giacinti, Gwenael
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2023, 522 (04) : 4955 - 4962
  • [35] TRANSPORT EQUATION FOR MHD TURBULENCE: APPLICATION TO PARTICLE ACCELERATION AT INTERPLANETARY SHOCKS
    Sokolov, Igor V.
    Roussev, Ilia I.
    Skender, Marina
    Gombosi, Tamas I.
    Usmanov, Arcadi V.
    ASTROPHYSICAL JOURNAL, 2009, 696 (01) : 261 - 267
  • [36] PARTICLE ACCELERATION IN RELATIVISTIC MAGNETIZED COLLISIONLESS ELECTRON-ION SHOCKS
    Sironi, Lorenzo
    Spitkovsky, Anatoly
    ASTROPHYSICAL JOURNAL, 2011, 726 (02)
  • [37] Particle transport in tangled magnetic fields and Fermi acceleration at relativistic shocks
    Lemoine, M
    Pelletier, G
    ASTROPHYSICAL JOURNAL, 2003, 589 (02) : L73 - L76
  • [38] The numerical simulation of radiative shocks. I. The elimination of numerical shock instabilities using a local oscillation filter
    Sutherland, RS
    Bisset, DK
    Bicknell, GV
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2003, 147 (01) : 187 - 195
  • [39] THE ROLE OF DIFFUSIVE SHOCK ACCELERATION ON NONEQUILIBRIUM IONIZATION IN SUPERNOVA REMNANT SHOCKS. II. EMITTED SPECTRA
    Patnaude, Daniel J.
    Slane, Patrick
    Raymond, John C.
    Ellison, Donald C.
    ASTROPHYSICAL JOURNAL, 2010, 725 (02) : 1476 - 1484
  • [40] Particle acceleration at oblique shocks and discontinuities of the density profile
    Gieseler, UDJ
    Kirk, JG
    Gallant, YA
    Achterberg, A
    ASTRONOMY & ASTROPHYSICS, 1999, 345 (01) : 298 - 306