A kinetic approach to cosmic-ray-induced streaming instability at supernova shocks

Monthly Notices of the Royal Astronomical Society

Volumn 392, Issue 4, 2009, Pages 1591-1600

  Amato, E ^a   Blasi, P ^a,b,c  

^a INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

^b NASA FERMILAB ASTROPHYSICS CENTER   (United States)

^c LABORATORI NAZIONALI DEL GRAN SASSO   (Italy)

Author keywords

Acceleration of particles; Shock waves

Indexed keywords

COSMIC RAYS; DISPERSION (WAVES); DISPERSIONS; KINETIC ENERGY; KINETICS; MAGNETOHYDRODYNAMICS; MAGNETOPLASMA; QUANTUM THEORY; SHOCK WAVES; SUPERNOVAE;

'CURRENT; ACCELERATION OF PARTICLES; CONDITION; DISPERSION RELATIONS; KINETIC APPROACH; MICROPHYSICS; NONRESONANT; RESONANT MODE; SHOCK FRONTS; SHOCK-WAVES;

COSMOLOGY;

EID: 58449129504     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.14200.x     Document Type: Article

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