Cosmic ray acceleration by a supernova shock in a dense circumstellar plasma
Monthly Notices of the Royal Astronomical Society 385:4 (2008) 1884-1892
Abstract:
Cosmic ray acceleration may occur at a supernova shock expanding into a circumstellar wind sustaining a Parker spiral magnetic field. Cosmic rays drift to the poles producing a large cosmic ray pressure which can generate polar density cavities through which cosmic rays escape upstream of the shock. This may be relevant to gamma-ray bursts accompanying shock breakout. 漏 2008 The Author. Journal compilation 漏 2008 RAS.Non-Spitzer return currents in intense laser-plasma interactions
PHYSICS OF PLASMAS 14:10 (2007) ARTN 102708
Absorption of ultra-short laser pulses and particle transport in dense targets
LASER AND PARTICLE BEAMS 24:2 (2006) 231-234
Effect of Target Composition on Proton Energy Spectra in Ultraintense Laser-Solid Interactions
Physical Review Letters 96 (2006) 035005 4pp
Fast electron transport in laser-produced plasmas and the KALOS code for solution of the Vlasov-Fokker-Planck equation
PLASMA PHYSICS AND CONTROLLED FUSION 48:3 (2006) R37-R57