Shock corrugation by Rayleigh-Taylor instability in gamma-ray burst afterglow jets

Physics & Astronomy

• afterglows 89%
• compressibility 19%
• cooling 27%
• corrugating 36%
• deceleration 22%
• equipartition theorem 30%
• gamma ray bursts 86%
• kinetic energy 16%
• light curve 20%
• magnetic fields 40%
• shock 62%
• synchrotrons 17%
• Taylor instability 100%
• thermal energy 41%
• turbulence 31%

Earth & Environmental Sciences

• calculation 11%
• compressibility 20%
• cooling 29%
• energy 29%
• gamma radiation 82%
• kinetic energy 19%
• turbulence 31%