UHECRs and Multiple Shock Acceleration in Active Galactic ... - TAUP

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One can define a conical shock as a surface formed by a sheaf of plane

oblique shocks all making the same angle η to the upstream flow or jet axis

(the flow upstream and downstream is always highly oblique on the surface of the shock)

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Multiple relativistic shock acceleration

One can define a conical shock as a surface formed by a sheaf of plane oblique shocks all making the same angle η to the upstream flow or jet axis (the flow upstream and downstream is always highly oblique on the surface of the shock)

Page 1 and 2: UHECRs and Multiple Shock Accelerat
Page 3: Cosmic ray spectrum
Page 6 and 7: Ultra High Energy Cosmic Rays: At t
Page 8 and 9: Relativistic sources
Page 10 and 11: AGN Jets Individual or multiple sho
Page 12 and 13: Shock-drift acceleration
Page 16 and 17: Overlook Facts: The best power-law
Page 18 and 19: Simulation method* • Injection of
Page 20 and 21: Simulation results
Page 22 and 23: Γsh = 45, 15 Γsh = 45, 15
Page 24 and 25: Summary - Conclusions I • We perf
Page 26 and 27: Back up slides
Page 28: One can define a conical shock as a

UHECRs and Multiple Shock Acceleration in Active Galactic ... - TAUP

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