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Title: Kinetic Simulations of Particle Acceleration at Shocks

Conference ·
OSTI ID:1196173
 [1];  [2]
  1. Princeton University
  2. Los Alamos National Laboratory

Collisionless shocks are mediated by collective electromagnetic interactions and are sources of non-thermal particles and emission. The full particle-in-cell approach and a hybrid approach are sketched, simulations of collisionless shocks are shown using a multicolor presentation. Results for SN 1006, a case involving ion acceleration and B field amplification where the shock is parallel, are shown. Electron acceleration takes place in planetary bow shocks and galaxy clusters. It is concluded that acceleration at shocks can be efficient: >15%; CRs amplify B field via streaming instability; ion DSA is efficient at parallel, strong shocks; ions are injected via reflection and shock drift acceleration; and electron DSA is efficient at oblique shocks.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
Princeton University
DOE Contract Number:
AC52-06NA25396
OSTI ID:
1196173
Report Number(s):
LA-UR-15-25380
Resource Relation:
Conference: Plasma Energization: Exchanges Between Fluid and Kinetic Scales ; 2015-05-04 - 2015-05-06 ; Los Alamos, New Mexico, United States, Melbourne (Australia), 19-25 Apr 2015
Country of Publication:
United States
Language:
English

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