Inductive and Electrostatic Acceleration in Relativistic Jet-Plasma Interactions
Creators
- 1. Stanford Linear Accelerator Center, Stanford University, Stanford, California 94309 (United States)
Description
We report on the observation of rapid particle acceleration in numerical simulations of relativistic jet-plasma interactions and discuss the underlying mechanisms. The dynamics of a charge-neutral, narrow, electron-positron jet propagating through an unmagnetized electron-ion plasma was investigated using a three-dimensional, electromagnetic, particle-in-cell computer code. The interaction excited magnetic filamentation as well as electrostatic plasma instabilities. In some cases, the longitudinal electric fields generated inductively and electrostatically reached the cold plasma-wave-breaking limit, and the longitudinal momentum of about half the positrons increased by 50% with a maximum gain exceeding a factor of 2 during the simulation period. Particle acceleration via these mechanisms occurred when the criteria for Weibel instability were satisfied
Additional details
Identifiers
Publishing Information
- Journal Title
- Physical Review Letters
- Journal Volume
- 96
- Journal Issue
- 11
- Journal Page Range
- p. 115006-115006.4
- ISSN
- 0031-9007
- CODEN
- PRLTAO
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 37083129
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- ACCELERATION; COLD PLASMA; COMPUTER CODES; ELECTRIC FIELDS; ELECTRON-POSITRON INTERACTIONS; ELECTRONS; IONS; LONGITUDINAL MOMENTUM; PLASMA INSTABILITY; PLASMA JETS; PLASMA SIMULATION; POSITRONS; RELATIVISTIC PLASMA; RELATIVISTIC RANGE; THREE-DIMENSIONAL CALCULATIONS
- Descriptors DEC
- ANTILEPTONS; ANTIMATTER; ANTIPARTICLES; CHARGED PARTICLES; ELEMENTARY PARTICLES; ENERGY RANGE; FERMIONS; INSTABILITY; INTERACTIONS; LEPTON-LEPTON INTERACTIONS; LEPTONS; LINEAR MOMENTUM; MATTER; PARTICLE INTERACTIONS; PLASMA; SIMULATION
Optional Information
- Notes
- (c) 2006 The American Physical Society