Wave dispersion in a counterstreaming, relativistic thermal, magnetized, electron-positron plasma

Journal Article · Sun May 15 00:00:00 EDT 2011 · Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics (Print)

DOI:https://doi.org/10.1103/PHYSREVE.83.056407· OSTI ID:21560295

Verdon, M W; Melrose, D B ^[1]

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1. School of Physics, University of Sydney, Sydney, New South Wales 2006 (Australia)

The dispersion equation is analyzed for waves in a strongly magnetized, electron-positron plasma in which counterstreaming electrons and positrons have a relativistic thermal distribution in their respective rest frames, for propagation parallel to the magnetic field. We derive the response tensor for the medium, demonstrate the dispersion curves for different temperatures, and discuss the differences from the cold-plasma case. Application to the case of pulsar magnetospheres is discussed.

• OSTI ID: 21560295
• Journal Information: Physical Review. E, Statistical, Nonlinear, and Soft Matter Physics (Print), Vol. 83, Issue 5; Other Information: DOI: 10.1103/PhysRevE.83.056407; (c) 2011 American Institute of Physics; ISSN 1539-3755
• Country of Publication: United States
• Language: English

Related Subjects

70 PLASMA PHYSICS AND FUSION TECHNOLOGY
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
COLD PLASMA
DISPERSIONS
ELECTRON-POSITRON INTERACTIONS
MAGNETIC FIELDS
MAGNETIZATION
PLASMA WAVES
PULSARS
RELATIVISTIC RANGE
STELLAR MAGNETOSPHERES
TEMPERATURE DISTRIBUTION
ATMOSPHERES
COSMIC RADIO SOURCES
ENERGY RANGE
INTERACTIONS
LEPTON-LEPTON INTERACTIONS
PARTICLE INTERACTIONS
PLASMA
STELLAR ATMOSPHERES