NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
A determination of relativistic shock jump conditions using Monte Carlo techniquesMonte Carlo techniques are used, assuming isotropic elastic scattering of all particles, to calculate jump conditions in parallel relativistic collisionless shocks in the absence of Fermi acceleration. The shock velocity and compression ratios are shown for arbitrary flow velocities and for any upstream temperature. Both single-component electron-positron plasma and two-component proton-electron plasmas are considered. It is shown that protons and electrons must share energy, directly or through the mediation of plasma waves, in order to satisfy the basic conservation conditions, and the electron and proton temperatures are determined for a particular microscopic, kinetic-theory model, namely, that protons always scatter elastically. The results are directly applicable to shocks in which waves of scattering superthermal particles are absent.
Document ID
19910065874
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Ellison, Donald C.
(North Carolina State Univ. Raleigh, NC, United States)
Reynolds, Stephen P.
(North Carolina State University Raleigh, United States)
Date Acquired
August 14, 2013
Publication Date
September 1, 1991
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 378
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
91A50497
Funding Number(s)
CONTRACT_GRANT: NAG5-1042
CONTRACT_GRANT: NSF AST-88-17567
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available