Research@StAndrews
 
The University of St Andrews

Research@StAndrews:FullText >
University of St Andrews Research >
University of St Andrews Research >
University of St Andrews Research >

Please use this identifier to cite or link to this item: http://hdl.handle.net/10023/3154
This item has been viewed 5 times in the last year. View Statistics

Files in This Item:

File Description SizeFormat
relav_harris_v6.pdf113.65 kBAdobe PDFView/Open
Title: Collisionless distribution function for the relativistic force-free Harris sheet
Authors: Stark, C. R.
Neukirch, T.
Keywords: Plasma confinement
Plasma kinetic theory
Plasma simulation
Plasma thermodynamics
Relativistic plasmas
QC Physics
Issue Date: Jan-2012
Citation: Stark , C R & Neukirch , T 2012 , ' Collisionless distribution function for the relativistic force-free Harris sheet ' Physics of Plasmas , vol 19 , no. 1 , 012115 .
Abstract: A self-consistent collisionless distribution function for the relativistic analogue of the force-free Harris sheet is presented. This distribution function is the relativistic generalization of the distribution function for the non-relativistic collisionless force-free Harris sheet recently found by Harrison and Neukirch [Phys. Rev. Lett. 102, 135003 (2009)], as it has the same dependence on the particle energy and canonical momenta. We present a detailed calculation which shows that the proposed distribution function generates the required current density profile (and thus magnetic field profile) in a frame of reference in which the electric potential vanishes identically. The connection between the parameters of the distribution function and the macroscopic parameters such as the current sheet thickness is discussed. (C) 2012 American Institute of Physics. [doi: 10.1063/1.3677268]
Version: Postprint
Status: Peer reviewed
URI: http://hdl.handle.net/10023/3154
DOI: http://dx.doi.org/10.1063/1.3677268
ISSN: 1070-664X
Type: Journal article
Rights: Copyright (2012) American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. The published article may be found at http://dx.doi.org/10.1063/1.3677268
Appears in Collections:Physics & Astronomy Research
Applied Mathematics Research
University of St Andrews Research



This item is protected by original copyright

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.

 

DSpace Software Copyright © 2002-2012  Duraspace - Feedback
For help contact: Digital-Repository@st-andrews.ac.uk | Copyright for this page belongs to St Andrews University Library | Terms and Conditions (Cookies)