2011
DOI: 10.1088/0951-7715/24/12/004
|View full text |Cite
|
Sign up to set email alerts
|

Instability of nonmonotone magnetic equilibria of the relativistic Vlasov–Maxwell system

Abstract: We consider the question of linear instability of an equilibrium of the Relativistic Vlasov-Maxwell (RVM) System that has a strong magnetic field. Standard instability results deal with systems where there are fewer particles with higher energies. In this paper we extend those results to the class of equilibria for which the number of particles does not depend monotonically on the energy. Without the standard sign assumptions, the analysis becomes significantly more involved.

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1

Citation Types

0
25
0

Year Published

2011
2011
2022
2022

Publication Types

Select...
4
1

Relationship

3
2

Authors

Journals

citations
Cited by 5 publications
(25 citation statements)
references
References 26 publications
0
25
0
Order By: Relevance
“…Two notable later results are [6,11]. We refer to [1] for additional references. The current result continues a program initiated by Lin and Strauss [9,10] and continued by the first author [1,2].…”
Section: Previous Resultsmentioning
confidence: 92%
See 3 more Smart Citations
“…Two notable later results are [6,11]. We refer to [1] for additional references. The current result continues a program initiated by Lin and Strauss [9,10] and continued by the first author [1,2].…”
Section: Previous Resultsmentioning
confidence: 92%
“…is the linearised Vlasov transport operator. We then invert (1.13) by applying λ (λ + D) −1 , which is an ergodic averaging operator along the trajectories of D (depending upon λ as a parameter), see [1,Eq. (2.10)].…”
Section: Resultsmentioning
confidence: 99%
See 2 more Smart Citations
“…There are two parallel approaches for inverting this equation in order to obtain an expression for f ± . In the first, which can be found in [1], we integrate (2.3) along the trajectories (X ± (s; x, v), V ± (s; x, v)) of the vectorfields D ± in phase space, which satisfẏ…”
mentioning
confidence: 99%