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Record W1632528017

The Cauchy problem for the 3D relativistic Vlasov-Maxwell system and its Darwin approximation

2010· article· en· W1632528017 on OpenAlexfundno aff
Reinel Sospedra‐Alfonso

Bibliographic record

VenueUVic’s Research and Learning Repository (University of Victoria) · 2010
Typearticle
Languageen
FieldMathematics
TopicGas Dynamics and Kinetic Theory
Canadian institutionsnot available
FundersNatural Sciences and Engineering Research Council of CanadaUniversity of Victoria
KeywordsMaxwell's equationsCauchy problemPhysicsRelativistic particleMathematicsInitial value problemMathematical physicsMathematical analysisClassical mechanicsQuantum mechanicsElectron
DOInot available

Abstract

fetched live from OpenAlex

The relativistic Vlasov-Maxwell system (RVM for short) is a kinetic model that
\narises in plasma physics and describes the time evolution of an ensemble of charged
\nparticles that interact only through their self-induced electromagnetic field. Collisions among the particles are neglected and they are assumed to move at speeds comparable to the speed of light. If the particles are allowed to move in the three dimensional space, then the main open problem concerning this system is to prove (or disprove) that solutions with sufficiently smooth Cauchy data do not develop singularities in finite time. Since the RVM system is essential in the study of dilute hot plasmas, much effort has been directed to the solution of its Cauchy problem. The underlying hyperbolic nature of the Maxwell equations and their nonlinear coupling with the Vlasov equation amount for the challenges imposed by this system.
\nIn this thesis, we show that solutions of the RVM system with smooth, compactly
\nsupported Cauchy data develop singularities only if the charge density blows-up in
\nfinite time. In particular, solutions can not break-down due to shock formations, since
\nin this case scenario the solution would remain bounded while its derivative blows-up.
\nOn the other hand, if the transversal component of the displacement current
\nis neglected from the Maxwell equations, then the RVM system reduces to the socalled
\nrelativistic Vlasov-Darwin (RVD) system. The latter has useful applications in numeric simulations of collisionless plasma, since the hyperbolic RVM is now reduced
\nto a more tractable elliptic system while preserving a fully coupled magnetic field. As
\nfor the RVM system, the main open problem for the RVD system is to prove whether
\nclassical solutions with unrestricted Cauchy data exist globally in time.
\nIn the second part of this thesis, we show that classical solutions of the RVD system
\nexist provided the Cauchy datum satisfies some suitable smallness assumption. The
\nproof presented here does not require estimates derived from the conservation of the total energy nor those on the transversal component of the electric field. These have been crucial in previous results concerning the RVD system. Instead, we exploit the potential formulation of the model equations. In particular, the Vlasov equation is rewritten in terms of the generalized variables and coupled with the equations satisfied by the scalar and vector Darwin potentials. This allows to use standard estimates for singular integrals and a recursive method to produce the existence of local in time classical solutions. Hence, by means of a bootstrap argument, we show that such solutions can be made global in time provided the Cauchy data is sufficiently small.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.003
metaresearch head score (Gemma)0.001
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesScience and technology studies
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Theoretical or conceptual · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.809
Threshold uncertainty score0.999

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0030.001
Meta-epidemiology (narrow)0.0000.000
Meta-epidemiology (broad)0.0000.000
Bibliometrics0.0000.000
Science and technology studies0.0020.000
Scholarly communication0.0000.000
Open science0.0000.000
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0000.000

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.024
GPT teacher head0.266
Teacher spread0.243 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

Study designTheoretical or conceptual
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations2
Published2010
Admission routes1
Has abstractyes

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