On a characteristic initial value problem in plasma physics

Bibliographic Details
Main Author: Calogero, Simone Carmelo
Publication Date: 2006
Format: Article
Language: eng
Source: Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)
Download full: http://hdl.handle.net/1822/5470
Summary: The relativistic Vlasov-Maxwell system of plasma physics is considered with initial data on a past light cone. This characteristic initial value problem arises in a natural way as a mathematical framework to study the existence of solutions isolated from incoming radiation. Various consequences of the mass-energy conservation and of the absence of incoming radiation condition are first derived assuming the existence of global smooth solutions. In the spherically symmetric case, the existence of a unique classical solution in the future of the initial cone follows by arguments similar to the case of initial data at time $t=0$. The total mass-energy of spherically symmetric solutions equals the (properly defined) mass-energy on backward and forward light cones.
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spelling On a characteristic initial value problem in plasma physicsVlasov-MaxwellInitial value problemRadiationThe relativistic Vlasov-Maxwell system of plasma physics is considered with initial data on a past light cone. This characteristic initial value problem arises in a natural way as a mathematical framework to study the existence of solutions isolated from incoming radiation. Various consequences of the mass-energy conservation and of the absence of incoming radiation condition are first derived assuming the existence of global smooth solutions. In the spherically symmetric case, the existence of a unique classical solution in the future of the initial cone follows by arguments similar to the case of initial data at time $t=0$. The total mass-energy of spherically symmetric solutions equals the (properly defined) mass-energy on backward and forward light cones.HYKE European Network - Contract nr. HPRN-CT-2002-00282.Research Council of Norway - Project nr. 160192/v30.SpringerUniversidade do MinhoCalogero, Simone Carmelo2006-032006-03-01T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfhttp://hdl.handle.net/1822/5470eng"Annales Henri Poincaré". ISSN 1424-0637. 7:2 (2006) 233-252.1424-0637The original publication is available at www.springerlink.comhttp://www.springerlink.com/content/685835h6448861lw/fulltext.pdfinfo:eu-repo/semantics/openAccessreponame:Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)instname:FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiainstacron:RCAAP2024-05-11T06:13:59Zoai:repositorium.sdum.uminho.pt:1822/5470Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireinfo@rcaap.ptopendoar:https://opendoar.ac.uk/repository/71602025-05-28T15:45:46.885043Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) - FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiafalse
dc.title.none.fl_str_mv On a characteristic initial value problem in plasma physics
title On a characteristic initial value problem in plasma physics
spellingShingle On a characteristic initial value problem in plasma physics
Calogero, Simone Carmelo
Vlasov-Maxwell
Initial value problem
Radiation
title_short On a characteristic initial value problem in plasma physics
title_full On a characteristic initial value problem in plasma physics
title_fullStr On a characteristic initial value problem in plasma physics
title_full_unstemmed On a characteristic initial value problem in plasma physics
title_sort On a characteristic initial value problem in plasma physics
author Calogero, Simone Carmelo
author_facet Calogero, Simone Carmelo
author_role author
dc.contributor.none.fl_str_mv Universidade do Minho
dc.contributor.author.fl_str_mv Calogero, Simone Carmelo
dc.subject.por.fl_str_mv Vlasov-Maxwell
Initial value problem
Radiation
topic Vlasov-Maxwell
Initial value problem
Radiation
description The relativistic Vlasov-Maxwell system of plasma physics is considered with initial data on a past light cone. This characteristic initial value problem arises in a natural way as a mathematical framework to study the existence of solutions isolated from incoming radiation. Various consequences of the mass-energy conservation and of the absence of incoming radiation condition are first derived assuming the existence of global smooth solutions. In the spherically symmetric case, the existence of a unique classical solution in the future of the initial cone follows by arguments similar to the case of initial data at time $t=0$. The total mass-energy of spherically symmetric solutions equals the (properly defined) mass-energy on backward and forward light cones.
publishDate 2006
dc.date.none.fl_str_mv 2006-03
2006-03-01T00:00:00Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
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status_str publishedVersion
dc.identifier.uri.fl_str_mv http://hdl.handle.net/1822/5470
url http://hdl.handle.net/1822/5470
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv "Annales Henri Poincaré". ISSN 1424-0637. 7:2 (2006) 233-252.
1424-0637
The original publication is available at www.springerlink.com
http://www.springerlink.com/content/685835h6448861lw/fulltext.pdf
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