Multiple ionization effects in x-ray emission induced by heavy ions

Detalhes bibliográficos
Autor(a) principal: Czarnota,M.
Data de Publicação: 2006
Outros Autores: Pajek,M., Banas,D., Dousse,J.-Cl., Maillard,Y.-P., Mauron,O., Raboud,P. A., Berset,M., Chmielewska,D., Rzadkiewicz,J., Sujkowski,Z., Hoszowska,J., Slabkowska,K., Polasik,M.
Tipo de documento: Artigo
Idioma: eng
Título da fonte: Brazilian Journal of Physics
Texto Completo: http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332006000400013
Resumo: The x-ray satellite structure of Pd Lalpha1,2(L3M4,5) transition excited by an impact of O7+ and Ne6+ ions with energies 279 and 178 MeV, respectively, which were measured using a high-resolution von Hamos crystal spectrometer, is discussed in terms of the multi-configuration Dirac-Fock (MCDF) calculations. We demonstrate, by using the arguments of the general central limit theorem (GCLT), that a structure of complex M-shell satellites of Pd Lalpha1,2(M-m) transitions for a higher number of spectator vacancies (m > 4), which consists of hundreds of thousands of individual x-ray transitions as obtained from the MCDF calculations, can be well described by a single Voigtian profile. The Lorentzian width of such Voigtian line can be well modeled by using the results of the MCDF calculations for simpler configurations with a number of vacancies m < 4 . This method allows one to describe realistically a complex structure of M-shell satellites, thus extending the applicability of the MCDF calculations, which are limited by an increasing complexity of numerical calculations.
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spelling Multiple ionization effects in x-ray emission induced by heavy ionsMultiple ionizationX-ray satellite structureMCDF calculationsThe x-ray satellite structure of Pd Lalpha1,2(L3M4,5) transition excited by an impact of O7+ and Ne6+ ions with energies 279 and 178 MeV, respectively, which were measured using a high-resolution von Hamos crystal spectrometer, is discussed in terms of the multi-configuration Dirac-Fock (MCDF) calculations. We demonstrate, by using the arguments of the general central limit theorem (GCLT), that a structure of complex M-shell satellites of Pd Lalpha1,2(M-m) transitions for a higher number of spectator vacancies (m > 4), which consists of hundreds of thousands of individual x-ray transitions as obtained from the MCDF calculations, can be well described by a single Voigtian profile. The Lorentzian width of such Voigtian line can be well modeled by using the results of the MCDF calculations for simpler configurations with a number of vacancies m < 4 . This method allows one to describe realistically a complex structure of M-shell satellites, thus extending the applicability of the MCDF calculations, which are limited by an increasing complexity of numerical calculations.Sociedade Brasileira de Física2006-06-01info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersiontext/htmlhttp://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332006000400013Brazilian Journal of Physics v.36 n.2b 2006reponame:Brazilian Journal of Physicsinstname:Sociedade Brasileira de Física (SBF)instacron:SBF10.1590/S0103-97332006000400013info:eu-repo/semantics/openAccessCzarnota,M.Pajek,M.Banas,D.Dousse,J.-Cl.Maillard,Y.-P.Mauron,O.Raboud,P. A.Berset,M.Chmielewska,D.Rzadkiewicz,J.Sujkowski,Z.Hoszowska,J.Slabkowska,K.Polasik,M.eng2006-07-31T00:00:00Zoai:scielo:S0103-97332006000400013Revistahttp://www.sbfisica.org.br/v1/home/index.php/pt/ONGhttps://old.scielo.br/oai/scielo-oai.phpsbfisica@sbfisica.org.br||sbfisica@sbfisica.org.br1678-44480103-9733opendoar:2006-07-31T00:00Brazilian Journal of Physics - Sociedade Brasileira de Física (SBF)false
dc.title.none.fl_str_mv Multiple ionization effects in x-ray emission induced by heavy ions
title Multiple ionization effects in x-ray emission induced by heavy ions
spellingShingle Multiple ionization effects in x-ray emission induced by heavy ions
Czarnota,M.
Multiple ionization
X-ray satellite structure
MCDF calculations
title_short Multiple ionization effects in x-ray emission induced by heavy ions
title_full Multiple ionization effects in x-ray emission induced by heavy ions
title_fullStr Multiple ionization effects in x-ray emission induced by heavy ions
title_full_unstemmed Multiple ionization effects in x-ray emission induced by heavy ions
title_sort Multiple ionization effects in x-ray emission induced by heavy ions
author Czarnota,M.
author_facet Czarnota,M.
Pajek,M.
Banas,D.
Dousse,J.-Cl.
Maillard,Y.-P.
Mauron,O.
Raboud,P. A.
Berset,M.
Chmielewska,D.
Rzadkiewicz,J.
Sujkowski,Z.
Hoszowska,J.
Slabkowska,K.
Polasik,M.
author_role author
author2 Pajek,M.
Banas,D.
Dousse,J.-Cl.
Maillard,Y.-P.
Mauron,O.
Raboud,P. A.
Berset,M.
Chmielewska,D.
Rzadkiewicz,J.
Sujkowski,Z.
Hoszowska,J.
Slabkowska,K.
Polasik,M.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.author.fl_str_mv Czarnota,M.
Pajek,M.
Banas,D.
Dousse,J.-Cl.
Maillard,Y.-P.
Mauron,O.
Raboud,P. A.
Berset,M.
Chmielewska,D.
Rzadkiewicz,J.
Sujkowski,Z.
Hoszowska,J.
Slabkowska,K.
Polasik,M.
dc.subject.por.fl_str_mv Multiple ionization
X-ray satellite structure
MCDF calculations
topic Multiple ionization
X-ray satellite structure
MCDF calculations
description The x-ray satellite structure of Pd Lalpha1,2(L3M4,5) transition excited by an impact of O7+ and Ne6+ ions with energies 279 and 178 MeV, respectively, which were measured using a high-resolution von Hamos crystal spectrometer, is discussed in terms of the multi-configuration Dirac-Fock (MCDF) calculations. We demonstrate, by using the arguments of the general central limit theorem (GCLT), that a structure of complex M-shell satellites of Pd Lalpha1,2(M-m) transitions for a higher number of spectator vacancies (m > 4), which consists of hundreds of thousands of individual x-ray transitions as obtained from the MCDF calculations, can be well described by a single Voigtian profile. The Lorentzian width of such Voigtian line can be well modeled by using the results of the MCDF calculations for simpler configurations with a number of vacancies m < 4 . This method allows one to describe realistically a complex structure of M-shell satellites, thus extending the applicability of the MCDF calculations, which are limited by an increasing complexity of numerical calculations.
publishDate 2006
dc.date.none.fl_str_mv 2006-06-01
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332006000400013
url http://old.scielo.br/scielo.php?script=sci_arttext&pid=S0103-97332006000400013
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv 10.1590/S0103-97332006000400013
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv text/html
dc.publisher.none.fl_str_mv Sociedade Brasileira de Física
publisher.none.fl_str_mv Sociedade Brasileira de Física
dc.source.none.fl_str_mv Brazilian Journal of Physics v.36 n.2b 2006
reponame:Brazilian Journal of Physics
instname:Sociedade Brasileira de Física (SBF)
instacron:SBF
instname_str Sociedade Brasileira de Física (SBF)
instacron_str SBF
institution SBF
reponame_str Brazilian Journal of Physics
collection Brazilian Journal of Physics
repository.name.fl_str_mv Brazilian Journal of Physics - Sociedade Brasileira de Física (SBF)
repository.mail.fl_str_mv sbfisica@sbfisica.org.br||sbfisica@sbfisica.org.br
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