Multiple Capture Contributions In Charge Exchange Induced X-ray Spectra And Their Relevance To Astrophysical Applications

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dc.conicet.avisoEditorialThe right to Post the Version of Record (VOR) to their personal web page or their employer’s web page 12 months after publication by AIP Publishing.*
dc.conicet.organizacionConsejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico - CONICET - Bahía Blanca. Instituto de Física del Sur
dc.conicet.organizacionUniversidad Nacional del Sur. Departamento de Física
dc.conicet.organizacionMissouri University of Science and Technology
dc.conicet.paisOrganizacionArgentina
dc.conicet.paisOrganizacionArgentina
dc.conicet.paisOrganizacionEstados Unidos
dc.conicet.produccionid2785309
dc.contributor.authorOtranto, Sebastian
dc.contributor.authorOlson, R. E.
dc.date.accessioned2015-09-23T19:45:20Z
dc.date.available2015-09-23T19:45:20Z
dc.date.issued2013-04-19
dc.date.updated2016-03-30 10:35:44.97925-03
dc.description.abstractIn this work, we present theoretical line emission cross sections for Ar18+ and Ne10+ colliding on Ar for impact energies in the range 5 eV/amu-10 keV/amu which covers typical EBIT-traps as well as Solar Wind energies. The present analysis is performed by means of a 5-body classical trajectory Monte Carlo (CTMC) model which allows us to model the multiple capture contribution to the X-ray line emission spectra. Our results are contrasted to recent capture and line emission data from Berlin-EBIT, NIST and the University of Nevada Reno.es
dc.description.filFil: Otranto, Sebastian. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico - CONICET - Bahía Blanca. Instituto de Física del Sur; Argentina. Universidad Nacional del Sur. Departamento de Física; Argentina
dc.description.filFil: Olson, R. E.. Missouri University of Science and Technology; Estados Unidos
dc.formatapplication/pdfes
dc.identifier.citationOtranto, Sebastian; Olson, R. E.; Multiple Capture Contributions In Charge Exchange Induced X-ray Spectra And Their Relevance To Astrophysical Applications; American Institute of Physics; AIP Conference Proceedings; 1525; 19-4-2013; 55-59es
dc.identifier.issn0094-243Xes
dc.identifier.urihttp://hdl.handle.net/11336/2082
dc.journal.ciudadNueva Yorkes
dc.journal.pagination55-59es
dc.journal.paisEstados Unidoses
dc.journal.titleAIP Conference Proceedingses
dc.journal.volume1525es
dc.language.isoenges
dc.publisherAmerican Institute of Physicses
dc.relation.alternativeidinfo:eu-repo/semantics/altIdentifier/url/http://scitation.aip.org/content/aip/proceeding/aipcp/10.1063/1.4802289
dc.relation.alternativeidinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1063/1.4802289
dc.rightsinfo:eu-repo/semantics/openAccess*
dc.rights.urihttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/*
dc.subjectCHARGE EXCHANGEes
dc.subjectMULTIPLE CAPTUREes
dc.subjectX-RAY EMISSIONes
dc.subject.classificationAstronomíaes
dc.subject.classificationCiencias Físicases
dc.subject.classificationCIENCIAS NATURALES Y EXACTASes
dc.subject.classificationFísica Atómica, Molecular y Químicaes
dc.subject.classificationCiencias Físicases
dc.subject.classificationCIENCIAS NATURALES Y EXACTASes
dc.titleMultiple Capture Contributions In Charge Exchange Induced X-ray Spectra And Their Relevance To Astrophysical Applicationses
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:ar-repo/semantics/artículo
dc.typeinfo:eu-repo/semantics/publishedVersion

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