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

dc.creatorOtranto, Sebastian
dc.creatorOlson, R. E.
dc.date.accessioned2015-09-23T19:45:20Z
dc.date.accessioned2018-11-06T13:44:03Z
dc.date.available2015-09-23T19:45:20Z
dc.date.available2018-11-06T13:44:03Z
dc.date.created2015-09-23T19:45:20Z
dc.date.issued2013-04-19
dc.identifierOtranto, 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; 55-59
dc.identifier0094-243X
dc.identifierhttp://hdl.handle.net/11336/2082
dc.identifier.urihttp://repositorioslatinoamericanos.uchile.cl/handle/2250/1878716
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.
dc.languageeng
dc.publisherAmerican Institute of Physics
dc.relationinfo:eu-repo/semantics/altIdentifier/url/http://scitation.aip.org/content/aip/proceeding/aipcp/10.1063/1.4802289
dc.relationinfo:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1063/1.4802289
dc.rightshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.rightsinfo:eu-repo/semantics/openAccess
dc.subjectCharge exchange
dc.subjectX-ray emission
dc.subjectMultiple capture
dc.titleMultiple Capture Contributions In Charge Exchange Induced X-ray Spectra And Their Relevance To Astrophysical Applications
dc.typeArtículos de revistas
dc.typeArtículos de revistas
dc.typeArtículos de revistas


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