Identificador persistente para citar o vincular este elemento: http://hdl.handle.net/10553/42190
Campo DC Valoridioma
dc.contributor.authorBarriga-Carrasco, Manuel D.en_US
dc.contributor.authorGonzález-Gallego, Luisen_US
dc.contributor.authorMiguel Gil, Juanen_US
dc.contributor.authorRodriguez, Rafaelen_US
dc.contributor.authorEspinosa, Guadalupeen_US
dc.contributor.otherRodriguez, Rafael-
dc.date.accessioned2018-10-19T09:50:45Z-
dc.date.available2018-10-19T09:50:45Z-
dc.date.issued2018en_US
dc.identifier.issn1070-664Xen_US
dc.identifier.urihttp://hdl.handle.net/10553/42190-
dc.description.abstractIn this work, we analyze the thermodynamic states of the helium plasma and their influence on the stopping power calculations which are needed for obtaining the energy loss of the iron beams traversing them. The analysis is made in ranges of plasma free electron densities (10(15)-10(19) cm(-3)) and temperatures (1-10 eV) of experiments with iron beams at 6 and 4.3 MeV/u energies. For this purpose, we use Saha-Boltzmann equations for local thermal equilibrium (LTE) and a collisional-radiative model for non-local thermal equilibrium (NLTE) in steady-state situation implemented in a computer code. For the highest temperatures and free electron densities, LTE and NLTE models provide quite similar results for the average ionization and ion abundances. When the opacity effects are taken into account in the NLTE simulations, the optically thick simulations provide fairly similar results to those of the LTE model. The plasma thermodynamic states have a direct impact on the calculation of the energy loss. The differences on the plasma stopping power between considering it in LTE or in NLTE may entail a 10% of the total stopping for the experiments analyzed in the electron density region of 10(18) -10(19) cm(-3). These differences can be around 27% for plasmas with smaller electron density of 10(17) cm(-3) and around 42% for plasmas with an electron density of 10(15) cm(-3). New experiments would be appreciated to be made in a future to corroborate the latest calculations.en_US
dc.languageengen_US
dc.publisher1070-664X
dc.relationDesarrollo de Modelos Físicos y Su Integración Computacional Para la Descripción Microscópica de Plasmas de Alta Densidad de Energíaen_US
dc.relationImplementation of activities described in the Roadmap to Fusion during Horizon 2020 through a Joint programme of the members of the EUROfusion consortiumen_US
dc.relationEurofusiónen_US
dc.relationAWP15-ENR-01/CEA-02en_US
dc.relation.ispartofPhysics of Plasmasen_US
dc.sourcePhysics of Plasmas [ISSN 1070-664X], v. 25 (9)en_US
dc.subject2213 Termodinámicaen_US
dc.subject.otherElectron densityen_US
dc.subject.otherEquilibrium thermodynamicsen_US
dc.subject.otherPlasmasen_US
dc.subject.otherBound statesen_US
dc.subject.otherStopping poweren_US
dc.subject.otherThermodynamic states and processesen_US
dc.titleEnergy loss of Fe ions in He plasmas at different thermodynamic statesen_US
dc.typeinfo:eu-repo/semantics/Articleen_US
dc.typeArticleen_US
dc.identifier.doi10.1063/1.5050528en_US
dc.identifier.scopus85054158909-
dc.identifier.isi000446156900057-
dcterms.isPartOfPhysics Of Plasmas
dcterms.sourcePhysics Of Plasmas[ISSN 1070-664X],v. 25 (9)
dc.contributor.authorscopusid6507061939-
dc.contributor.authorscopusid57188874806-
dc.contributor.authorscopusid55566759900-
dc.contributor.authorscopusid56314921800-
dc.contributor.authorscopusid55285592600-
dc.identifier.issue9-
dc.relation.volume25en_US
dc.investigacionIngeniería y Arquitecturaen_US
dc.type2Artículoen_US
dc.identifier.wosWOS:000446156900057-
dc.contributor.daisngid1453755-
dc.contributor.daisngid21616360-
dc.contributor.daisngid292327-
dc.contributor.daisngid799688-
dc.contributor.daisngid13599639-
dc.identifier.investigatorRIDL-1938-2017-
dc.utils.revisionen_US
dc.contributor.wosstandardWOS:Barriga-Carrasco, MD-
dc.contributor.wosstandardWOS:Gonzalez-Gallego, L-
dc.contributor.wosstandardWOS:Gil, JM-
dc.contributor.wosstandardWOS:Rodriguez, R-
dc.contributor.wosstandardWOS:Espinosa, G-
dc.date.coverdateSeptiembre 2018en_US
dc.identifier.ulpgcen_US
dc.description.sjr0,841
dc.description.jcr1,913
dc.description.sjrqQ1
dc.description.jcrqQ3
dc.description.scieSCIE
item.grantfulltextopen-
item.fulltextCon texto completo-
crisitem.author.deptGIR IUNAT: Interacción Radiación-Materia-
crisitem.author.deptIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.deptDepartamento de Física-
crisitem.author.deptGIR IUNAT: Interacción Radiación-Materia-
crisitem.author.deptIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.deptDepartamento de Física-
crisitem.author.deptGIR IUNAT: Interacción Radiación-Materia-
crisitem.author.deptIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.deptDepartamento de Física-
crisitem.author.orcid0000-0001-9006-4128-
crisitem.author.orcid0000-0002-8326-3169-
crisitem.author.orcid0000-0002-2317-7277-
crisitem.author.parentorgIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.parentorgIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.parentorgIU de Estudios Ambientales y Recursos Naturales-
crisitem.author.fullNameGil De La Fe, Juan Miguel-
crisitem.author.fullNameRodríguez Pérez, Rafael-
crisitem.author.fullNameEspinosa Vivas, Guadalupe-
crisitem.project.principalinvestigatorGil De La Fe, Juan Miguel-
crisitem.project.principalinvestigatorMartel Escobar, Pablo-
crisitem.project.principalinvestigatorMartel Escobar, Pablo-
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miniatura
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