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dc.contributor.author Cariatore, Nelson Daniel
dc.contributor.author Otranto, Sebastián
dc.contributor.author Olson, R.
dc.date.available 2018-10-11T20:59:59Z
dc.date.issued 2016-06
dc.identifier.citation Cariatore, Nelson Daniel; Otranto, Sebastián; Olson, R.; Reply to "comment on 'Classical description of H(1s) and H∗(n=2) for cross-section calculations relevant to charge-exchange diagnostics'"; American Physical Society; Physical Review A: Atomic, Molecular and Optical Physics; 93; 6; 6-2016; 667021-667025
dc.identifier.issn 1050-2947
dc.identifier.uri http://hdl.handle.net/11336/62270
dc.description.abstract In reply to the Comment of Jorge et al. [Phys. Rev. A 93, 066701 (2016)], we agree and reconfirm that the alternative classical trajectory Monte Carlo method (called hydrogenic-Z-CTMC) radial distributions for H∗(n = 2) we recently published are not stable in time. However, we show that such lack of stability which is more noticeable for H(2s) than for H(2p) is due to the initialization procedure employed and not to the hydrogenic-Z-CTMC method itself. A new set of completely stable hydrogenic-Z-CTMC calculations for H∗(n = 2) is introduced and found in very good agreement with standard microcanonical results reinforcing our previous findings. A second criticism of Jorge et al. concerning the number of components in hydrogenic-ZCTMC with n > 1 for H(1s) is shown not to have a significant impact on relative (n,l) populations in the final state.
dc.format application/pdf
dc.language.iso eng
dc.publisher American Physical Society
dc.rights info:eu-repo/semantics/restrictedAccess
dc.rights.uri https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.subject charge exchange
dc.subject line emission cross sections
dc.subject ctmc
dc.subject.classification Astronomía
dc.subject.classification Ciencias Físicas
dc.subject.classification CIENCIAS NATURALES Y EXACTAS
dc.title Reply to "comment on 'Classical description of H(1s) and H∗(n=2) for cross-section calculations relevant to charge-exchange diagnostics'"
dc.type info:eu-repo/semantics/article
dc.type info:ar-repo/semantics/artículo
dc.type info:eu-repo/semantics/publishedVersion
dc.date.updated 2018-10-08T17:58:50Z
dc.journal.volume 93
dc.journal.number 6
dc.journal.pagination 667021-667025
dc.journal.pais Estados Unidos
dc.journal.ciudad Nueva York
dc.description.fil Fil: Cariatore, Nelson Daniel. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Bahía Blanca. Instituto de Física del Sur. Universidad Nacional del Sur. Departamento de Física. Instituto de Física del Sur; Argentina
dc.description.fil Fil: Otranto, Sebastián. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Bahía Blanca. Instituto de Física del Sur. Universidad Nacional del Sur. Departamento de Física. Instituto de Física del Sur; Argentina
dc.description.fil Fil: Olson, R.. University of Missouri; Estados Unidos
dc.journal.title Physical Review A: Atomic, Molecular and Optical Physics
dc.relation.alternativeid info:eu-repo/semantics/altIdentifier/url/http://journals.aps.org/pra/abstract/10.1103/PhysRevA.93.066702
dc.relation.alternativeid info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1103/PhysRevA.93.066702
dc.conicet.fuente unificacion


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info:eu-repo/semantics/restrictedAccess Excepto donde se diga explícitamente, este item se publica bajo la siguiente descripción: Creative Commons Attribution-NonCommercial-ShareAlike 2.5 Unported (CC BY-NC-SA 2.5)