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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


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