dc.contributor.author | Megias, G. D. | |
dc.contributor.author | Barbaro, M. B. | |
dc.contributor.author | Caballero, J. A. | |
dc.contributor.author | Gonzalez-Jimenez, R. | |
dc.contributor.author | Donnelly, T William | |
dc.date.accessioned | 2014-09-16T20:26:44Z | |
dc.date.available | 2014-09-16T20:26:44Z | |
dc.date.issued | 2014-09 | |
dc.date.submitted | 2014-07 | |
dc.identifier.issn | 0556-2813 | |
dc.identifier.issn | 1089-490X | |
dc.identifier.uri | http://hdl.handle.net/1721.1/89663 | |
dc.description.abstract | We present a systematic analysis of the quasielastic scaling functions computed within the relativistic mean field (RMF) theory and we propose an extension of the superscaling approach (SuSA) model based on these results. The main aim of this work is to develop a realistic and accurate phenomenological model (SuSAv2), which incorporates the different RMF effects in the longitudinal and transverse nuclear responses, as well as in the isovector and isoscalar channels. This provides a complete set of reference scaling functions to describe in a consistent way both (e,e′) processes and the neutrino/antineutrino-nucleus reactions in the quasielastic region. A comparison of the model predictions with electron and neutrino scattering data is presented. | en_US |
dc.description.sponsorship | United States. Dept. of Energy (Cooperative Agreement DE-FC02-94ER40818) | en_US |
dc.publisher | American Physical Society | en_US |
dc.relation.isversionof | http://dx.doi.org/10.1103/PhysRevC.90.035501 | en_US |
dc.rights | Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. | en_US |
dc.source | American Physical Society | en_US |
dc.title | Extensions of superscaling from relativistic mean field theory: The SuSAv2 model | en_US |
dc.type | Article | en_US |
dc.identifier.citation | Gonzalez-Jimenez, R., G. D. Megias, M. B. Barbaro, J. A. Cabellero, and T. W. Donnelly. "Extensions of superscaling from relativistic mean field theory: The SuSAv2 model." Phys. Rev. C 90, 035501 (September 2014). © 2014 American Physical Society | en_US |
dc.contributor.department | Massachusetts Institute of Technology. Center for Theoretical Physics | en_US |
dc.contributor.department | Massachusetts Institute of Technology. Department of Physics | en_US |
dc.contributor.department | Massachusetts Institute of Technology. Laboratory for Nuclear Science | en_US |
dc.contributor.mitauthor | Donnelly, T. William | en_US |
dc.relation.journal | Physical Review C | en_US |
dc.eprint.version | Final published version | en_US |
dc.type.uri | http://purl.org/eprint/type/JournalArticle | en_US |
eprint.status | http://purl.org/eprint/status/PeerReviewed | en_US |
dc.date.updated | 2014-09-15T22:00:11Z | |
dc.language.rfc3066 | en | |
dc.rights.holder | American Physical Society | |
dspace.orderedauthors | Gonzalez-Jimenez, R.; Megias, G. D.; Barbaro, M. B.; Caballero, J. A.; Donnelly, T. W. | en_US |
dc.identifier.orcid | https://orcid.org/0000-0002-3524-1432 | |
mit.license | PUBLISHER_POLICY | en_US |
mit.metadata.status | Complete | |