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Charged-current inclusive neutrino cross sections in the SuperScaling model

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dc.book.title9th International Physics Conference of the Balkan Physical Union (BPU-9)
dc.contributor.authorIvanov, M. V.
dc.contributor.authorMegías, G. D.
dc.contributor.authorGonzález Jiménez, Raúl
dc.contributor.authorMoreno Díaz, Óscar
dc.contributor.authorBárbaro, M. B.
dc.contributor.authorCaballero, J. A.
dc.contributor.authorDonnelly, T. W.
dc.contributor.authorAntonov, A. N.
dc.contributor.authorMoya de Guerra, Elvira
dc.contributor.authorUdías Moinelo, José Manuel
dc.date.accessioned2023-06-18T07:15:23Z
dc.date.available2023-06-18T07:15:23Z
dc.date.issued2016
dc.description© 2016 AIP Publishing LLC. ISSN: 0094-243X International Physics Conference of the Balkan-Physical-Union (BPU)(9. 2015. Estambul, Turquía). This work was partially supported by INFN under project MANYBODY, by Spanish DGI and FEDER funds (FIS2011-28738-C02-01, FPA2013-41267), by the Junta de Andalucia, by the Spanish Consolider-Ingenio 2000 program CPAN (CSD2007-00042), by the Campus of Excellence International (CEI) of Moncloa project (Madrid) and Andalucia Tech, by the Bulgarian National Science Fund under contracts No. DFNI-T02/19 and DFNI-E02/6. R.G.J. acknowledges financial help from the Interuniversity Attraction Poles Programme initiated by the Belgian Science Policy Office.
dc.description.abstractSuperScaling model (SuSA) predictions to neutrino-induced charged-current pi(+) production in the Delta-resonance region are explored under MiniBooNE experimental conditions. The SuSA charged-current pi(+) results are in good agreement with data on neutrino flux-averaged double-differential cross sections. The SuSA model for quasielastic scattering and its extension to the pion production region are used for predictions of charged-current inclusive neutrino-nucleus cross sections. Results are also compared with the T2K experimental data for inclusive scattering.
dc.description.departmentDepto. de Estructura de la Materia, Física Térmica y Electrónica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.sponsorshipINFN
dc.description.sponsorshipSpanish DGI
dc.description.sponsorshipFEDER funds
dc.description.sponsorshipJunta de Andalucia
dc.description.sponsorshipSpanish Consolider-Ingenio 2000
dc.description.sponsorshipCampus of Excellence International (CEI)
dc.description.sponsorshipBulgarian National Science Fund
dc.description.sponsorshipBelgian Science Policy Office
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/38496
dc.identifier.doi10.1063/1.4944128
dc.identifier.isbn978-0-7354-1369-6
dc.identifier.officialurlhttp://dx.doi.org/10.1063/1.4944128
dc.identifier.relatedurlhttp://scitation.aip.org/
dc.identifier.urihttps://hdl.handle.net/20.500.14352/24879
dc.issue.number1722
dc.language.isoeng
dc.publisherAmer Inst Physics
dc.relation.ispartofseriesAIP Conference Proceedings
dc.relation.projectIDMANYBODY
dc.relation.projectIDFIS2011-28738-C02-01
dc.relation.projectIDFPA2013-41267
dc.relation.projectIDCPAN (CSD2007-00042)
dc.relation.projectIDMoncloa project (Madrid) and Andalucia Tech
dc.relation.projectIDDFNI-T02/19
dc.relation.projectIDDFNI-E02/6. R.G.J.
dc.relation.projectIDInteruniversity Attraction Poles Programme
dc.rights.accessRightsopen access
dc.subject.cdu539.1
dc.subject.keywordNucleus scattering
dc.subject.ucmFísica nuclear
dc.subject.unesco2207 Física Atómica y Nuclear
dc.titleCharged-current inclusive neutrino cross sections in the SuperScaling model
dc.typebook part
dc.volume.number1722
dcterms.references[1] K. Abe et al. (T2K Collaboration), Phys. Rev. D 87, p. 092003 (2013). [2] J. E. Amaro et al., Phys. Rev. C 71, p. 015501 (2005). [3] A. A. Aguilar-Arevalo et al. (MiniBooNE Collaboration), Phys. Rev. D 83, p. 052007 (2011). [4] T. W. Donnelly and I. Sick, Phys. Rev. Lett. 82, p. 3212 (1999). [5] T. W. Donnelly and I. Sick, Phys. Rev. C 60, p. 065502 (1999). [6] W. M. Alberico et al., Phys. Rev. C 38, p. 1801 (1988). [7] M. B. Barbaro, R. Cenni, A. D. Pace, T. W. Donnelly, and A. Molinari, Nucl. Phys. A 643, p. 137 (1998). [8] J. Jourdan, Nucl. Phys. A 603, p. 117 (1996). [9] M. B. Barbaro, J. A. Caballero, T. W. Donnelly, , and C. Maieron, Phys. Rev. C 69, p. 035502 (2004). [10] C. Maieron et al., Phys. Rev. C 80, p. 035504 (2009). [11] M. V. Ivanov et al., Phys. Lett. B 711, p. 178 (2012). [12] C. Maieron, T. W. Donnelly, and I. Sick, Phys. Rev. C 65, p. 025502 (2002). [13] Y. Umino and J. M. Udias, Phys. Rev. C 52, p. 3399 (1995). [14] L. Alvarez-Ruso, S. K. Singh, and M. J. V. Vacas, Phys. Rev. C 59, p. 3386 (1999). [15] E. A. Paschos, J.-Y. Yu, and M. Sakuda, Phys. Rev. D 69, p. 014013 (2004). [16] G. D. Megias et al., Phys. Rev. D 89, p. 093002 (2014).
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