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dc.contributor.authorZaidi, F.
dc.contributor.authorRuiz Simó, Ignacio Luis 
dc.date.accessioned2022-04-07T11:26:51Z
dc.date.available2022-04-07T11:26:51Z
dc.date.issued2022-02-28
dc.identifier.citationF. Zaidi, V. Ansari, M. Sajjad Athar, H. Haider, I. Ruiz Simo, and S. K. Singh Phys. Rev. D 105, 033010 [https://doi.org/10.1103/PhysRevD.105.033010]es_ES
dc.identifier.urihttp://hdl.handle.net/10481/74217
dc.descriptionF. Z. is thankful to the Council of Scientific and Industrial Research (CSIR), India, for providing the research associate fellowship No. 09/112(0622)2K19 EMR-I. M. S. A. is thankful to the Department of Science and Technology (DST), Government of India for providing financial assistance under Grant No. SR/MF/PS- 01/2016-AMU/G. I. R. S. acknowledges support from project No. PID2020–114767 GB-I00 funded by MCIN/ AEI/10.13039/501100011033, from project No. A-FQM- 390-UGR20 funded by FEDER/Junta de Andalucia- Consejeria de Transformacion Economica, Industria, Conocimiento y Universidades, and by Junta de Andalucia (Grant No. FQM-225).es_ES
dc.description.abstractThe nuclear medium effects are studied in the ντ/¯ντ interactions from nuclei in the deep inelastic scattering region and applied to the 40Ar nucleus to obtain the scattering cross sections in the energy region of the proposed DUNE experiment. The free nucleon structure functions [FiN(x,Q2); (i=1–5)] have been calculated at the next-to-leading order using Martin–Motylinski–Harland-Lang–Thorne 2014 as well as the Coordinated Theoretical-Experimental Project on QCD parametrizations for parton distribution functions (PDFs) and including the effect of perturbative and nonperturbative QCD corrections [Ansari et al., Phys. Rev. D 102, 113007 (2020)]. These free nucleon structure functions are then convoluted with the nucleon spectral function in the nucleus to obtain the nuclear structure functions [FiA(x,Q2); (i=1–5)]. The nucleon spectral function takes into account the Fermi motion and the binding energy of the nucleons as well as the nucleon correlations within the nucleus. These nuclear structure functions are then used to calculate the deep inelastic scattering cross sections. Moreover, the contribution of π and ρ mesons as well as the corrections due to the shadowing and antishadowing effects in the relevant kinematic region of the Bjorken variable x are also included. The numerical results for the nuclear structure functions and scattering cross sections have been presented and compared with the results obtained in the phenomenological approach using nuclear PDFs from nCTEQ15 and nCTEQnu.es_ES
dc.description.sponsorshipJunta de Andalucía-Consejería de Transformacion Económica, Industria, Conocimiento y Universidadeses_ES
dc.description.sponsorshipDepartment of Science and Technology, Ministry of Science and Technology, India A-FQM-390-UGR20, MCIN/AEI/10.13039/501100011033, PID2020–114767 GB-I00, SR/MF/PS-01/2016-AMU/Ges_ES
dc.description.sponsorshipCouncil of Scientific and Industrial Research, India 09/112(0622)2K19 EMR-Ies_ES
dc.description.sponsorshipEuropean Regional Development Fundes_ES
dc.description.sponsorshipJunta de Andalucía FQM-225es_ES
dc.language.isoenges_ES
dc.publisherAmerican Physical Societyes_ES
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 España*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/*
dc.titleNuclear medium effects in the deep inelastic ντ/¯ντ−40Ar scattering at DUNE energieses_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.rights.accessRightsinfo:eu-repo/semantics/openAccesses_ES
dc.identifier.doi10.1103/PhysRevD.105.033010
dc.type.hasVersioninfo:eu-repo/semantics/publishedVersiones_ES


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