Tuning the GENIE pion production model with MINERvA data

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CONCYTEC, Direccion de Gestion de la Investigacion-Pontificia Universidad Catolica del Peru (DGI-PUCP), and Vicerrectorado de Investigacion-Universidad Nacional de Ingenieria (VRI-UNI) (Peru); and by the Latin American Center for Physics (CLAF); NCN Opus Grant No. 2016/21/B/ST2/01092 (Poland). We th...

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oai_identifier_str oai:repositorio.concytec.gob.pe:20.500.12390/1177
network_acronym_str CONC
network_name_str CONCYTEC-Institucional
repository_id_str 4689
dc.title.none.fl_str_mv Tuning the GENIE pion production model with MINERvA data
title Tuning the GENIE pion production model with MINERvA data
spellingShingle Tuning the GENIE pion production model with MINERvA data
Stowell, P
Neutrino interactions
Few-GeV energies
Systematic uncertainties
title_short Tuning the GENIE pion production model with MINERvA data
title_full Tuning the GENIE pion production model with MINERvA data
title_fullStr Tuning the GENIE pion production model with MINERvA data
title_full_unstemmed Tuning the GENIE pion production model with MINERvA data
title_sort Tuning the GENIE pion production model with MINERvA data
author Stowell, P
author_facet Stowell, P
Pickering, L
Willcinson, C
Wret, C
Akbar, F
Andrade, DA
Ascencio, MV
Bellantoni, L
Bercellie, A
Betancourt, M
Bodek, A
Bravar, A
Budd, H
Caceres, G
Cai, T
Cameiro, MF
Chaves, J
da Motta, H
Dytman, SA
Diaz, GA
Felix, J
Fields, L
Filkins, A
Fine, R
Fiza, N
Galindo, R
Gallagher, H
Ghosh, A
Gran, R
Harris, DA
Henry, S
Jena, S
Jena, D
Kleykamp, J
Kordosky, M
Last, D
Le, T
Lu, XG
Maher, E
Manly, S
Mann, WA
Marshall, CM
McFarland, KS
Messerly, B
Miller, J
Morfin, JG
Mousseau, J
Naples, D
Nelson, JK
Nguyen, C
Norrick, A
Nuruzzaman
Paolone, V
Perdue, GN
Ramirez, MA
Ransome, RD
Ray, H
Rimal, D
Rodrigues, PA
Ruterbories, D
Schellman, H
Salinas, CJS
Su, H
Sultana, M
Syrotenko, VS
Valencia, E
Wolcott, J
Wospakrik, M
Yaeggy, B
Zazueta, L
Zhang, D
author_role author
author2 Pickering, L
Willcinson, C
Wret, C
Akbar, F
Andrade, DA
Ascencio, MV
Bellantoni, L
Bercellie, A
Betancourt, M
Bodek, A
Bravar, A
Budd, H
Caceres, G
Cai, T
Cameiro, MF
Chaves, J
da Motta, H
Dytman, SA
Diaz, GA
Felix, J
Fields, L
Filkins, A
Fine, R
Fiza, N
Galindo, R
Gallagher, H
Ghosh, A
Gran, R
Harris, DA
Henry, S
Jena, S
Jena, D
Kleykamp, J
Kordosky, M
Last, D
Le, T
Lu, XG
Maher, E
Manly, S
Mann, WA
Marshall, CM
McFarland, KS
Messerly, B
Miller, J
Morfin, JG
Mousseau, J
Naples, D
Nelson, JK
Nguyen, C
Norrick, A
Nuruzzaman
Paolone, V
Perdue, GN
Ramirez, MA
Ransome, RD
Ray, H
Rimal, D
Rodrigues, PA
Ruterbories, D
Schellman, H
Salinas, CJS
Su, H
Sultana, M
Syrotenko, VS
Valencia, E
Wolcott, J
Wospakrik, M
Yaeggy, B
Zazueta, L
Zhang, D
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dc.contributor.author.fl_str_mv Stowell, P
Pickering, L
Willcinson, C
Wret, C
Akbar, F
Andrade, DA
Ascencio, MV
Bellantoni, L
Bercellie, A
Betancourt, M
Bodek, A
Bravar, A
Budd, H
Caceres, G
Cai, T
Cameiro, MF
Chaves, J
da Motta, H
Dytman, SA
Diaz, GA
Felix, J
Fields, L
Filkins, A
Fine, R
Fiza, N
Galindo, R
Gallagher, H
Ghosh, A
Gran, R
Harris, DA
Henry, S
Jena, S
Jena, D
Kleykamp, J
Kordosky, M
Last, D
Le, T
Lu, XG
Maher, E
Manly, S
Mann, WA
Marshall, CM
McFarland, KS
Messerly, B
Miller, J
Morfin, JG
Mousseau, J
Naples, D
Nelson, JK
Nguyen, C
Norrick, A
Nuruzzaman
Paolone, V
Perdue, GN
Ramirez, MA
Ransome, RD
Ray, H
Rimal, D
Rodrigues, PA
Ruterbories, D
Schellman, H
Salinas, CJS
Su, H
Sultana, M
Syrotenko, VS
Valencia, E
Wolcott, J
Wospakrik, M
Yaeggy, B
Zazueta, L
Zhang, D
dc.subject.en.fl_str_mv Neutrino interactions
Few-GeV energies
Systematic uncertainties
topic Neutrino interactions
Few-GeV energies
Systematic uncertainties
description CONCYTEC, Direccion de Gestion de la Investigacion-Pontificia Universidad Catolica del Peru (DGI-PUCP), and Vicerrectorado de Investigacion-Universidad Nacional de Ingenieria (VRI-UNI) (Peru); and by the Latin American Center for Physics (CLAF); NCN Opus Grant No. 2016/21/B/ST2/01092 (Poland). We thank the MINOS Collaboration for use of its near detector data. Finally, we thank the staff of Fermilab for support of the beam line, the detector, and the computing infrastructure.
publishDate 2019
dc.date.accessioned.none.fl_str_mv 2024-05-30T23:13:38Z
dc.date.available.none.fl_str_mv 2024-05-30T23:13:38Z
dc.date.issued.fl_str_mv 2019
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/20.500.12390/1177
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1103/PhysRevD.100.072005
dc.identifier.isi.none.fl_str_mv 489827100003
url https://hdl.handle.net/20.500.12390/1177
https://doi.org/10.1103/PhysRevD.100.072005
identifier_str_mv 489827100003
dc.language.iso.none.fl_str_mv eng
language eng
dc.relation.ispartof.none.fl_str_mv Physical Review D
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
dc.rights.uri.none.fl_str_mv https://creativecommons.org/licenses/by/4.0/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/4.0/
dc.publisher.en.fl_str_mv American Physical Society
dc.source.none.fl_str_mv reponame:CONCYTEC-Institucional
instname:Consejo Nacional de Ciencia Tecnología e Innovación
instacron:CONCYTEC
instname_str Consejo Nacional de Ciencia Tecnología e Innovación
instacron_str CONCYTEC
institution CONCYTEC
reponame_str CONCYTEC-Institucional
collection CONCYTEC-Institucional
repository.name.fl_str_mv Repositorio Institucional CONCYTEC
repository.mail.fl_str_mv repositorio@concytec.gob.pe
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spelling 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, PPickering, LWillcinson, CWret, CAkbar, FAndrade, DAAscencio, MVBellantoni, LBercellie, ABetancourt, MBodek, ABravar, ABudd, HCaceres, GCai, TCameiro, MFChaves, Jda Motta, HDytman, SADiaz, GAFelix, JFields, LFilkins, AFine, RFiza, NGalindo, RGallagher, HGhosh, AGran, RHarris, DAHenry, SJena, SJena, DKleykamp, JKordosky, MLast, DLe, TLu, XGMaher, EManly, SMann, WAMarshall, CMMcFarland, KSMesserly, BMiller, JMorfin, JGMousseau, JNaples, DNelson, JKNguyen, CNorrick, ANuruzzamanPaolone, VPerdue, GNRamirez, MARansome, RDRay, HRimal, DRodrigues, PARuterbories, DSchellman, HSalinas, CJSSu, HSultana, MSyrotenko, VSValencia, EWolcott, JWospakrik, MYaeggy, BZazueta, LZhang, D2024-05-30T23:13:38Z2024-05-30T23:13:38Z2019https://hdl.handle.net/20.500.12390/1177https://doi.org/10.1103/PhysRevD.100.072005489827100003CONCYTEC, Direccion de Gestion de la Investigacion-Pontificia Universidad Catolica del Peru (DGI-PUCP), and Vicerrectorado de Investigacion-Universidad Nacional de Ingenieria (VRI-UNI) (Peru); and by the Latin American Center for Physics (CLAF); NCN Opus Grant No. 2016/21/B/ST2/01092 (Poland). We thank the MINOS Collaboration for use of its near detector data. Finally, we thank the staff of Fermilab for support of the beam line, the detector, and the computing infrastructure.Faced with unresolved tensions between neutrino interaction measurements at few-GeV neutrino energies, current experiments are forced to accept large systematic uncertainties to cover discrepancies between their data and model predictions. The widely used pion production model in genie is compared to four MINER⁢⁢A charged current pion production measurements using nuisance. Tunings, i.e., adjustments of model parameters, to help match genie to MINER⁢⁢A and older bubble chamber data are presented. We find that scattering off nuclear targets as measured in MINER⁢⁢A is not in good agreement with expectations based upon scattering off nucleon (hydrogen or deuterium) targets in existing bubble chamber data. An additional ad hoc correction for the low−2 region, where collective nuclear effects are expected to be large, is presented. While these tunings and corrections improve the agreement of genie with the data, the modeling is imperfect. The development of these tunings within the nuisance framework allows for straightforward extensions to other neutrino event generators and models, and allows omitting and including new datasets as they become available.Consejo Nacional de Ciencia, Tecnología e Innovación Tecnológica - ConcytecengAmerican Physical SocietyPhysical Review Dinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/4.0/Neutrino interactionsFew-GeV energiesSystematic uncertaintiesTuning the GENIE pion production model with MINERvA datainfo:eu-repo/semantics/articlereponame:CONCYTEC-Institucionalinstname:Consejo Nacional de Ciencia Tecnología e Innovacióninstacron:CONCYTEC#PLACEHOLDER_PARENT_METADATA_VALUE#20.500.12390/1177oai:repositorio.concytec.gob.pe:20.500.12390/11772025-09-23 13:50:23.68https://creativecommons.org/licenses/by/4.0/info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_14cbinfo:eu-repo/semantics/closedAccessmetadata only 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<Person id="rp02330" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Valencia, E</DisplayName> <Person id="rp00796" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Wolcott, J</DisplayName> <Person id="rp00822" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Wospakrik, M</DisplayName> <Person id="rp00782" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Yaeggy, B</DisplayName> <Person id="rp00816" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Zazueta, L</DisplayName> <Person id="rp02335" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Zhang, D</DisplayName> <Person id="rp00853" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> </Authors> <Editors> </Editors> <Publishers> <Publisher> <DisplayName>American Physical Society</DisplayName> <OrgUnit /> </Publisher> </Publishers> <License>https://creativecommons.org/licenses/by/4.0/</License> <Keyword>Neutrino interactions</Keyword> <Keyword>Few-GeV energies</Keyword> <Keyword>Systematic uncertainties</Keyword> <Abstract>Faced with unresolved tensions between neutrino interaction measurements at few-GeV neutrino energies, current experiments are forced to accept large systematic uncertainties to cover discrepancies between their data and model predictions. The widely used pion production model in genie is compared to four MINER⁢⁢A charged current pion production measurements using nuisance. Tunings, i.e., adjustments of model parameters, to help match genie to MINER⁢⁢A and older bubble chamber data are presented. We find that scattering off nuclear targets as measured in MINER⁢⁢A is not in good agreement with expectations based upon scattering off nucleon (hydrogen or deuterium) targets in existing bubble chamber data. An additional ad hoc correction for the low−2 region, where collective nuclear effects are expected to be large, is presented. While these tunings and corrections improve the agreement of genie with the data, the modeling is imperfect. The development of these tunings within the nuisance framework allows for straightforward extensions to other neutrino event generators and models, and allows omitting and including new datasets as they become available.</Abstract> <Access xmlns="http://purl.org/coar/access_right" > </Access> </Publication> -1
score 13.914502
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