Neutrino flux predictions for the NuMI beam

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This work was supported by the Fermi National Accelerator Laboratory under U.S. Department of Energy (DOE) Award No. DE-AC02-07CH11359 which included the MINERvA construction project. Construction support was also granted by the United States National Science Foundation (NSF) under Grant No. PHY-061...

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Autores: Aliaga, L, Kordosky, M, Golan, T, Altinok, O, Bellantoni, L, Bercellie, A, Betancourt, M, Bravar, A, Budd, H, Carneiro, MF, Dytman, S, Diaz, GA, Endress, E, Felix, J, Fields, L, Fine, R, Gago, AM, Galindo, R, Gallagher, H, Gran, R, Harris, DA, Higuera, A, Hurtado, K, Kiveni, M, Kleykamp, J, Le, T, Maher, E, Manly, S, Mann, WA, Marshall, CM, Caicedo, DAM, McFarland, KS, McGivern, CL, McGowan, AM, Messerly, B, Miller, J, Mislivec, A, Morfin, JG, Mousseau, J, Naples, D, Nelson, JK, Norrick, A, Paolone, V, Park, J, Patrick, CE, Perdue, GN, Ransome, RD, Ray, H, Ren, L, Rimal, D, Rodrigues, PA, Ruterbories, D, Schellman, H, Salinas, CJS, Falero, SS, Tice, BG, Valencia, E, Walton, T, Wolcott, J, Wospakrik, M, Zhang, D
Formato: artículo
Fecha de Publicación:2016
Institución:Consejo Nacional de Ciencia Tecnología e Innovación
Repositorio:CONCYTEC-Institucional
Lenguaje:inglés
OAI Identifier:oai:repositorio.concytec.gob.pe:20.500.12390/1205
Enlace del recurso:https://hdl.handle.net/20.500.12390/1205
https://doi.org/10.1103/PhysRevD.94.092005
Nivel de acceso:acceso abierto
Materia:Instrumentación y Detectores
Física de altas energías
Experimento (hep-ex)
https://purl.org/pe-repo/ocde/ford#1.03.01
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network_acronym_str CONC
network_name_str CONCYTEC-Institucional
repository_id_str 4689
dc.title.none.fl_str_mv Neutrino flux predictions for the NuMI beam
title Neutrino flux predictions for the NuMI beam
spellingShingle Neutrino flux predictions for the NuMI beam
Aliaga, L
Instrumentación y Detectores
Física de altas energías
Experimento (hep-ex)
https://purl.org/pe-repo/ocde/ford#1.03.01
title_short Neutrino flux predictions for the NuMI beam
title_full Neutrino flux predictions for the NuMI beam
title_fullStr Neutrino flux predictions for the NuMI beam
title_full_unstemmed Neutrino flux predictions for the NuMI beam
title_sort Neutrino flux predictions for the NuMI beam
author Aliaga, L
author_facet Aliaga, L
Kordosky, M
Golan, T
Altinok, O
Bellantoni, L
Bercellie, A
Betancourt, M
Bravar, A
Budd, H
Carneiro, MF
Dytman, S
Diaz, GA
Endress, E
Felix, J
Fields, L
Fine, R
Gago, AM
Galindo, R
Gallagher, H
Gran, R
Harris, DA
Higuera, A
Hurtado, K
Kiveni, M
Kleykamp, J
Le, T
Maher, E
Manly, S
Mann, WA
Marshall, CM
Caicedo, DAM
McFarland, KS
McGivern, CL
McGowan, AM
Messerly, B
Miller, J
Mislivec, A
Morfin, JG
Mousseau, J
Naples, D
Nelson, JK
Norrick, A
Paolone, V
Park, J
Patrick, CE
Perdue, GN
Ransome, RD
Ray, H
Ren, L
Rimal, D
Rodrigues, PA
Ruterbories, D
Schellman, H
Salinas, CJS
Falero, SS
Tice, BG
Valencia, E
Walton, T
Wolcott, J
Wospakrik, M
Zhang, D
author_role author
author2 Kordosky, M
Golan, T
Altinok, O
Bellantoni, L
Bercellie, A
Betancourt, M
Bravar, A
Budd, H
Carneiro, MF
Dytman, S
Diaz, GA
Endress, E
Felix, J
Fields, L
Fine, R
Gago, AM
Galindo, R
Gallagher, H
Gran, R
Harris, DA
Higuera, A
Hurtado, K
Kiveni, M
Kleykamp, J
Le, T
Maher, E
Manly, S
Mann, WA
Marshall, CM
Caicedo, DAM
McFarland, KS
McGivern, CL
McGowan, AM
Messerly, B
Miller, J
Mislivec, A
Morfin, JG
Mousseau, J
Naples, D
Nelson, JK
Norrick, A
Paolone, V
Park, J
Patrick, CE
Perdue, GN
Ransome, RD
Ray, H
Ren, L
Rimal, D
Rodrigues, PA
Ruterbories, D
Schellman, H
Salinas, CJS
Falero, SS
Tice, BG
Valencia, E
Walton, T
Wolcott, J
Wospakrik, M
Zhang, D
author2_role author
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dc.contributor.author.fl_str_mv Aliaga, L
Kordosky, M
Golan, T
Altinok, O
Bellantoni, L
Bercellie, A
Betancourt, M
Bravar, A
Budd, H
Carneiro, MF
Dytman, S
Diaz, GA
Endress, E
Felix, J
Fields, L
Fine, R
Gago, AM
Galindo, R
Gallagher, H
Gran, R
Harris, DA
Higuera, A
Hurtado, K
Kiveni, M
Kleykamp, J
Le, T
Maher, E
Manly, S
Mann, WA
Marshall, CM
Caicedo, DAM
McFarland, KS
McGivern, CL
McGowan, AM
Messerly, B
Miller, J
Mislivec, A
Morfin, JG
Mousseau, J
Naples, D
Nelson, JK
Norrick, A
Paolone, V
Park, J
Patrick, CE
Perdue, GN
Ransome, RD
Ray, H
Ren, L
Rimal, D
Rodrigues, PA
Ruterbories, D
Schellman, H
Salinas, CJS
Falero, SS
Tice, BG
Valencia, E
Walton, T
Wolcott, J
Wospakrik, M
Zhang, D
dc.subject.none.fl_str_mv Instrumentación y Detectores
topic Instrumentación y Detectores
Física de altas energías
Experimento (hep-ex)
https://purl.org/pe-repo/ocde/ford#1.03.01
dc.subject.es_PE.fl_str_mv Física de altas energías
Experimento (hep-ex)
dc.subject.ocde.none.fl_str_mv https://purl.org/pe-repo/ocde/ford#1.03.01
description This work was supported by the Fermi National Accelerator Laboratory under U.S. Department of Energy (DOE) Award No. DE-AC02-07CH11359 which included the MINERvA construction project. Construction support was also granted by the United States National Science Foundation (NSF) under Grant No. PHY-0619727 and by the University of Rochester. Support for participating scientists was provided by NSF and DOE (USA), Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior fundacao do Ministerio da Educacao (CAPES) and Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq) (Brazil), Consejo Nacional de Ciencia y Tecnologia (CoNaCyT) (Mexico), Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT), programs including Fondo Nacional de Desarrollo Cientifico y Tecnologico (FONDECYT) (Chile), by Consejo Nacional de Ciencia, Tecnologia e Innovacion Tecnologica (CONCYTEC), Direccion de Gestion de la Investigacion de la Pontificia Universidad Catolica del Peru (DGI-PUCP) and Instituto General de Investigacion de la Universidad Nacional de Ingenieria (IDI/IGI-UNI) (Peru), and the Latin American Center for Physics (CLAF). We thank the MINOS Collaboration for use of its near detector data. We acknowledge the dedicated work of the Fermilab staff responsible for the operation and maintenance of the beamline and detector and the Fermilab Computing Division for support of data processing.
publishDate 2016
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 2016
dc.type.none.fl_str_mv info:eu-repo/semantics/article
format article
dc.identifier.uri.none.fl_str_mv https://hdl.handle.net/20.500.12390/1205
dc.identifier.doi.none.fl_str_mv https://doi.org/10.1103/PhysRevD.94.092005
dc.identifier.isi.none.fl_str_mv 388823900001
url https://hdl.handle.net/20.500.12390/1205
https://doi.org/10.1103/PhysRevD.94.092005
identifier_str_mv 388823900001
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-nc-nd/4.0/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-nd/4.0/
dc.publisher.none.fl_str_mv American Physical Society
publisher.none.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 Publicationrp00771500rp00794500rp01057500rp01058500rp00818500rp00801500rp00807500rp00781500rp00812400rp00761500rp00821500rp00797500rp01212500rp00774500rp00791500rp00813500rp00854500rp01060500rp00789500rp00784500rp00775500rp01061500rp01059500rp01064500rp00815500rp00765400rp00783500rp00819500rp00814500rp00786500rp03124500rp00779500rp01065500rp00817500rp00793500rp00768500rp00757500rp00776500rp00799500rp00808500rp00780500rp00754500rp00759500rp01210500rp00758500rp00806500rp00802500rp00766500rp00763500rp00804500rp00769500rp00778500rp00773500rp00809500rp00810500rp00851500rp00796500rp00855500rp00822500rp00782500rp00853500Aliaga, LKordosky, MGolan, TAltinok, OBellantoni, LBercellie, ABetancourt, MBravar, ABudd, HCarneiro, MFDytman, SDiaz, GAEndress, EFelix, JFields, LFine, RGago, AMGalindo, RGallagher, HGran, RHarris, DAHiguera, AHurtado, KKiveni, MKleykamp, JLe, TMaher, EManly, SMann, WAMarshall, CMCaicedo, DAMMcFarland, KSMcGivern, CLMcGowan, AMMesserly, BMiller, JMislivec, AMorfin, JGMousseau, JNaples, DNelson, JKNorrick, APaolone, VPark, JPatrick, CEPerdue, GNRansome, RDRay, HRen, LRimal, DRodrigues, PARuterbories, DSchellman, HSalinas, CJSFalero, SSTice, BGValencia, EWalton, TWolcott, JWospakrik, MZhang, D2024-05-30T23:13:38Z2024-05-30T23:13:38Z2016https://hdl.handle.net/20.500.12390/1205https://doi.org/10.1103/PhysRevD.94.092005388823900001This work was supported by the Fermi National Accelerator Laboratory under U.S. Department of Energy (DOE) Award No. DE-AC02-07CH11359 which included the MINERvA construction project. Construction support was also granted by the United States National Science Foundation (NSF) under Grant No. PHY-0619727 and by the University of Rochester. Support for participating scientists was provided by NSF and DOE (USA), Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior fundacao do Ministerio da Educacao (CAPES) and Conselho Nacional de Desenvolvimento Cientifico e Tecnologico (CNPq) (Brazil), Consejo Nacional de Ciencia y Tecnologia (CoNaCyT) (Mexico), Comision Nacional de Investigacion Cientifica y Tecnologica (CONICYT), programs including Fondo Nacional de Desarrollo Cientifico y Tecnologico (FONDECYT) (Chile), by Consejo Nacional de Ciencia, Tecnologia e Innovacion Tecnologica (CONCYTEC), Direccion de Gestion de la Investigacion de la Pontificia Universidad Catolica del Peru (DGI-PUCP) and Instituto General de Investigacion de la Universidad Nacional de Ingenieria (IDI/IGI-UNI) (Peru), and the Latin American Center for Physics (CLAF). We thank the MINOS Collaboration for use of its near detector data. We acknowledge the dedicated work of the Fermilab staff responsible for the operation and maintenance of the beamline and detector and the Fermilab Computing Division for support of data processing.Knowledge of the neutrino flux produced by the Neutrinos at the Main Injector (NuMI) beamline is essential to the neutrino oscillation and neutrino interaction measurements of the MINERvA, MINOS+, NOvA and MicroBooNE experiments at Fermi National Accelerator Laboratory. We have produced a flux prediction which uses all available and relevant hadron production data, incorporating measurements of particle production off of thin targets as well as measurements of particle yields from a spare NuMI target exposed to a 120 GeV proton beam. The result is the most precise flux prediction achieved for a neutrino beam in the one to tens of GeV energy region. We have also compared the prediction to in situ measurements of the neutrino flux and find good agreement.Fondo Nacional de Desarrollo Científico y Tecnológico - FondecytengAmerican Physical SocietyPhysical Review Dinfo:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/4.0/Instrumentación y DetectoresFísica de altas energías-1Experimento (hep-ex)-1https://purl.org/pe-repo/ocde/ford#1.03.01-1Neutrino flux predictions for the NuMI beaminfo:eu-repo/semantics/articlereponame:CONCYTEC-Institucionalinstname:Consejo Nacional de Ciencia Tecnología e Innovacióninstacron:CONCYTEC20.500.12390/1205oai:repositorio.concytec.gob.pe:20.500.12390/12052024-05-30 16:01:44.586https://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccesshttp://purl.org/coar/access_right/c_14cbinfo:eu-repo/semantics/closedAccessmetadata only accesshttps://repositorio.concytec.gob.peRepositorio Institucional 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<Author> <DisplayName>Messerly, B</DisplayName> <Person id="rp00793" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Miller, J</DisplayName> <Person id="rp00768" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Mislivec, A</DisplayName> <Person id="rp00757" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Morfin, JG</DisplayName> <Person id="rp00776" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Mousseau, J</DisplayName> <Person id="rp00799" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Naples, D</DisplayName> <Person id="rp00808" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Nelson, JK</DisplayName> <Person id="rp00780" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Norrick, A</DisplayName> <Person id="rp00754" /> 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D</DisplayName> <Person id="rp00804" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Rodrigues, PA</DisplayName> <Person id="rp00769" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Ruterbories, D</DisplayName> <Person id="rp00778" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Schellman, H</DisplayName> <Person id="rp00773" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Salinas, CJS</DisplayName> <Person id="rp00809" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Falero, SS</DisplayName> <Person id="rp00810" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Tice, BG</DisplayName> <Person id="rp00851" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Valencia, E</DisplayName> <Person id="rp00796" /> <Affiliation> <OrgUnit> </OrgUnit> </Affiliation> </Author> <Author> <DisplayName>Walton, T</DisplayName> <Person id="rp00855" /> <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>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-nc-nd/4.0/</License> <Keyword>Instrumentación y Detectores</Keyword> <Keyword>Física de altas energías</Keyword> <Keyword>Experimento (hep-ex)</Keyword> <Abstract>Knowledge of the neutrino flux produced by the Neutrinos at the Main Injector (NuMI) beamline is essential to the neutrino oscillation and neutrino interaction measurements of the MINERvA, MINOS+, NOvA and MicroBooNE experiments at Fermi National Accelerator Laboratory. We have produced a flux prediction which uses all available and relevant hadron production data, incorporating measurements of particle production off of thin targets as well as measurements of particle yields from a spare NuMI target exposed to a 120 GeV proton beam. The result is the most precise flux prediction achieved for a neutrino beam in the one to tens of GeV energy region. We have also compared the prediction to in situ measurements of the neutrino flux and find good agreement.</Abstract> <Access xmlns="http://purl.org/coar/access_right" > </Access> </Publication> -1
score 12.791002
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