Neutrino flux predictions for the NuMI beam
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Neutrino flux predictions for the NuMI beam

L. Aliaga,M. Kordosky,Tomasz Golan,O. Altinok,L. Bellantoni,A. Bercellie,M. Betancourt,A. Bravar,H. Budd,M. F. Carneiro,S. Dytman,G. A. Díaz,E. Endress,J. Felix,L. Fields,Robert Fine,A. M. Gago,R. Galindo,H. Gallagher,R. Gran,D. A. Harris,A. Higuera,K. Hurtado,M. Kiveni,J. Kleykamp,T. Le,E. Maher,Steven Manly,W. A. Mann,C. M. Marshall,D. A. Martinez Caicedo,K. S. McFarland,C. L. McGivern,Aaron McGowan,B. Messerly,Jonathan Miller,A. Mislivec,J. G. Morfín,J. Mousseau,D. Naples,J. K. Nelson,A. Norrick,Nuruzzaman,V. Paolone,J. Park,Cheryl Patrick,G. N. Perdue,R. D. Ransome,H. Ray,L. Ren,D. Rimal,P. A. Rodrigues,D. Ruterbories,H. Schellman,Carlos Javier Solano Salinas,S. Sánchez Falero,B. G. Tice,E. Valencia,T. Walton,J. Wolcott,M. Wospakrik,D. Zhang,MINERνA Collaboration;L. Aliaga;M. Kordosky;Tomasz Golan;O. Altinok;L. Bellantoni;A. Bercellie;M. Betancourt;A. Bravar;H. Budd;M. F. Carneiro;S. Dytman;G. A. Díaz;E. Endress;J. Felix;L. Fields;Robert Fine;A. M. Gago;R. Galindo;H. Gallagher;R. Gran;D. A. Harris;A. Higuera;K. Hurtado;M. Kiveni;J. Kleykamp;T. Le;E. Maher;Steven Manly;W. A. Mann;C. M. Marshall;D. A. Martinez Caicedo;K. S. McFarland;C. L. McGivern;Aaron McGowan;B. Messerly;Jonathan Miller;A. Mislivec;J. G. Morfín;J. Mousseau;D. Naples;J. K. Nelson;A. Norrick;Nuruzzaman;V. Paolone;J. Park;Cheryl Patrick;G. N. Perdue;R. D. Ransome;H. Ray;L. Ren;D. Rimal;P. A. Rodrigues;D. Ruterbories;H. Schellman;Carlos Javier Solano Salinas;S. Sánchez Falero;B. G. Tice;E. Valencia;T. Walton;J. Wolcott;M. Wospakrik;D. Zhang;MINERνA Collaboration;
physical review d 2016 Vol. 94 pp. 092005-
164
collaboration2016physicalneutrino

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.

Keywords

gev beam neutrino flux numi oscillation and neutrino flux prediction flux produced measurements of particle

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DOI:
10.1103/physrevd.94.092005
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https://sciprofiles.com/publication/view/5507b3e62...

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Ref Key: collaboration2016physicalneutrino
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