Neutrino flux predictions for the NuMI beam

L. Aliaga; M. Kordosky; T. Golan; O. Altinok; L. Bellantoni; A. Bercellie; M. Betancourt; A. Bravar; H. Budd; M. F. Carneiro; S. A. Dytman; G. A. Díaz; E. Endress; J. Felix; L. Fields; R. Fine; A. Gago; R. Galindo; H. Gallagher; R. Gran; D. A. Harris; A. Higuera; K. Hurtado; M. Kiveni; J. Kleykamp; T. Le; E. Maher; S. Manly; W. A. Mann; C. M. Marshall; D. A. Martinez Caicedo; K. S. McFarland; C. L. McGivern; A. M. McGowan; B. Messerly; J. Miller; A. Mislivec; J. G. Morfín; J. Mousseau; D. Naples; J. K. Nelson; A. Norrick; NULL Nuruzzaman; V. Paolone; J. Park; C. E. Patrick; G. N. Perdue; R. D. Ransome; H. Ray; L. Ren; D. Rimal; P. A. Rodrigues; D. Ruterbories; H. Schellman; C. J. Solano Salinas; S. Sánchez Falero; B. G. Tice; E. Valencia; T. Walton; J. Wolcott; M. Wospakrik; D. Zhang

Neutrino flux predictions for the NuMI beam

L. Aliaga
, M. Kordosky
, T. Golan
, O. Altinok
, L. Bellantoni
, A. Bercellie
, M. Betancourt
, A. Bravar
, H. Budd
, M. F. Carneiro
, S. A. Dytman
, G. A. Díaz
, E. Endress
, J. Felix
, L. Fields
, R. Fine
, A. Gago
, R. Galindo
, H. Gallagher
, R. Gran

D. A. Harris, A. Higuera, K. Hurtado, M. Kiveni, J. Kleykamp, T. Le, E. Maher, S. Manly, W. A. Mann, C. M. Marshall, D. A. Martinez Caicedo, K. S. McFarland, C. L. McGivern, A. M. McGowan, B. Messerly, J. Miller, A. Mislivec, J. G. Morfín, J. Mousseau, D. Naples, J. K. Nelson, A. Norrick, NULL Nuruzzaman, V. Paolone, J. Park, C. E. Patrick, G. N. Perdue, R. D. Ransome, H. Ray, L. Ren, D. Rimal, P. A. Rodrigues, D. Ruterbories, H. Schellman, C. J. Solano Salinas, S. Sánchez Falero, B. G. Tice, E. Valencia, T. Walton, J. Wolcott, M. Wospakrik, D. Zhang

William & Mary
Fermi National Accelerator Laboratory
University of Rochester
Tufts University
Université de Genève
Centro Brasileiro de Pesquisas Físicas
University of Pittsburgh
Pontificia Universidad Católica del Perú
Universidad de Guanajuato
Northwestern University
Universidad Técnica Federico Santa María
University of Minnesota Duluth
University of Houston
Universidad Nacional de Ingenieria, Lima
Rutgers University–New Brunswick
Massachusetts College of Liberal Arts
Illinois Institute of Technology
Iowa State University
University of Florida
University of Michigan, Ann Arbor
Oregon State University
Hampton University

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135 Citas (Scopus)

Resumen

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.

Idioma original	Español
Publicación	Physical Review D
Volumen	94
Estado	Publicada - 29 nov. 2016

Citar esto

@article{a667def50e43495d959f70d9496a950a,

title = "Neutrino flux predictions for the NuMI beam",

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.",

author = "L. Aliaga and M. Kordosky and T. Golan and O. Altinok and L. Bellantoni and A. Bercellie and M. Betancourt and A. Bravar and H. Budd and Carneiro, \{M. F.\} and Dytman, \{S. A.\} and D{\'i}az, \{G. A.\} and E. Endress and J. Felix and L. Fields and R. Fine and A. Gago and R. Galindo and H. Gallagher and R. Gran and Harris, \{D. A.\} and A. Higuera and K. Hurtado and M. Kiveni and J. Kleykamp and T. Le and E. Maher and S. Manly and Mann, \{W. A.\} and Marshall, \{C. M.\} and \{Martinez Caicedo\}, \{D. A.\} and McFarland, \{K. S.\} and McGivern, \{C. L.\} and McGowan, \{A. M.\} and B. Messerly and J. Miller and A. Mislivec and Morf{\'i}n, \{J. G.\} and J. Mousseau and D. Naples and Nelson, \{J. K.\} and A. Norrick and NULL Nuruzzaman and V. Paolone and J. Park and Patrick, \{C. E.\} and Perdue, \{G. N.\} and Ransome, \{R. D.\} and H. Ray and L. Ren and D. Rimal and Rodrigues, \{P. A.\} and D. Ruterbories and H. Schellman and \{Solano Salinas\}, \{C. J.\} and \{S{\'a}nchez Falero\}, S. and Tice, \{B. G.\} and E. Valencia and T. Walton and J. Wolcott and M. Wospakrik and D. Zhang",

year = "2016",

month = nov,

day = "29",

language = "Espa{\~n}ol",

volume = "94",

journal = "Physical Review D",

issn = "2470-0010",

}

Aliaga, L, Kordosky, M, Golan, T, Altinok, O, Bellantoni, L, Bercellie, A, Betancourt, M, Bravar, A, Budd, H, Carneiro, MF, Dytman, SA, Díaz, GA, Endress, E, Felix, J, Fields, L, Fine, R, Gago, A, 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, Martinez Caicedo, DA, McFarland, KS, McGivern, CL, McGowan, AM, Messerly, B, Miller, J, Mislivec, A, Morfín, JG, Mousseau, J, Naples, D, Nelson, JK, Norrick, A, Nuruzzaman, NULL, Paolone, V, Park, J, Patrick, CE, Perdue, GN, Ransome, RD, Ray, H, Ren, L, Rimal, D, Rodrigues, PA, Ruterbories, D, Schellman, H, Solano Salinas, CJ, Sánchez Falero, S, Tice, BG, Valencia, E, Walton, T, Wolcott, J, Wospakrik, M & Zhang, D 2016, 'Neutrino flux predictions for the NuMI beam', Physical Review D, vol. 94.

TY - JOUR

T1 - Neutrino flux predictions for the NuMI beam

AU - Aliaga, L.

AU - Kordosky, M.

AU - Golan, T.

AU - Altinok, O.

AU - Bellantoni, L.

AU - Bercellie, A.

AU - Betancourt, M.

AU - Bravar, A.

AU - Budd, H.

AU - Carneiro, M. F.

AU - Dytman, S. A.

AU - Díaz, G. A.

AU - Endress, E.

AU - Felix, J.

AU - Fields, L.

AU - Fine, R.

AU - Gago, A.

AU - Galindo, R.

AU - Gallagher, H.

AU - Gran, R.

AU - Harris, D. A.

AU - Higuera, A.

AU - Hurtado, K.

AU - Kiveni, M.

AU - Kleykamp, J.

AU - Le, T.

AU - Maher, E.

AU - Manly, S.

AU - Mann, W. A.

AU - Marshall, C. M.

AU - Martinez Caicedo, D. A.

AU - McFarland, K. S.

AU - McGivern, C. L.

AU - McGowan, A. M.

AU - Messerly, B.

AU - Miller, J.

AU - Mislivec, A.

AU - Morfín, J. G.

AU - Mousseau, J.

AU - Naples, D.

AU - Nelson, J. K.

AU - Norrick, A.

AU - Nuruzzaman, NULL

AU - Paolone, V.

AU - Park, J.

AU - Patrick, C. E.

AU - Perdue, G. N.

AU - Ransome, R. D.

AU - Ray, H.

AU - Ren, L.

AU - Rimal, D.

AU - Rodrigues, P. A.

AU - Ruterbories, D.

AU - Schellman, H.

AU - Solano Salinas, C. J.

AU - Sánchez Falero, S.

AU - Tice, B. G.

AU - Valencia, E.

AU - Walton, T.

AU - Wolcott, J.

AU - Wospakrik, M.

AU - Zhang, D.

PY - 2016/11/29

Y1 - 2016/11/29

N2 - 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.

AB - 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.

M3 - Artículo

SN - 2470-0010

VL - 94

JO - Physical Review D

JF - Physical Review D

ER -