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Determination of the neutrino fluxes in the Brookhaven wide-band beams

L. A. Ahrens, S. H. Aronson, P. L. Connolly, B. G. Gibbard, M. J. Murtagh, S. J. Murtagh, S. Terada, and D. H. White

J. L. Callas, D. Cutts, M. Diwan, J. S. Hoftun, R. E. Lanou, and T. Shinkawa

Y. Kurihara

K. Amako and S. Kabe

Y. Nagashima, Y. Suzuki, S. Tatsumi, and Y. Yamaguchi

K. Abe, E. W. Beier, D. C. Doughty, L. S. Durkin, S. M. Heagy, M. Hurley, A. K. Mann, F. M. Newcomer, H. H. Williams et al.

D. Hedin, M. D. Marx, and E. Stern

  • Physics Department, Brookhaven National Laboratory, Upton, New York 11973

  • Department of Physics, Brown University, Providence, Rhode Island 02912

  • Department of Physics, Hiroshima University, Hiroshima 730, Japan

  • National Laboratory for High Energy Physics (KEK), Ibaraki-ken 305, Japan

  • Physics Department, Osaka University, Toyanaka, Osaka 560, Japan

and T. York

  • Department of Physics, University of Pennsylvania, Philadelphia, Pennsylvania 19104

  • Department of Physics, State University of New York at Stony Brook, Stony Brook, New York 11794

Phys. Rev. D 34, 75 – Published 1 July, 1986

DOI: https://doi.org/10.1103/PhysRevD.34.75

Abstract

The neutrino fluxes φ(E(νμ)), φ(E(ν¯μ)), and φ(E(νe)) in the Brookhaven Alternating Gradient Synchrotron wide-band beams have been determined by measurements of quasielastic interactions observed in a massive, high-resolution detector. These fluxes are accurately reproduced by Monte Carlo calculations.

References (13)

  1. L. A. Ahrens et al., Phys. Rev. Lett. 51, 1514 (1983); , ibid. 54, 18 (1985).
  2. K. Abe et al., Phys. Rev. Lett. 56, 1107 (1986).
  3. L. A. Ahrens et al., Phys. Rev. D 31, 2732 (1985).
  4. N. Baker et al., Phys. Rev. D 23, 2499 (1981); K. L. Miller et al., ibid. 26, 537 (1982); T. Kitagaki et al., ibid. 28, 436 (1983).
  5. W. T. Weng, IEEE Trans. Nucl. Sci. NS - 30, 2956 (1983); W. T. Weng et al.., BNL Report No. 51310, 1979 (unpublished).
  6. The literature on neutrino beams and magnetic-horn design is sparse. A high-intensity neutrino beam was described in M. Giesch et al., Nucl. Instrum. Methods 20, 58 (1963), where an estimate of the expected neutrino flux was made. The neutrino beam at the Brookhaven AGS has used a horn geometry which was initially described in R. Palmer, Proceedings of an Informal Conference on Experimental Neutrino Physics, CERN, 1965, edited by C. Franzinetti (CERN Report No. 65-32, 1965).
  7. A detailed presentation of the quasielastic cross sections can be found in C. H. Llewellyn Smith, Phys. Rep. 3 C, 262 (1972). The vector and axial-vector masses used by us were MV=0.84 GeV and MA=1.03 GeV. Corrections for Pauli exclusion and Fermi momentum are treated in J. S. Bell and C. H. Llewellyn Smith, Nucl. Phys. B 28, 317 (1971); J. Mougey et al., A 262, 461 (1976).
  8. C. Visser, NUBEAM_, a neutrino-beam simulator, Hydra Applications Library, CERN, 1979. This program was modified extensively by R. Carlini, Los Alamos National Laboratory. The program and input data appropriate for a 28-GeV proton beam may be obtained from D. H. White, Physics Department, Brookhaven National Laboratory, Upton, New York 11973.
  9. Particle Data Group, Rev. Mod. Phys. 56, S1 (1984) A. S. Carroll et al., Phys. Lett. 80 B, 319 (1979).
  10. J. R. Sanford and C. L. Wang, BNL Report No. 11479, 1967 (unpublished).
  11. H. Grote, R. Hagedorn, and J. Ranft, CERN report, 1970 (unpublished).
  12. D. H. White, BNL Report No. 36278, OG 793, 1985 (unpublished).
  13. G. Bunce, BNL Report No. 50874, 1978 (unpublished).

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