Determination of the neutrino fluxes in the Brookhaven wide-band beams
Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields1986Vol. 34(1), pp. 75–84
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L. Ahrens, S. H. Aronson, P. L. Connolly, Bruce Gibbard, M. J. Murtagh, S. J. Murtagh, S. Terada, D. H. White, J. L. Callas, D. Cutts, M. Diwan, J. S. Hoftun, R. E. Lanou, T. Shinkawa, Y. Kurihara, K. Amako, S. Kabe, Y. Nagashima, Y. Suzuki, S. Tatsumi, Y. Yamaguchi, K. Abe, E. W. Beier, D. Doughty, L. S. Durkin, S. M. Heagy, M. Hurley, A. K. Mann, F. M. Newcomer, Harlan R. Williams, A. York, D. Hedin, Matthias Marx, E. G. Stern
Abstract
The neutrino fluxes \ensuremath{\varphi}(E(${\ensuremath{\nu}}_{\ensuremath{\mu}}$)), \ensuremath{\varphi}(E(\ensuremath{\nu}${\ifmmode\bar\else\textasciimacron\fi{}}_{\ensuremath{\mu}}$)), and \ensuremath{\varphi}(E(${\ensuremath{\nu}}_{e}$)) 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.
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