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Published byEvan Andrews Modified over 9 years ago
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MiniBooNE Flux Uncertainty Arising from Finite HARP Statistics Consider and e flux combined as well as e ’s from kaon decay alone. Flux uncertainty as a function of parent meson and neutrino energy. Flux uncertainty as a function of parent meson averaged over all neutrino energies. Uncertainties studied for 4 geometrical coverage as well as for forward analysis only.
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Neutrino Flux Uncertainty Achievable from 1.4M HARP Events. (4 geometrical acceptance) and e combined flux uncertainty verses neutrino energy for 5 parent meson types ( +, -, K +, K -, K 0 ) Uncertainty integrated over neutrino energy. *statistical error only
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e Flux Uncertainty Achievable from 1.4M HARP Events. (4 geometrical acceptance) e flux uncertainty from kaon decay verses neutrino energy. Uncertainty integrated over neutrino energy. *statistical error only
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HARP Forward Analysis (excluding the TPC) Statistics reduced accordingly for partially detected cones. 100% uncertainty assumed for undetected cones.
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Neutrino Flux Uncertainty Achievable from 1.4M HARP Events. (forward analysis only) and e combined flux uncertainty verses neutrino energy for 5 parent meson types ( +, -, K +, K -, K 0 ) Uncertainty integrated over neutrino energy. *statistical error only * Additional uncertainty mainly at low energies.
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e Flux Uncertainty Achievable from 1.4M HARP Events. (forward analysis only) e flux uncertainty from kaon decay verses neutrino energy. Uncertainty integrated over neutrino energy. *statistical error only * Additional uncertainty mainly at low energies.
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