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.

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Presentation transcript:

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.

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

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

HARP Forward Analysis (excluding the TPC) Statistics reduced accordingly for partially detected cones. 100% uncertainty assumed for undetected cones.

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.

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.