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2012

Neutrino energy reconstruction problems and neutrino oscillations

Martini, M., Ericson, M., Chanfray, G.

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We discuss the accuracy of the usual procedure for neutrino energy reconstruction which is based on the quasielastic kinematics.

Our results are described in terms of a probability distribution for a real neutrino energy value.
Several factors are responsible of the deviations from the reconstructed value.
The main one is the multinucleon component of the neutrino interaction which in the case of Cherenkov detectors enters as a quasielastic cross section, increasing the mean neutrino energy which can differ appreciably from the reconstructed value.

Neutrino energy reconstruction problems and neutrino oscillations · Around

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M. Martini, M. Ericson, G. Chanfray, J. Marteau, Phys. Rev. C80
2009
Earlier work this paper cites.

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Later among the works it cites.
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