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    Average prompt fission neutron multiplicities measured in the U235(n,f) reaction induced by neutrons of energy from 1 to 700 MeV

    B. Mauss1,2,*, J. Taïeb1,2, B. Laurent1,2, G. Bélier1,2, A. Chatillon1,2, D. Étasse3, P. Morfouace1,2, O. Roig1,2, M. Devlin4 et al.

    R. C. Haight4 and K. J. Kelly4

    • *Contact author: benoit.mauss@cea.fr

    Phys. Rev. C 113, 064603 – Published 5 June, 2026

    DOI: https://doi.org/10.1103/q6cp-hyb8

    Abstract

    Background: The development of GenIV nuclear reactors will take advantage of fast neutrons. They will necessitate nuclear data of low uncertainties over a wide range of neutron energies, notably above 1 MeV. As far as U235 is concerned, current experimental data on average prompt neutron multiplicities (ν¯prompt) of qualified uncertainties show some discrepancies and do not always cover the full incoming neutron energy range of interest.

    Purpose: Measure the average prompt neutron multiplicity in the U235(n,f) reaction as a function of incoming neutron energy between 1 and 700 MeV.

    Methods: The double time-of-flight technique was used at the Los Alamos Neutron Science Center to measure incoming and prompt fission neutron energies. The data were measured relative to the very well-known Cf252(sf) prompt fission neutron spectrum (PFNS) and ν¯promptCf. The integral over the reconstructed PFNS energy and angle distributions in the U235(n,f) reaction provided ν¯prompt.

    Results: ν¯prompt was obtained between 1 and 700 MeV with uncertainties below 0.5% above neutron incoming energies of 3 MeV. There are discrepancies between the data and the evaluations JEFF 4.0, ENDF/B-VIII.1, and JENDL-5.

    Conclusions: The results are the most precise measurements of ν¯prompt in the U235(n,f) reaction so far and cover well the region of interest for nuclear applications between 1 and 25 MeV. In addition, the data are precise enough to highlight the impact of second-chance fission on the increase rate of ν¯prompt as a function of the incoming neutron energy.

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