Antineutrino emission and gamma background characteristics from a thermal research reactor
V.M. Bui, L. Giot, M. Fallot, V. Communeau, S. Cormon, M. Estienne,, M.Lenoir, N. Peuvrel, T. Shiba, A. S. Cucoanes, M. Elnimr, J. Martino, A., Onillon, A. Porta, G. Pronost, A. Remoto, N. Thiolliere, F. Yermia, A.-A., Zakari-Issoufou

TL;DR
This paper models antineutrino emission and gamma background from the OSIRIS research reactor using detailed core simulations, providing essential data for neutrino experiments and background mitigation.
Contribution
It introduces a comprehensive calculation of antineutrino flux and gamma spectra from a research reactor using the summation method coupled with a complete core model, including off-equilibrium corrections.
Findings
Calculated antineutrino flux for OSIRIS reactor
Provided gamma energy spectrum at core level
Simulated gamma and neutron propagation through shielding
Abstract
The detailed understanding of the antineutrino emission from research reactors is mandatory for any high sensitivity experiments either for fundamental or applied neutrino physics, as well as a good control of the gamma and neutron backgrounds induced by the reactor operation. In this article, the antineutrino emission associated to a thermal research reactor: the OSIRIS reactor located in Saclay, France, is computed in a first part. The calculation is performed with the summation method, which sums all the contributions of the beta decay branches of the fission products, coupled for the first time with a complete core model of the OSIRIS reactor core. The MCNP Utility for Reactor Evolution code was used, allowing to take into account the contributions of all beta decayers in-core. This calculation is representative of the isotopic contributions to the antineutrino flux which can be…
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Taxonomy
TopicsNeutrino Physics Research · Scientific Research and Discoveries · Dark Matter and Cosmic Phenomena
