• Open Access

Cosmogenic neutron production at Daya Bay

F. P. An et al. (The Daya Bay Collaboration)
Phys. Rev. D 97, 052009 – Published 26 March 2018

Abstract

Neutrons produced by cosmic ray muons are an important background for underground experiments studying neutrino oscillations, neutrinoless double beta decay, dark matter, and other rare-event signals. A measurement of the neutron yield in the three different experimental halls of the Daya Bay Reactor Neutrino Experiment at varying depth is reported. The neutron yield in Daya Bay’s liquid scintillator is measured to be Yn=(10.26±0.86)×105, (10.22±0.87)×105, and (17.03±1.22)×105μ1g1cm2 at depths of 250, 265, and 860 meters-water-equivalent. These results are compared to other measurements and the simulated neutron yield in Fluka and Geant4. A global fit including the Daya Bay measurements yields a power law coefficient of 0.77±0.03 for the dependence of the neutron yield on muon energy.

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  • Received 3 November 2017

DOI:https://doi.org/10.1103/PhysRevD.97.052009

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsNuclear Physics

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Vol. 97, Iss. 5 — 1 March 2018

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