Cosmogenic neutron production at Daya Bay

  • (The Daya Bay Collaboration)

研究成果: Article同行評審

13 引文 斯高帕斯(Scopus)

摘要

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)×10-5, (10.22±0.87)×10-5, and (17.03±1.22)×10-5 μ-1 g-1 cm2 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.

原文English
文章編號054019
期刊Physical Review D
97
發行號5
DOIs
出版狀態Published - 1 3月 2018

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