Cosmogenic neutron production at Daya Bay

11Citations
Citations of this article
26Readers
Mendeley users who have this article in their library.

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)×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.

Cite

CITATION STYLE

APA

An, F. P., Balantekin, A. B., Band, H. R., Bishai, M., Blyth, S., Cao, D., … Zou, J. H. (2018). Cosmogenic neutron production at Daya Bay. Physical Review D, 97(5). https://doi.org/10.1103/PhysRevD.97.052009

Register to see more suggestions

Mendeley helps you to discover research relevant for your work.

Already have an account?

Save time finding and organizing research with Mendeley

Sign up for free