Cosmogenic neutron production at the Sudbury Neutrino Observatory

Authors

B. Aharmim, Laurentian University
S. N. Ahmed, Queen’s University
A. E. Anthony, The University of Texas at Austin
N. Barros, Laboratório de Instrumentacao e Física Experimental de Partículas
E. W. Beier, University of Pennsylvania
A. Bellerive, Carleton University
B. Beltran, University of Alberta
M. Bergevin, University of Guelph
S. D. Biller, University of Oxford
R. Bonventre, University of California, Berkeley
K. Boudjemline, Carleton University
M. G. Boulay, Queen’s University
B. Cai, Queen’s University
E. J. Callaghan, University of California, Berkeley
J. Caravaca, University of California, Berkeley
Y. D. Chan, Lawrence Berkeley National Laboratory
D. Chauhan, Laurentian University
M. Chen, Queen’s University
B. T. Cleveland, University of Oxford
G. A. Cox, University of Washington
R. Curley, University of California, Berkeley
X. Dai, Carleton University
H. Deng, University of Pennsylvania
F. B. Descamps, University of California, Berkeley
J. A. Detwiler, Lawrence Berkeley National Laboratory
P. J. Doe, University of Washington
G. Doucas, University of Oxford
P. L. Drouin, Carleton University

Document Type

Article

Publication Date

12-12-2019

Abstract

Neutrons produced in nuclear interactions initiated by cosmic-ray muons present an irreducible background to many rare-event searches, even in detectors located deep underground. Models for the production of these neutrons have been tested against previous experimental data, but the extrapolation to deeper sites is not well understood. Here we report results from an analysis of cosmogenically produced neutrons at the Sudbury Neutrino Observatory. A specific set of observables are presented, which can be used to benchmark the validity of geant4 physics models. In addition, the cosmogenic neutron yield, in units of 10-4 cm2/(g·μ), is measured to be 7.28±0.09(stat)-1.12+1.59(syst) in pure heavy water and 7.30±0.07(stat)-1.02+1.40(syst) in NaCl-loaded heavy water. These results provide unique insights into this potential background source for experiments at SNOLAB.

Publication Source (Journal or Book title)

Physical Review D

Recommended Citation

Aharmim, B., Ahmed, S., Anthony, A., Barros, N., Beier, E., Bellerive, A., Beltran, B., Bergevin, M., Biller, S., Bonventre, R., Boudjemline, K., Boulay, M., Cai, B., Callaghan, E., Caravaca, J., Chan, Y., Chauhan, D., Chen, M., Cleveland, B., Cox, G., Curley, R., Dai, X., Deng, H., Descamps, F., Detwiler, J., Doe, P., Doucas, G., & Drouin, P. (2019). Cosmogenic neutron production at the Sudbury Neutrino Observatory. Physical Review D, 100 (11) https://doi.org/10.1103/PhysRevD.100.112005