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Cosmogenic neutron production at the Sudbury Neutrino Observatory

Urheber*innen

Aharmim,  B.
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Ahmed,  S. N.
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Anthony,  A. E.
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Barros,  N.
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Beier,  E. W.
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Bellerive,  A.
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Beltran,  B.
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Bergevin,  M.
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Biller,  S. D.
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Bonventre,  R.
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Boudjemline,  K.
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Boulay,  M. G.
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Cai,  B.
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Callaghan,  E. J.
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Caravaca,  J.
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Chan,  Y. D.
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Chauhan,  D.
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Chen,  M.
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Cleveland,  B. T.
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Cox,  G. A.
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Curley,  R.
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Dai,  X.
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Deng,  H.
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Descamps,  F. B.
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Detwiler,  J. A.
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Doe,  P. J.
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Doucas,  G.
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Drouin,  P.-L.
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Dunford,  M.
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Elliott,  S. R.
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Evans,  H. C.
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Ewan,  G. T.
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Farine,  J.
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Fergani,  H.
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Fleurot,  F.
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Ford,  R. J.
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Formaggio,  J. A.
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Gagnon,  N.
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Gilje,  K.
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Goon,  J. TM.
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Graham,  K.
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Guillian,  E.
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Habib,  S.
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Hahn,  R. L.
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Hallin,  A. L.
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Hallman,  E. D.
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Harvey,  P. J.
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Hazama,  R.
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Heintzelman,  W. J.
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Heise,  J.
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Helmer,  R. L.
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Hime,  A.
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Howard,  C.
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Huang,  M.
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Jagam,  P.
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Jamieson,  B.
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Jelley,  N. A.
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Jerkins,  M.
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Kéfélian,  C.
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Keeter,  K. J.
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Klein,  J. R.
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Kormos,  L. L.
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Kos,  M.
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Krüger,  A.
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Kraus,  C.
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Krauss,  C. B.
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Kutter,  T.
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/persons/resource/kyba

Kyba,  C.
1.4 Remote Sensing, 1.0 Geodesy, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

Land,  B. J.
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Lange,  R.
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Law,  J.
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Lawson,  I. T.
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Lesko,  K. T.
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Leslie,  J. R.
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Levine,  I.
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Loach,  J. C.
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MacLellan,  R.
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Majerus,  S.
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Mak,  H. B.
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Maneira,  J.
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Martin,  R. D.
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Mastbaum,  A.
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McCauley,  N.
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McDonald,  A. B.
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McGee,  S. R.
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Miller,  M. L.
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Monreal,  B.
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Monroe,  J.
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Nickel,  B. G.
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Noble,  A. J.
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O’Keeffe,  H. M.
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Oblath,  N. S.
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Okada,  C. E.
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Ollerhead,  R. W.
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Orebi Gann,  G. D.
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Oser,  S. M.
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Ott,  R. A.
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Peeters,  S. J. M.
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Poon,  A. W. P.
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Prior,  G.
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Reitzner,  S. D.
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Rielage,  K.
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Robertson,  B. C.
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Robertson,  R. G. H.
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Schwendener,  M. H.
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Secrest,  J. A.
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Seibert,  S. R.
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Simard,  O.
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Sinclair,  D.
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Skensved,  P.
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Sonley,  T. J.
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Stonehill,  L. C.
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Tešić,  G.
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Tolich,  N.
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Tsui,  T.
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Van Berg,  R.
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VanDevender,  B. A.
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Virtue,  C. J.
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Wall,  B. L.
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Waller,  D.
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Wan Chan Tseung,  H.
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Wark,  D. L.
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Wendland,  J.
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West,  N.
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Wilkerson,  J. F.
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Wilson,  J. R.
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Winchester,  T.
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Wright,  A.
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Yeh,  M.
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Zhang,  F.
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Zuber,  K.
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Externe Ressourcen
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Volltexte (frei zugänglich)

5000424.pdf
(Verlagsversion), 724KB

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Zitation

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.-L., Dunford, M., Elliott, S., Evans, H., Ewan, G., Farine, J., Fergani, H., Fleurot, F., Ford, R., Formaggio, J., Gagnon, N., Gilje, K., Goon, J., Graham, K., Guillian, E., Habib, S., Hahn, R., Hallin, A., Hallman, E., Harvey, P., Hazama, R., Heintzelman, W., Heise, J., Helmer, R., Hime, A., Howard, C., Huang, M., Jagam, P., Jamieson, B., Jelley, N., Jerkins, M., Kéfélian, C., Keeter, K., Klein, J., Kormos, L., Kos, M., Krüger, A., Kraus, C., Krauss, C., Kutter, T., Kyba, C., Land, B., Lange, R., Law, J., Lawson, I., Lesko, K., Leslie, J., Levine, I., Loach, J., MacLellan, R., Majerus, S., Mak, H., Maneira, J., Martin, R., Mastbaum, A., McCauley, N., McDonald, A., McGee, S., Miller, M., Monreal, B., Monroe, J., Nickel, B., Noble, A., O’Keeffe, H., Oblath, N., Okada, C., Ollerhead, R., Orebi Gann, G., Oser, S., Ott, R., Peeters, S., Poon, A., Prior, G., Reitzner, S., Rielage, K., Robertson, B., Robertson, R., Schwendener, M., Secrest, J., Seibert, S., Simard, O., Sinclair, D., Skensved, P., Sonley, T., Stonehill, L., Tešić, G., Tolich, N., Tsui, T., Van Berg, R., VanDevender, B., Virtue, C., Wall, B., Waller, D., Wan Chan Tseung, H., Wark, D., Wendland, J., West, N., Wilkerson, J., Wilson, J., Winchester, T., Wright, A., Yeh, M., Zhang, F., Zuber, K. (2019): Cosmogenic neutron production at the Sudbury Neutrino Observatory. - Physical Review D, 100, 11, 112005.
https://doi.org/10.1103/PhysRevD.100.112005


Zitierlink: https://gfzpublic.gfz-potsdam.de/pubman/item/item_5000424
Zusammenfassung
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)+1.59−1.12(syst) in pure heavy water and 7.30±0.07(stat)+1.40−1.02(syst) in NaCl-loaded heavy water. These results provide unique insights into this potential background source for experiments at SNOLAB.