Yields and production rates of cosmogenic [superscript 9]Li and [superscript 8]He measured with the Double Chooz near and far detectors

The yields and production rates of the radioisotopes [superscript 9]Li and [superscript 8]He created by cosmic muon spallation on [superscript 12]C, have been measured by the two detectors of the Double Chooz experiment. The identical detectors are located at separate sites and depths, which means t...

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Main Authors: de Kerret, H., Abrahão, T., Almazan, H., dos Anjos, J. C, Appel, S., Barriere, J. C, Bekman, I., Bezerra, T. J C, Bezrukov, L., Blucher, E., Brugière, T., Buck, C., Busenitz, J., Cabrera, A., Cerrada, M., Chauveau, E., Chimenti, P., Corpace, O., Dawson, J. V, Djurcic, Z., Etenko, A., Franco, D., Furuta, H., Gil-Botella, I., Givaudan, A., Gomez, H., Gonzalez, L. F G, Goodman, M. C, Hara, T., Haser, J., Hellwig, D., Ishitsuka, M., Jochum, J., Jollet, C., Kale, K., Kaneda, M., Karakac, M., Kawasaki, T., Kemp, E., Kryn, D., Kuze, M., Lachenmaier, T., Lane, C. E, Lasserre, T., Lastoria, C., Lhuillier, D., Lima, H. P, Lindner, M., López-Castaño, J. M, LoSecco, J. M, Lubsandorzhiev, B., Maeda, J., Mariani, C., Maricic, J., Martino, J., Matsubara, T., Mention, G., Meregaglia, A., Miletic, T., Milincic, R., Navas-Nicolás, D., Novella, P., Nunokawa, H., Oberauer, L., Obolensky, M., Onillon, A., Oralbaev, A., Palomares, C., Pepe, I. M, Pronost, G., Reichenbacher, J., Reinhold, B., Settimo, M., Schönert, S., Schoppmann, S., Scola, L., Sharankova, R., Sibille, V., Sinev, V., Skorokhvatov, M., Soldin, P., Stahl, A., Stancu, I., Stokes, L. F F, Suekane, F., Sukhotin, S., Sumiyoshi, T., Sun, Y., Tonazzo, A., Veyssiere, C., Viaud, B., Vivier, M., Wagner, S., Wiebusch, C., Wurm, M., Yang, G., Yermia, F., Hourlier, Adrien C.
Other Authors: Massachusetts Institute of Technology. Laboratory for Nuclear Science
Format: Article
Language:English
Published: Springer Berlin Heidelberg 2018
Online Access:http://hdl.handle.net/1721.1/119501
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author de Kerret, H.
Abrahão, T.
Almazan, H.
dos Anjos, J. C
Appel, S.
Barriere, J. C
Bekman, I.
Bezerra, T. J C
Bezrukov, L.
Blucher, E.
Brugière, T.
Buck, C.
Busenitz, J.
Cabrera, A.
Cerrada, M.
Chauveau, E.
Chimenti, P.
Corpace, O.
Dawson, J. V
Djurcic, Z.
Etenko, A.
Franco, D.
Furuta, H.
Gil-Botella, I.
Givaudan, A.
Gomez, H.
Gonzalez, L. F G
Goodman, M. C
Hara, T.
Haser, J.
Hellwig, D.
Ishitsuka, M.
Jochum, J.
Jollet, C.
Kale, K.
Kaneda, M.
Karakac, M.
Kawasaki, T.
Kemp, E.
Kryn, D.
Kuze, M.
Lachenmaier, T.
Lane, C. E
Lasserre, T.
Lastoria, C.
Lhuillier, D.
Lima, H. P
Lindner, M.
López-Castaño, J. M
LoSecco, J. M
Lubsandorzhiev, B.
Maeda, J.
Mariani, C.
Maricic, J.
Martino, J.
Matsubara, T.
Mention, G.
Meregaglia, A.
Miletic, T.
Milincic, R.
Navas-Nicolás, D.
Novella, P.
Nunokawa, H.
Oberauer, L.
Obolensky, M.
Onillon, A.
Oralbaev, A.
Palomares, C.
Pepe, I. M
Pronost, G.
Reichenbacher, J.
Reinhold, B.
Settimo, M.
Schönert, S.
Schoppmann, S.
Scola, L.
Sharankova, R.
Sibille, V.
Sinev, V.
Skorokhvatov, M.
Soldin, P.
Stahl, A.
Stancu, I.
Stokes, L. F F
Suekane, F.
Sukhotin, S.
Sumiyoshi, T.
Sun, Y.
Tonazzo, A.
Veyssiere, C.
Viaud, B.
Vivier, M.
Wagner, S.
Wiebusch, C.
Wurm, M.
Yang, G.
Yermia, F.
Hourlier, Adrien C.
author2 Massachusetts Institute of Technology. Laboratory for Nuclear Science
author_facet Massachusetts Institute of Technology. Laboratory for Nuclear Science
de Kerret, H.
Abrahão, T.
Almazan, H.
dos Anjos, J. C
Appel, S.
Barriere, J. C
Bekman, I.
Bezerra, T. J C
Bezrukov, L.
Blucher, E.
Brugière, T.
Buck, C.
Busenitz, J.
Cabrera, A.
Cerrada, M.
Chauveau, E.
Chimenti, P.
Corpace, O.
Dawson, J. V
Djurcic, Z.
Etenko, A.
Franco, D.
Furuta, H.
Gil-Botella, I.
Givaudan, A.
Gomez, H.
Gonzalez, L. F G
Goodman, M. C
Hara, T.
Haser, J.
Hellwig, D.
Ishitsuka, M.
Jochum, J.
Jollet, C.
Kale, K.
Kaneda, M.
Karakac, M.
Kawasaki, T.
Kemp, E.
Kryn, D.
Kuze, M.
Lachenmaier, T.
Lane, C. E
Lasserre, T.
Lastoria, C.
Lhuillier, D.
Lima, H. P
Lindner, M.
López-Castaño, J. M
LoSecco, J. M
Lubsandorzhiev, B.
Maeda, J.
Mariani, C.
Maricic, J.
Martino, J.
Matsubara, T.
Mention, G.
Meregaglia, A.
Miletic, T.
Milincic, R.
Navas-Nicolás, D.
Novella, P.
Nunokawa, H.
Oberauer, L.
Obolensky, M.
Onillon, A.
Oralbaev, A.
Palomares, C.
Pepe, I. M
Pronost, G.
Reichenbacher, J.
Reinhold, B.
Settimo, M.
Schönert, S.
Schoppmann, S.
Scola, L.
Sharankova, R.
Sibille, V.
Sinev, V.
Skorokhvatov, M.
Soldin, P.
Stahl, A.
Stancu, I.
Stokes, L. F F
Suekane, F.
Sukhotin, S.
Sumiyoshi, T.
Sun, Y.
Tonazzo, A.
Veyssiere, C.
Viaud, B.
Vivier, M.
Wagner, S.
Wiebusch, C.
Wurm, M.
Yang, G.
Yermia, F.
Hourlier, Adrien C.
author_sort de Kerret, H.
collection MIT
description The yields and production rates of the radioisotopes [superscript 9]Li and [superscript 8]He created by cosmic muon spallation on [superscript 12]C, have been measured by the two detectors of the Double Chooz experiment. The identical detectors are located at separate sites and depths, which means that they are subject to different muon spectra. The near (far) detector has an overburden of ∼120 m.w.e. (∼300 m.w.e.) corresponding to a mean muon energy of 32.1 ± 2.0 GeV (63.7 ± 5.5 GeV). Comparing the data to a detailed simulation of the [superscript 9]Li and [superscript 8]He decays, the contribution of the [superscript 8]He radioisotope at both detectors is found to be compatible with zero. The observed [superscript 9]Li yields in the near and far detectors are 5.51 ± 0.51 and 7.90 ± 0.51, respectively, in units of 10[superscript −8]μ[superscript −1]g[superscript −1]cm[superscript 2]. The shallow overburdens of the near and far detectors give a unique insight when combined with measurements by KamLAND and Borexino to give the first multi-experiment, data driven relationship between the 9Li yield and the mean muon energy according to the power law Y=Y[subscript 0](⟨E[subscript μ]⟩/1 GeV)[superscript ¯ over α], giving [¯over α]=0.72±0.06 and Y0 = (0.43 ± 0.11) × 10[superscript −8]μ[superscript −1]g[superscript −1]cm[superscript 2]. This relationship gives future liquid scintillator based experiments the ability to predict their cosmogenic [superscript 9]Li background rates. Open image in new window Keywords Neutrino Detectors and Telescopes (experiments)
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spelling mit-1721.1/1195012022-09-29T10:54:21Z Yields and production rates of cosmogenic [superscript 9]Li and [superscript 8]He measured with the Double Chooz near and far detectors de Kerret, H. Abrahão, T. Almazan, H. dos Anjos, J. C Appel, S. Barriere, J. C Bekman, I. Bezerra, T. J C Bezrukov, L. Blucher, E. Brugière, T. Buck, C. Busenitz, J. Cabrera, A. Cerrada, M. Chauveau, E. Chimenti, P. Corpace, O. Dawson, J. V Djurcic, Z. Etenko, A. Franco, D. Furuta, H. Gil-Botella, I. Givaudan, A. Gomez, H. Gonzalez, L. F G Goodman, M. C Hara, T. Haser, J. Hellwig, D. Ishitsuka, M. Jochum, J. Jollet, C. Kale, K. Kaneda, M. Karakac, M. Kawasaki, T. Kemp, E. Kryn, D. Kuze, M. Lachenmaier, T. Lane, C. E Lasserre, T. Lastoria, C. Lhuillier, D. Lima, H. P Lindner, M. López-Castaño, J. M LoSecco, J. M Lubsandorzhiev, B. Maeda, J. Mariani, C. Maricic, J. Martino, J. Matsubara, T. Mention, G. Meregaglia, A. Miletic, T. Milincic, R. Navas-Nicolás, D. Novella, P. Nunokawa, H. Oberauer, L. Obolensky, M. Onillon, A. Oralbaev, A. Palomares, C. Pepe, I. M Pronost, G. Reichenbacher, J. Reinhold, B. Settimo, M. Schönert, S. Schoppmann, S. Scola, L. Sharankova, R. Sibille, V. Sinev, V. Skorokhvatov, M. Soldin, P. Stahl, A. Stancu, I. Stokes, L. F F Suekane, F. Sukhotin, S. Sumiyoshi, T. Sun, Y. Tonazzo, A. Veyssiere, C. Viaud, B. Vivier, M. Wagner, S. Wiebusch, C. Wurm, M. Yang, G. Yermia, F. Hourlier, Adrien C. Massachusetts Institute of Technology. Laboratory for Nuclear Science Hourlier, Adrien C. The yields and production rates of the radioisotopes [superscript 9]Li and [superscript 8]He created by cosmic muon spallation on [superscript 12]C, have been measured by the two detectors of the Double Chooz experiment. The identical detectors are located at separate sites and depths, which means that they are subject to different muon spectra. The near (far) detector has an overburden of ∼120 m.w.e. (∼300 m.w.e.) corresponding to a mean muon energy of 32.1 ± 2.0 GeV (63.7 ± 5.5 GeV). Comparing the data to a detailed simulation of the [superscript 9]Li and [superscript 8]He decays, the contribution of the [superscript 8]He radioisotope at both detectors is found to be compatible with zero. The observed [superscript 9]Li yields in the near and far detectors are 5.51 ± 0.51 and 7.90 ± 0.51, respectively, in units of 10[superscript −8]μ[superscript −1]g[superscript −1]cm[superscript 2]. The shallow overburdens of the near and far detectors give a unique insight when combined with measurements by KamLAND and Borexino to give the first multi-experiment, data driven relationship between the 9Li yield and the mean muon energy according to the power law Y=Y[subscript 0](⟨E[subscript μ]⟩/1 GeV)[superscript ¯ over α], giving [¯over α]=0.72±0.06 and Y0 = (0.43 ± 0.11) × 10[superscript −8]μ[superscript −1]g[superscript −1]cm[superscript 2]. This relationship gives future liquid scintillator based experiments the ability to predict their cosmogenic [superscript 9]Li background rates. Open image in new window Keywords Neutrino Detectors and Telescopes (experiments) National Science Foundation (U.S.) United States. Department of Energy 2018-12-11T15:45:13Z 2018-12-11T15:45:13Z 2018-11 2018-07 2018-11-14T06:43:06Z Article http://purl.org/eprint/type/JournalArticle 1029-8479 http://hdl.handle.net/1721.1/119501 The Double Chooz collaboration, et al. “Yields and Production Rates of Cosmogenic [superscript 9]Li and [superscript 8]He Measured with the Double Chooz near and Far Detectors.” Journal of High Energy Physics, vol. 2018, no. 11, Nov. 2018. en https://doi.org/10.1007/JHEP11(2018)053 Journal of High Energy Physics Creative Commons Attribution http://creativecommons.org/licenses/by/4.0/ The Author(s) application/pdf Springer Berlin Heidelberg Springer Berlin Heidelberg
spellingShingle de Kerret, H.
Abrahão, T.
Almazan, H.
dos Anjos, J. C
Appel, S.
Barriere, J. C
Bekman, I.
Bezerra, T. J C
Bezrukov, L.
Blucher, E.
Brugière, T.
Buck, C.
Busenitz, J.
Cabrera, A.
Cerrada, M.
Chauveau, E.
Chimenti, P.
Corpace, O.
Dawson, J. V
Djurcic, Z.
Etenko, A.
Franco, D.
Furuta, H.
Gil-Botella, I.
Givaudan, A.
Gomez, H.
Gonzalez, L. F G
Goodman, M. C
Hara, T.
Haser, J.
Hellwig, D.
Ishitsuka, M.
Jochum, J.
Jollet, C.
Kale, K.
Kaneda, M.
Karakac, M.
Kawasaki, T.
Kemp, E.
Kryn, D.
Kuze, M.
Lachenmaier, T.
Lane, C. E
Lasserre, T.
Lastoria, C.
Lhuillier, D.
Lima, H. P
Lindner, M.
López-Castaño, J. M
LoSecco, J. M
Lubsandorzhiev, B.
Maeda, J.
Mariani, C.
Maricic, J.
Martino, J.
Matsubara, T.
Mention, G.
Meregaglia, A.
Miletic, T.
Milincic, R.
Navas-Nicolás, D.
Novella, P.
Nunokawa, H.
Oberauer, L.
Obolensky, M.
Onillon, A.
Oralbaev, A.
Palomares, C.
Pepe, I. M
Pronost, G.
Reichenbacher, J.
Reinhold, B.
Settimo, M.
Schönert, S.
Schoppmann, S.
Scola, L.
Sharankova, R.
Sibille, V.
Sinev, V.
Skorokhvatov, M.
Soldin, P.
Stahl, A.
Stancu, I.
Stokes, L. F F
Suekane, F.
Sukhotin, S.
Sumiyoshi, T.
Sun, Y.
Tonazzo, A.
Veyssiere, C.
Viaud, B.
Vivier, M.
Wagner, S.
Wiebusch, C.
Wurm, M.
Yang, G.
Yermia, F.
Hourlier, Adrien C.
Yields and production rates of cosmogenic [superscript 9]Li and [superscript 8]He measured with the Double Chooz near and far detectors
title Yields and production rates of cosmogenic [superscript 9]Li and [superscript 8]He measured with the Double Chooz near and far detectors
title_full Yields and production rates of cosmogenic [superscript 9]Li and [superscript 8]He measured with the Double Chooz near and far detectors
title_fullStr Yields and production rates of cosmogenic [superscript 9]Li and [superscript 8]He measured with the Double Chooz near and far detectors
title_full_unstemmed Yields and production rates of cosmogenic [superscript 9]Li and [superscript 8]He measured with the Double Chooz near and far detectors
title_short Yields and production rates of cosmogenic [superscript 9]Li and [superscript 8]He measured with the Double Chooz near and far detectors
title_sort yields and production rates of cosmogenic superscript 9 li and superscript 8 he measured with the double chooz near and far detectors
url http://hdl.handle.net/1721.1/119501
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AT palomaresc yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT pepeim yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT pronostg yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT reichenbacherj yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT reinholdb yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT settimom yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT schonerts yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT schoppmanns yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT scolal yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT sharankovar yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT sibillev yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT sinevv yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT skorokhvatovm yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT soldinp yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT stahla yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT stancui yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT stokeslff yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT suekanef yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT sukhotins yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT sumiyoshit yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT suny yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT tonazzoa yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT veyssierec yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT viaudb yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT vivierm yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT wagners yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT wiebuschc yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT wurmm yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT yangg yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT yermiaf yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors
AT hourlieradrienc yieldsandproductionratesofcosmogenicsuperscript9liandsuperscript8hemeasuredwiththedoublechooznearandfardetectors