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Record W2766137297 · doi:10.1103/physrevd.97.052009

Cosmogenic neutron production at Daya Bay

2018· article· en· W2766137297 on OpenAlexaff
Fengpeng An, A. B. Balantekin, H. R. Band, M. Bishai, S. Blyth, D. Cao, G. F. Cao, Jun Cao, Y. L. Chan, J. F. Chang, Y. Chang, H. S. Chen, S. M. Chen, Ye-Fei Chen, Y. X. Chen, Jie Cheng, Zhaokan Cheng, J. J. Cherwinka, M. C. Chu, A. Chukanov, J. P. Cummings, Yayun Ding, M. Diwan, M. Dolgareva, J. Dove, D. A. Dwyer, W. R. Edwards, R. Gill, M. Gonchar, G. Gong, Haipeng Gong, M. Grassi, W. Gu, Lei Guo, Xin-Heng Guo, Yuhang Guo, Ziwei Guo, R. Hackenburg, S. Hans, M. He, K. M. Heeger, Y. K. Heng, A. Higuera, Y. Hsiung, Beibei Hu, T. Hu, Han‐Xiong Huang, X. T. Huang, Y. B. Huang, Patrick Huber, W. Huo, Ghulam Hussain, D. E. Jaffe, K. L. Jen, X. L. Ji, X. Ji, J. B. Jiao, R. A. Johnson, D. Jones, Li-Wei Kang, S. H. Kettell, Amir N. Khan, L. W. Koerner, S. Kohn, M. Krämer, M. W. Kwok, T. J. Langford, K. Lau, L. Lebanowski, J. Lee, J. H. C. Lee, R. T. Lei, R. Leitner, J. K. C. Leung, C. Li, D. J. Li, F. Li, G. S. Li, Q. J. Li, S. Li, S. C. Li, W. D. Li, X. N. Li, Xuejing Li, Yufeng Li, Ziwei Li, H. Liang, C.-J. Lin, Guey-Lin Lin, Y. C. Lin, J. J. Ling, J. M. Link, L. Littenberg, B. R. Littlejohn, J. C. Liu, J. L. Liu, T. Lohse, C. Lu, H. Q. Lu, J. S. Lu, X.-G. Lu, X. B., X. Y., Y. Q., Yury Malyshkin, D. A. Martínez Caicedo, Kirk T. McDonald, R. D. McKeown, I. V. Mitchell, Y. Nakajima, J. Napolitano, D. Naumov, E. Naumova, J. P. Ochoa‐Ricoux, A. Olshevskiy, H.-R. Pan, J. Park, S. Patton, V. Pec, J. C. Peng, L. Pinsky, C. S. J. Pun, F. Z. Qi, M. Qi, X. Qian, Rui Qiu, N. Raper, Jie Ren, R. Rosero, B. Roskovec, Xichao Ruan, H. Steiner, Jian Sun, W. Tang, D. Taychenachev, Konstantin Treskov, K. V. Tsang, W.-H. Tse, C. E. Tull, N. Viaux Maira, B. Viren, V. Vorobel, C. H. Wang, Meng Wang, N. Y. Wang, R. G. Wang, W. Wang, X. Wang, Y. F. Wang, Zhimin Wang, Z. M. Wang, H. Wei, Liangjian Wen, K. Whisnant, C. White, T. Wise, H. L. H. Wong, S. C. F. Wong, E. Worcester, Chengxin Wu, Q. Wu, W. Wu, D. M. Xia, J. K. Xia, Z. Z. Xing, Jilei Xu, Y. Xu, T. Xue, C.G. Yang, H. Yang, L. Yang, M. Yang, M. Yang, Yifan Yang, M. Ye, Ziping Ye, M. Yeh, Ben Young, Zeyuan Yu, S. Zeng, Liang Zhan, C. Zhang, C. C. Zhang, H. H. Zhang, J. W. Zhang, Qingmin Zhang, R. Zhang, X. T. Zhang, Y. M. Zhang, Y. X. Zhang, Z. J. Zhang, Z. P. Zhang, Z. Y. Zhang, J. Zhao, Li Zhou, H.L. Zhuang, J. H. Zou

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2018
Typearticle
Languageen
FieldPhysics and Astronomy
TopicNeutrino Physics Research
Canadian institutionsInstitute of Particle Physics
FundersComisión Nacional de Investigación Científica y TecnológicaJoint Institute for Nuclear ResearchNatural Science Foundation of Guangdong ProvinceMinistry of Science and Technology of the People's Republic of ChinaResearch Grants Council, University Grants CommitteeMinisterstvo Školství, Mládeže a TělovýchovyChinese Academy of SciencesNational Natural Science Foundation of ChinaChina RailwayRussian Foundation for Basic ResearchCAS Center for Excellence in Particle PhysicsMinistry of EducationU.S. Department of EnergyNational Science Foundation
KeywordsNuclear physicsNeutronPhysicsMuonYield (engineering)ScintillatorNeutrinoCosmic rayDetector

Abstract

fetched live from OpenAlex

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 ${Y}_{n}=(10.26\ifmmode\pm\else\textpm\fi{}0.86)\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}5}$, $(10.22\ifmmode\pm\else\textpm\fi{}0.87)\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}5}$, and $(17.03\ifmmode\pm\else\textpm\fi{}1.22)\ifmmode\times\else\texttimes\fi{}{10}^{\ensuremath{-}5}\text{ }\text{ }{\ensuremath{\mu}}^{\ensuremath{-}1}\text{ }{\mathrm{g}}^{\ensuremath{-}1}\text{ }{\mathrm{cm}}^{2}$ 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 $0.77\ifmmode\pm\else\textpm\fi{}0.03$ for the dependence of the neutron yield on muon energy.

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame distilled prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. Learned from the 10,348 direct Codex labels and 10,348 direct Gemma labels. Candidate is the union of thresholded teacher heads; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels or direct frontier model labels.

metaresearch head score (Codex)0.001
metaresearch head score (Gemma)0.000
Version: codex-gemma-dda1882f352aValidation status: machine_predicted_unvalidated
Candidate categoriesMeta-epidemiology (narrow), Insufficient payload (model declined to judge)
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Bench or experimental · Consensus signal: none
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.342
Threshold uncertainty score0.999

Codex and Gemma teacher scores by category

CategoryCodexGemma
Metaresearch0.0010.000
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0020.001
Bibliometrics0.0000.002
Science and technology studies0.0010.001
Scholarly communication0.0000.001
Open science0.0010.001
Research integrity0.0000.001
Insufficient payload (model declined to judge)0.0010.012

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.025
GPT teacher head0.449
Teacher spread0.424 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one teacher head, not a consensus.

Study designBench or experimental
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations19
Published2018
Admission routes1
Has abstractyes

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