TY - JOUR
T1 - Measurement of ambient neutrons in an underground laboratory at the Kamioka Observatory
AU - Mizukoshi, Keita
AU - Taishaku, Ryosuke
AU - Hosokawa, Keishi
AU - Kobayashi, Kazuyoshi
AU - Miuchi, Kentaro
AU - Naka, Tatsuhiro
AU - Takeda, Atsushi
AU - Tanaka, Masashi
AU - Wada, Yoshiki
AU - Yorita, Kohei
AU - Yoshida, Sei
N1 - Funding Information:
The authors would like to thank Dr Yuji Kishimoto from KEK for lending us the 3He proportional counter. We also thank Kamioka Mining and Smelting Co., Ltd. for the various support for our research activities in the underground laboratories. We appreciate the useful comments about the rock samples given by Prof. Keiko Suzuki and Dr Koji Kiyosugi from Kobe University. We are grateful to Dr Koichi Ichimura from the Institute for Cosmic Ray Research and Dr Saori Umehara from Osaka University for useful advice on the rock components. We are grateful to Dr Yasuhiro Takemoto from Osaka University for the detector operation. This work was supported by Ministry of Education, Culture, Sports, Science and Technology (MEXT) KAKENHI Grants-in-Aid for Scientific Research on Innovative Areas 26104001, 26104003, 26104004, 26104005, a JSPS KAKENHI Grant-in-Aid for Scientific Research (S) 24224007, and Japan Society for the Promotion of Science (JSPS) KAKENHI Grants-in-Aid for Scientific Research (A)16H02189, (A)17H01661. This work was partially supported by the joint research program of the Institute for Cosmic Ray Research (ICRR), the University of Tokyo.
Publisher Copyright:
© The Author(s) 2018. Published by Oxford University Press on behalf of the Physical Society of Japan.
PY - 2018/12/1
Y1 - 2018/12/1
N2 - Ambient neutrons are one of the most serious backgrounds for underground experiments searching for rare events. The ambient neutron flux in an underground laboratory at the Kamioka Observatory was measured using a 3He proportional counter with various moderator setups. Since the detector response largely depends on the spectral shape, the energy spectra of the neutrons transported from the rock to the laboratory were estimated by Monte Carlo simulations. The ratio of the thermal neutron flux to the total neutron flux was found to depend on the ther-malizing efficiency of the rock. Therefore, the ratio of the count rate without a moderator to that with a moderator was used to determine this parameter. Consequently, the most likely neutron spectrum predicted by the simulations for the parameters determined by the experimental results was obtained. The result suggests an interesting spectral shape, which has not been indicated in previous studies. The total ambient neutron flux is (23.5 ± 0.7stat.+−1.92.1 sys.) × 10−6 cm−2 s−1. This result, especially the energy spectrum information, could be a new and important input for estimating the background in current and future experiments in the underground laboratory at the Kamioka Observatory.
AB - Ambient neutrons are one of the most serious backgrounds for underground experiments searching for rare events. The ambient neutron flux in an underground laboratory at the Kamioka Observatory was measured using a 3He proportional counter with various moderator setups. Since the detector response largely depends on the spectral shape, the energy spectra of the neutrons transported from the rock to the laboratory were estimated by Monte Carlo simulations. The ratio of the thermal neutron flux to the total neutron flux was found to depend on the ther-malizing efficiency of the rock. Therefore, the ratio of the count rate without a moderator to that with a moderator was used to determine this parameter. Consequently, the most likely neutron spectrum predicted by the simulations for the parameters determined by the experimental results was obtained. The result suggests an interesting spectral shape, which has not been indicated in previous studies. The total ambient neutron flux is (23.5 ± 0.7stat.+−1.92.1 sys.) × 10−6 cm−2 s−1. This result, especially the energy spectrum information, could be a new and important input for estimating the background in current and future experiments in the underground laboratory at the Kamioka Observatory.
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U2 - 10.1093/ptep/pty133
DO - 10.1093/ptep/pty133
M3 - Article
AN - SCOPUS:85063219725
SN - 2050-3911
VL - 2018
JO - Progress of Theoretical and Experimental Physics
JF - Progress of Theoretical and Experimental Physics
IS - 12
M1 - 123C01
ER -