TY - JOUR
T1 - Measurement of ambient neutrons in an underground laboratory at Kamioka Observatory and future plan
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 thank Dr. Yuji Kishimoto of KEK for lending us the 3He proportional counter. We also thank Kamioka Mining and Smelting Co., Ltd. for various supports given to our research activities in the underground laboratories. This work was supported by the MEXT KAKENHI Grant-in-Aid for Scientific Research on Innovative Areas 26104001, 26104003, 26104004, 26104005, JSPS KAKENHI Grant-in-Aid for Scientific Research (S) 24224007, JSPS KAKENHI Grant-in-Aid for Scientific Research (A)16H02189, (A)17H01661, and Grant-in-Aid for JSPS Fellows 19J20418. This work was partially supported by the joint research program of the Institute for Cosmic Ray Research (ICRR), the University of Tokyo.
Publisher Copyright:
© 2020 Published under licence by IOP Publishing Ltd.
PY - 2020/3/20
Y1 - 2020/3/20
N2 - Ambient neutrons are one of the most serious backgrounds for underground experiments in search of rare events. The ambient neutron flux in an underground laboratory of 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 thermalizing efficiency of the rock. Thus, 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 [1]. In this paper, we explain our method of the result and discuss our future plan.
AB - Ambient neutrons are one of the most serious backgrounds for underground experiments in search of rare events. The ambient neutron flux in an underground laboratory of 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 thermalizing efficiency of the rock. Thus, 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 [1]. In this paper, we explain our method of the result and discuss our future plan.
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U2 - 10.1088/1742-6596/1468/1/012247
DO - 10.1088/1742-6596/1468/1/012247
M3 - Conference article
AN - SCOPUS:85083117358
SN - 1742-6588
VL - 1468
JO - Journal of Physics: Conference Series
JF - Journal of Physics: Conference Series
IS - 1
M1 - 012247
T2 - 16th International Conference on Topics in Astroparticle and Underground Physics, TAUP 2019
Y2 - 9 September 2019 through 13 September 2019
ER -