2019年11月3日
Measurement of ambient neutrons in an underground laboratory at Kamioka Observatory and future plan
- ,
- ,
- ,
- ,
- ,
- ,
- ,
- ,
- ,
- 巻
- 1468
- 号
- 記述言語
- 英語
- 掲載種別
- 機関テクニカルレポート,技術報告書,プレプリント等
- DOI
- 10.1088/1742-6596/1468/1/012247
Ambient neutrons are one of the most serious backgrounds for underground<br />
experiments in search of rare events. The ambient neutron flux in an<br />
underground laboratory of Kamioka Observatory was measured using a<br />
$\mathrm{^3He}$ proportional counter with various moderator setups. Since the<br />
detector response largely depends on the spectral shape, the energy spectra of<br />
the neutrons transported from the rock to the laboratory were estimated by<br />
Monte-Carlo simulations. The ratio of the thermal neutron flux to the total<br />
neutron flux was found to depend on the thermalizing efficiency of the rock.<br />
Thus, the ratio of the count rate without a moderator to that with a moderator<br />
was used to determine this parameter. Consequently, the most-likely neutron<br />
spectrum predicted by the simulations for the parameters determined by the<br />
experimental results was obtained. The result suggests an interesting spectral<br />
shape, which has not been indicated in previous studies. The total ambient<br />
neutron flux is $(23.5 \pm 0.7 \ \mathrm{_{stat. } } ^{+1.9}_{-2.1} \<br />
\mathrm{_{sys. } }) \times 10^{-6}$ cm$^{-2}$ s$^{-1}$. In this paper, we explain<br />
our method of the result and discuss our future plan.
experiments in search of rare events. The ambient neutron flux in an<br />
underground laboratory of Kamioka Observatory was measured using a<br />
$\mathrm{^3He}$ proportional counter with various moderator setups. Since the<br />
detector response largely depends on the spectral shape, the energy spectra of<br />
the neutrons transported from the rock to the laboratory were estimated by<br />
Monte-Carlo simulations. The ratio of the thermal neutron flux to the total<br />
neutron flux was found to depend on the thermalizing efficiency of the rock.<br />
Thus, the ratio of the count rate without a moderator to that with a moderator<br />
was used to determine this parameter. Consequently, the most-likely neutron<br />
spectrum predicted by the simulations for the parameters determined by the<br />
experimental results was obtained. The result suggests an interesting spectral<br />
shape, which has not been indicated in previous studies. The total ambient<br />
neutron flux is $(23.5 \pm 0.7 \ \mathrm{_{stat. } } ^{+1.9}_{-2.1} \<br />
\mathrm{_{sys. } }) \times 10^{-6}$ cm$^{-2}$ s$^{-1}$. In this paper, we explain<br />
our method of the result and discuss our future plan.
- リンク情報
-
- DOI
- https://doi.org/10.1088/1742-6596/1468/1/012247
- arXiv
- http://arxiv.org/abs/arXiv:1911.00729
- Web of Science
- https://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=JSTA_CEL&SrcApp=J_Gate_JST&DestLinkType=FullRecord&KeyUT=WOS:000539995300245&DestApp=WOS_CPL
- URL
- http://arxiv.org/abs/1911.00729v1
- ID情報
-
- DOI : 10.1088/1742-6596/1468/1/012247
- ISSN : 1742-6588
- eISSN : 1742-6596
- arXiv ID : arXiv:1911.00729
- Web of Science ID : WOS:000539995300245