日本地球惑星科学連合2016年大会

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セッション記号 M (領域外・複数領域) » M-TT 計測技術・研究手法

[M-TT28] 地球化学の最前線:未来の地球化学を展望して

2016年5月22日(日) 09:00 〜 10:30 A04 (アパホテル&リゾート 東京ベイ幕張)

コンビーナ:*小畑 元(東京大学大気海洋研究所海洋化学部門海洋無機化学分野)、角野 浩史(東京大学大学院総合文化研究科広域科学専攻相関基礎科学系)、横山 哲也(東京工業大学大学院理工学研究科地球惑星科学専攻)、平田 岳史(京都大学大学院理学研究科地球惑星科学専攻)、角皆 潤(名古屋大学大学院環境学研究科)、高橋 嘉夫(東京大学大学院理学系研究科地球惑星科学専攻)、橘 省吾(北海道大学大学院理学研究院自然史科学専攻地球惑星システム科学分野)、鈴木 勝彦(国立研究開発法人海洋研究開発機構・海底資源研究開発センター)、下田 玄(産業技術総合研究所地質調査総合センター)、鍵 裕之(東京大学大学院理学系研究科附属地殻化学実験施設)、横山 祐典(東京大学 大気海洋研究所 高解像度環境解析研究センター)、座長:角野 浩史(東京大学大学院総合文化研究科広域科学専攻相関基礎科学系)、横山 哲也小畑 元(東京大学大気海洋研究所海洋化学部門海洋無機化学分野)

09:15 〜 09:30

[MTT28-02] "He Standard of Japan" (HESJ)の3He/4He比校正

*三島 賢二1角野 浩史2山田 崇人3家城 斉3長倉 直樹3音野 瑛俊4 (1.高エ研、2.東大総合文化、3.東大理、4.九大RCAPP)

キーワード:同位体比分析、3He/4He比、質量分析、ビッグバン元素合成、中性子ベータ崩壊

3He/4He ratios in terrestrial samples vary more than three orders of magnitude, because primordial helium with 3He/4He of (1.4–4.6) x 10–4 has been diluted by addition of radiogenic 4He produced by decay of U- and Th-series elements in different degrees depending on 3He/(U+Th) ratio of each reservoir. This feature makes 3He/4He ratio a powerful tracer in geochemistry and cosmochemistry. Though atmospheric helium with 3He/4He ratio of 1.4 x 10–6 is used to calibrate 3He/4He measurement with a noble gas mass spectrometer, relatively low concentration and 3He/4He ratio of the atmospheric helium cause many difficulties to use it as a working standard for daily measurements. Thus noble gas laboratories often use their own working standards prepared from a natural gas sample with high 3He/4He ratio or by mixing of isotopically pure 3He and 4He. "He Standard of Japan" (HESJ) is one of the latter originally prepared by four noble gas laboratories in Japan [1] and now distributed worldwide as an interlaboratory standard [1,2]. However, 3He/4He ratio of HESJ was determined by comparison with that of atmospheric helium, i.e., absolute 3He/4He ratio has not been determined yet and the accuracy of the value still rely on the early determinations of absolute 3He/4He ratio of atmospheric helium [3].
As long as 3He/4He ratio is used to compare relative contributions of primordial and radiogenic in each geochemical reservoir, absolute 3He/4He value of atmospheric helium or HESJ is less important. However, it is a critical issue in some applications of helium isotopes, such as tritium-3He dating and an experimental project to measure the neutron lifetime with total uncertainty of 1 sec (0.1%) using pulsed neutron source at J-PARC [4].
A neutron decays into a proton, an electron, and an anti-neutrino with a lifetime of 880.3 ± 1.1 sec [5]. The lifetime is an important constant in the Big Bang nucleosynthesis (BBN) that controls amounts of primordial elements in our universe. In this experiment, the incident neutron flux is measured by counting 3He(n,p)3H reaction in a time projection chamber detector filled with 3He, 4He and CO2. To determine neutron lifetime with uncertainty less than 0.1%, 3He number density in the detector must be accurately known with even smaller uncertainty. As a part of this experiment, we are developing a gas handling system to control 3He number density with uncertainty of 0.1%. The 3He gas is mixed with research grade He in a vessel with measuring pressures of these gases precisely using a calibrated piezoresistive transducer.
We fabricated control samples of known 3He/4He ratio using the gas handling system and measured the ratio using a sector type single focusing noble gas mass spectrometer with double collector system [6] at Dept. of Basic Sci., the Univ. of Tokyo by referring to HESJ. The results will contribute to determine the absolute 3He/4He value of HESJ, and that of atmospheric helium also [6].
[1] J. Matsuda et al., Geochem. J. 36, 191 (2002).
[2] Y. Sano, T. Tokutake, and N. Takahata, Anal. Sci. 24, 521 (2008).
[3] Y. Sano, B. Marty and P. Burnard, “The Noble Gases as Geochemical Tracers”, Chapter 2. “Noble gases in the atmosphere”, Springer (2013).
[4] Y. Arimoto, et al, Nucl. Inst. Meth. Phys. Res. A 799, 187–196, (2015).
[5] K.A. Olive et al. (Particle Data Group), Chin. Phys. C, 38, 090001 (2014) and 2015 update.
[6] H. Sumino et al., J. Mass Spectrom. Soc. Jpn. 49, 61 (2001).