Neutrino geophysics with KamLAND and future prospects

被引:52
作者
Enomoto, S. [1 ]
Ohtani, E.
Inoue, K.
Suzuki, A.
机构
[1] Tohoku Univ, Grad Sch Sci, Dept Phys, Res Ctr Neutrino Sci, Sendai, Miyagi 9808578, Japan
[2] Tohoku Univ, Grad Sch Sci, Inst Mineral Petrol & Econ Geol, Sendai, Miyagi 9808578, Japan
关键词
geoneutrino; KamLAND; terrestrial heat flux; Uranium and Thorium; bulk silicate Earth; thermal history; VELOCITY STRUCTURE; EARTH; CRUST; MANTLE;
D O I
10.1016/j.epsl.2007.03.038
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The Kamioka liquid scintillator anti-neutrino detector (KamLAND) is a low-energy and low-background neutrino detector which could be a useful probe for determining the U and Th abundances of the Earth. We constructed a model of the Earth in order to evaluate the rate of geologically produced anti-neutrinos (geoneutrinos) detectable by KamLAND. We found that KamLAND can be used to determine the absolute abundances of U and Th in the Earth with accuracy sufficient for placing important constraints on Earth's accretion and succeeding thermal history. Within the uncertainty of the measurement, the present observation of geoneutrinos with KamLAND is consistent with our model prediction based on the bulk silicate Earth (BSE) composition. If a neutrino detector were to be built in Hawaii, where effects of the continental crust would be negligible, it could be used to estimate the U and Th content in the lower mantle and the core. Our calculation of the geoneutrino event rate on the Earth's surface indicates that geoneutrino observation can provide key information for testing the current models of the U and Th content and distribution in the Earth. (C) 2007 Elsevier B.V All rights reserved.
引用
收藏
页码:147 / 159
页数:13
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