TY - JOUR
T1 - Stochastic modeling of 3-D compositional distribution in the crust with Bayesian inference and application to geoneutrino observation in Japan
AU - Takeuchi, N.
AU - Ueki, K.
AU - Iizuka, T.
AU - Nagao, J.
AU - Tanaka, A.
AU - Enomoto, S.
AU - Shirahata, Y.
AU - Watanabe, H.
AU - Yamano, M.
AU - Tanaka, H. K.M.
N1 - Funding Information:
We thank W. F. McDonough, F. Mantovani and J. Detwiler for discussions and comments and K. Ozawa for providing some of the xenolith samples analyzed in this study. This work was supported by JSPS KAKENHI Grant Number 15H05833. The tomography model used in this study is available on the web page of NIED JAPAN. All the other input and output data of this study are explicitly presented in the tables or Supplementary information .
Publisher Copyright:
© 2019
PY - 2019/3
Y1 - 2019/3
N2 - Geoneutrino observations, first achieved by KamLAND in 2005 and followed by Borexino in 2010, have accumulated statistics and improved sensitivity for more than ten years. The uncertainty of the geoneutrino flux at the surface is now reduced to a level small enough to set useful constraints on U and Th abundances in the Bulk Silicate Earth (BSE). However, in order to make inferences on earth's compositional model, the contributions from the local crust need to be understood within a similar uncertainty. Here we develop a new method to construct a stochastic crustal composition model utilizing Bayesian inference. While the methodology has general applicability, it incorporates all the local uniqueness in its probabilistic framework. Unlike common approaches for this type of problem, our method does not depend on crustal segmentation into upper, (middle) and lower, whose classification and boundaries are not always well defined. We also develop a new modeling method to infer rock composition distributions that conserve mass balance and therefore do not bias the results. Combined with a new vast collection of geochemical data for rock samples in the Japan arc, we apply this method to geoneutrino observation at Kamioka, Japan. Currently a difficulty remains in the handling of correlations in the flux integration; we conservatively assume maximum correlation, which leads to large flux estimation errors of 60–70%. Despite the large errors, this is the first local crustal model for geoneutrino flux prediction with probabilistic error estimation in a reproducible way.
AB - Geoneutrino observations, first achieved by KamLAND in 2005 and followed by Borexino in 2010, have accumulated statistics and improved sensitivity for more than ten years. The uncertainty of the geoneutrino flux at the surface is now reduced to a level small enough to set useful constraints on U and Th abundances in the Bulk Silicate Earth (BSE). However, in order to make inferences on earth's compositional model, the contributions from the local crust need to be understood within a similar uncertainty. Here we develop a new method to construct a stochastic crustal composition model utilizing Bayesian inference. While the methodology has general applicability, it incorporates all the local uniqueness in its probabilistic framework. Unlike common approaches for this type of problem, our method does not depend on crustal segmentation into upper, (middle) and lower, whose classification and boundaries are not always well defined. We also develop a new modeling method to infer rock composition distributions that conserve mass balance and therefore do not bias the results. Combined with a new vast collection of geochemical data for rock samples in the Japan arc, we apply this method to geoneutrino observation at Kamioka, Japan. Currently a difficulty remains in the handling of correlations in the flux integration; we conservatively assume maximum correlation, which leads to large flux estimation errors of 60–70%. Despite the large errors, this is the first local crustal model for geoneutrino flux prediction with probabilistic error estimation in a reproducible way.
KW - Bayesian
KW - Crustal lithology
KW - Crustal structure
KW - Geoneutrinos
KW - Heat-producing elements
KW - Rock composition
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U2 - 10.1016/j.pepi.2019.01.002
DO - 10.1016/j.pepi.2019.01.002
M3 - Article
AN - SCOPUS:85062608116
SN - 0031-9201
VL - 288
SP - 37
EP - 57
JO - Physics of the Earth and Planetary Interiors
JF - Physics of the Earth and Planetary Interiors
ER -