TY - JOUR
T1 - Thermodynamic modeling of hydrous-melt–olivine equilibrium using exhaustive variable selection
AU - Ueki, Kenta
AU - Kuwatani, Tatsu
AU - Okamoto, Atsushi
AU - Akaho, Shotaro
AU - Iwamori, Hikaru
N1 - Funding Information:
We thank Keith Putirka for a constructive and detailed review, and Kei Hirose for careful editorial handling of the manuscript. Maurizio Petrelli and an anonymous reviewer are thanked for useful and detailed comments on an earlier version of the manuscript. We thank Taku Tsuchiya, Ryuichi Nomura, and Atsushi Yasumoto for insightful discussions. We gratefully acknowledge grants from The Joint Usage/Research Center programs of the Earthquake Research Institute, University of Tokyo, Japan, 2015-B-04 (Geochemical Data Analysis Using Machine Learning) and 2018-B-01 (Data-driven Geoscience: Application to Dynamics in Mobile Belts). K.U. was supported by Japan Society for the Promotion of Science KAKENHI Grant Numbers JP15H05833, JP17H02063, and JP19K04026, and T.K. was supported by Japan Society for the Promotion of Science KAKENHI Grant numbers JP15K20864 and JP25120005 and by Japan Science and Technology Agency PRESTO Grant Number JPMJPR1676. S.A. and T.K. were supported by Japan Science and Technology Agency CREST Grant No. JPMJCR1761. Some of the experimental data used for the model-selection and parameter optimization were obtained from the Library of Experimental Phase Relations open database of melting experiments (Hirschmann et al. 2008). The R source code and dataset used in this study are provided in Supplementary materials 1 and 2 respectively. We thank Keith Putirka for a constructive and detailed review, and Kei Hirose for careful editorial handling of the manuscript. Maurizio Petrelli and an anonymous reviewer are thanked for useful and detailed comments on an earlier version of the manuscript. We thank Taku Tsuchiya, Ryuichi Nomura, and Atsushi Yasumoto for insightful discussions. We gratefully acknowledge grants from The Joint Usage/Research Center programs of the Earthquake Research Institute, University of Tokyo, Japan, 2015-B-04 (Geochemical Data Analysis Using Machine Learning) and 2018-B-01 (Data-driven Geoscience: Application to Dynamics in Mobile Belts). K.U. was supported by Japan Society for the Promotion of Science KAKENHI Grant Numbers JP15H05833, JP17H02063, and JP19K04026, and T.K. was supported by Japan Society for the Promotion of Science KAKENHI Grant numbers JP15K20864 and JP25120005 and by Japan Science and Technology Agency PRESTO Grant Number JPMJPR1676. S.A. and T.K. were supported by Japan Science and Technology Agency CREST Grant No. JPMJCR1761. Some of the experimental data used for the model-selection and parameter optimization were obtained from the Library of Experimental Phase Relations open database of melting experiments (Hirschmann et al. 2008). The R source code and dataset used in this study are provided in Supplementary materials 1 and 2 respectively.
Funding Information:
We thank Keith Putirka for a constructive and detailed review, and Kei Hirose for careful editorial handling of the manuscript. Maurizio Petrelli and an anonymous reviewer are thanked for useful and detailed comments on an earlier version of the manuscript. We thank Taku Tsuchiya, Ryuichi Nomura, and Atsushi Yasumoto for insightful discussions. We gratefully acknowledge grants from The Joint Usage/Research Center programs of the Earthquake Research Institute, University of Tokyo , Japan, 2015-B-04 (Geochemical Data Analysis Using Machine Learning) and 2018-B-01 (Data-driven Geoscience: Application to Dynamics in Mobile Belts). K.U. was supported by Japan Society for the Promotion of Science KAKENHI Grant Numbers JP15H05833 , JP17H02063 , and JP19K04026 , and T.K. was supported by Japan Society for the Promotion of Science KAKENHI Grant numbers JP15K20864 and JP25120005 and by Japan Science and Technology Agency PRESTO Grant Number JPMJPR1676 . S.A. and T.K. were supported by Japan Science and Technology Agency CREST Grant No. JPMJCR1761 . Some of the experimental data used for the model-selection and parameter optimization were obtained from the Library of Experimental Phase Relations open database of melting experiments ( Hirschmann et al., 2008 ). The R source code and dataset used in this study are provided in Supplementary materials 1 and 2 respectively.
Publisher Copyright:
© 2020 The Authors
PY - 2020/3
Y1 - 2020/3
N2 - Water in silicate melt influences the phase relations of a hydrous-melt system. Given the importance of water in silicate melts, a quantitative thermodynamic understanding of the non-ideality of hydrous melt is necessary to properly model natural magmatic processes. This paper presents a novel method for quantitative thermodynamic modeling of hydrous-melt–olivine equilibrium. Specifically, a machine learning method, exhaustive variable selection (ES), is used to model the non-ideality of hydrous melts. Using the ES method, we quantitatively validate the predictive capacities of all possible combinations of variables and then adopt the combination with the highest predictive capacity as the optimal model equation. The ES method allows us to obtain the underlying thermodynamic relationship of the hydrous-melt–olivine system, such as the relative importance of different variables to the thermodynamic equilibrium, as well as to construct a robust and generalized model. We show that the combination of a linear term and a squared term of the total water concentration of melt is significant for describing the hydrous-melt–olivine equilibrium. This result is interpreted in terms of the microstructural changes related to the dissociation of water in silicate melt. Calculations using the optimal model reproduce the experimentally determined effects of water on the olivine liquidus and the distribution coefficient for Mg between olivine and hydrous melt. Our study demonstrates that the ES method yields a thermodynamic equilibrium model that captures the essential thermodynamic relationship explaining the high-dimensional and complex experimental data.
AB - Water in silicate melt influences the phase relations of a hydrous-melt system. Given the importance of water in silicate melts, a quantitative thermodynamic understanding of the non-ideality of hydrous melt is necessary to properly model natural magmatic processes. This paper presents a novel method for quantitative thermodynamic modeling of hydrous-melt–olivine equilibrium. Specifically, a machine learning method, exhaustive variable selection (ES), is used to model the non-ideality of hydrous melts. Using the ES method, we quantitatively validate the predictive capacities of all possible combinations of variables and then adopt the combination with the highest predictive capacity as the optimal model equation. The ES method allows us to obtain the underlying thermodynamic relationship of the hydrous-melt–olivine system, such as the relative importance of different variables to the thermodynamic equilibrium, as well as to construct a robust and generalized model. We show that the combination of a linear term and a squared term of the total water concentration of melt is significant for describing the hydrous-melt–olivine equilibrium. This result is interpreted in terms of the microstructural changes related to the dissociation of water in silicate melt. Calculations using the optimal model reproduce the experimentally determined effects of water on the olivine liquidus and the distribution coefficient for Mg between olivine and hydrous melt. Our study demonstrates that the ES method yields a thermodynamic equilibrium model that captures the essential thermodynamic relationship explaining the high-dimensional and complex experimental data.
KW - Basalt
KW - Hydrous melt
KW - Machine learning
KW - Mantle melting
KW - Thermodynamic equilibrium model
KW - Thermodynamics
UR - http://www.scopus.com/inward/record.url?scp=85079362039&partnerID=8YFLogxK
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U2 - 10.1016/j.pepi.2020.106430
DO - 10.1016/j.pepi.2020.106430
M3 - Article
AN - SCOPUS:85079362039
SN - 0031-9201
VL - 300
JO - Physics of the Earth and Planetary Interiors
JF - Physics of the Earth and Planetary Interiors
M1 - 106430
ER -