We present an emulation-based approach to understand the interactions among different chemical and biological processes modelled in environmental reactive transport models (RTMs) and explore how the parameterisation of these processes influences the results of multi-component RTMs. We utilise a previously published RTM consisting of 20 primary species, 20 secondary complexes, 17 mineral reactions, and 2 biologically mediated reactions; this RTM describes bio-stimulation using sediment from a contaminated aquifer. We choose a subset of the input parameters to vary over a range of values. The result is the construction of a new dataset that describes the model behaviour over a range of environmental conditions. Using this dataset to train a statistical model creates an emulator of the underlying RTM. This is a condensed representation of the original RTM that facilitates rapid exploration of a broad range of environmental conditions and sensitivities. As an illustration of this approach, we use the emulator to explore how varying the boundary conditions in the RTM describing the aquifer impacts the rates and volumes of mineral precipitation. A key result of this work is the recognition of an unanticipated dependency of pyrite precipitation on p CO 2 in the injection fluid due to the stoichiometry of the microbially mediated sulfate reduction reaction. This complex relationship was made apparent by the emulator, while the underlying RTM was not specifically constructed to create such a feedback. We argue that this emulation approach to sensitivity analysis for RTMs may be useful in discovering such new coupled sensitives in geochemical systems and for designing experiments to optimise environmental remediation. Finally, we demonstrate that this approach can maximise specific mineral precipitation or dissolution reactions by using the emulator to find local maxima, which can be widely applied in environmental systems.
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Newcastle Univ, Sch Math Stat & Phys, Herschel Bldg, Newcastle Upon Tyne NE1 7RU, EnglandNewcastle Univ, Sch Math Stat & Phys, Herschel Bldg, Newcastle Upon Tyne NE1 7RU, England
Harnois-Deraps, Joachim
Hernandez-Aguayo, Cesar
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Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85748 Garching, Germany
Excellence Cluster ORIGINS, Bolrzmannstr 2, D-85748 Garching, GermanyNewcastle Univ, Sch Math Stat & Phys, Herschel Bldg, Newcastle Upon Tyne NE1 7RU, England
Hernandez-Aguayo, Cesar
Cuesta-Lazaro, Carolina
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Harvard & Smithsonian, Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
NSF AI Inst Artificial Intelligence & Fundamental, Cambridge, MA 02139 USA
MIT, Dept Phys, Cambridge, MA 02139 USA
Univ Durham, Inst Computat Cosmol, Dept Phys, South Rd, Durham DH1 3LE, EnglandNewcastle Univ, Sch Math Stat & Phys, Herschel Bldg, Newcastle Upon Tyne NE1 7RU, England
Cuesta-Lazaro, Carolina
Arnold, Christian
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Univ Durham, Inst Computat Cosmol, Dept Phys, South Rd, Durham DH1 3LE, EnglandNewcastle Univ, Sch Math Stat & Phys, Herschel Bldg, Newcastle Upon Tyne NE1 7RU, England
Arnold, Christian
Li, Baojiu
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Univ Durham, Inst Computat Cosmol, Dept Phys, South Rd, Durham DH1 3LE, EnglandNewcastle Univ, Sch Math Stat & Phys, Herschel Bldg, Newcastle Upon Tyne NE1 7RU, England
Li, Baojiu
Davies, Christopher T.
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Ludwig Maximilians Univ Munchen, Fac Phys, Scheinerstr 1, D-81679 Munich, GermanyNewcastle Univ, Sch Math Stat & Phys, Herschel Bldg, Newcastle Upon Tyne NE1 7RU, England
Davies, Christopher T.
Cai, Yan-Chuan
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Univ Edinburgh, Inst Astron, Blackford Hill, Edinburgh EH9 3HJ, ScotlandNewcastle Univ, Sch Math Stat & Phys, Herschel Bldg, Newcastle Upon Tyne NE1 7RU, England