Atomic-scale mechanism of carbon nucleation from a deep crustal fluid by replica exchange reactive molecular dynamics simulation

被引:4
|
作者
Leyssale, Jean-Marc [1 ]
Galvez, Matthieu E. [2 ,3 ,4 ]
Valdenaire, Pierre-Louis [5 ]
Pellenq, Roland [5 ,6 ]
van Duin, Adri C. T. [7 ]
机构
[1] Univ Bordeaux, CNRS, Bordeaux INP, ISM,UMR 5255, F-33400 Talence, France
[2] Univ Lausanne, Inst Sci Terre, Fac Geosci & Environm, CH-1015 Lausanne, Switzerland
[3] Swiss Fed Inst Technol, Soc Sci Branco Weiss Fellowship, CH-8092 Zurich, Switzerland
[4] Swiss Fed Inst Technol, Dept Earth Sci, CH-8092 Zurich, Switzerland
[5] MIT, CNRS MIT Aix Marseille Univ Joint Lab MultiScale, IRL 3466, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[6] George Washington Univ, Childrens Natl Med Ctr, Childrens Res Inst, EpiDaPo Lab,CNRS, 111 Michigan Ave NW, Washington, DC 20010 USA
[7] Penn State Univ, Dept Mech & Nucl Engn, University Pk, PA 16802 USA
关键词
Carbon cycle; Graphite; Soot; Hydrothermal synthesis; Crustal fluid; Reactive MD; FORCE-FIELD; GRAPHITE DEPOSITS; ORGANIC-CARBON; REAXFF; OXYGEN; GRAPHITIZATION; HYDROCARBONS; PRESSURE; DIOXIDE; WATER;
D O I
10.1016/j.gca.2022.04.024
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
We present a mechanistic model of carbon nucleation and growth from a fluid at elevated temperature (T) and pressure conditions, typical of those found in the shallow Earth's lithosphere. Our model uses a replica exchange reactive molecular dynamics framework in which molecular configurations are swapped between adjacent T replica at regular intervals according to underlying statistical mechanics. This framework allows predicting complex molecular structures and thermodynamics while remaining computationally efficient. Here we simulate the reactivity of an unstable mixture of CO2 and CH4 at 1000 K and 1 GPa. We find that the path to thermodynamic equilibrium is initially entropy-driven, producing a diversity of short-lived species, including various alcohols with intermediate carbon oxidation states. Cyclic and polycyclic radicals that are sometimes resonance-stabilized form next and set the stage for carbon nucleation. The carbon exsolution process releases abundant water, is exothermic and starts with the nucleation of a large aggregate of hydrogenated graphene flakes from covalently bonded poly cyclic units. The carbon backbone of this nucleus subsequently grows into a hydrogen-depleted fullerene-like structure, before evolving toward a partially bilayered graphene layer. Overall, our results show that the mechanism of graphitic C formation is certainly not bimolecular, and that it may involve a combination of key condensation and radical chain reactions. This will help understand the isotopic, and reactive characteristics of carbon-bearing fluids during their upward transit through the Earth's mantle and crust. Moreover, the mechanistic insights outlined here present intriguing similarities with the process of soot and interstellar dust formation, which suggests that the widespread distribution of abiotic polyaromatic and graphitic material on Earth and beyond may reflect the prevalence of a fundamental chemical pathway.(C) 2022 Published by Elsevier Ltd.
引用
收藏
页码:106 / 118
页数:13
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