2020
DOI: 10.1038/s41598-020-61644-5
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Formation of complex hydrocarbon systems from methane at the upper mantle thermobaric conditions

Abstract: the existence of methane in the earth's mantle does not cause any doubt, however, its possible chemical transformation under the mantle thermobaric conditions is not enough known. investigation of methane at the upper mantle thermobaric conditions, using diamond anvil cells, demonstrated the possible formation of ethane, propane and n-butane from methane, however, theoretical calculations of methane behaviour at extreme temperature and pressure predicted also heavier hydrocarbons. We experimentally investigate… Show more

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Cited by 17 publications
(8 citation statements)
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“…The origin and fate of methane (CH 4 ) continues to be a compelling topic of investigation, both on Earth, for its important role in energy and climate studies, in biogeochemical cycling on the planet's surface and subsurface biosphere, and for moons and planets elsewhere in the solar system. [1][2][3][4][5][6][7][8] Biotic CH 4 is produced either microbially or through the thermal decomposition of organic matter whereas abiotic CH 4 is produced through chemical reactions that do not directly involve organic matter but include both high-temperature processes related to magmatic activity [9][10][11][12] and low-temperature abiotic organic synthesis related to processes of water-rock reaction such as serpentinization. 3,13 Differentiating between such sources remains a challenge.…”
Section: Introductionmentioning
confidence: 99%
“…The origin and fate of methane (CH 4 ) continues to be a compelling topic of investigation, both on Earth, for its important role in energy and climate studies, in biogeochemical cycling on the planet's surface and subsurface biosphere, and for moons and planets elsewhere in the solar system. [1][2][3][4][5][6][7][8] Biotic CH 4 is produced either microbially or through the thermal decomposition of organic matter whereas abiotic CH 4 is produced through chemical reactions that do not directly involve organic matter but include both high-temperature processes related to magmatic activity [9][10][11][12] and low-temperature abiotic organic synthesis related to processes of water-rock reaction such as serpentinization. 3,13 Differentiating between such sources remains a challenge.…”
Section: Introductionmentioning
confidence: 99%
“…Hydrogen is the most abundant element in the universe, and hydrogen transfer (H-transfer) under high pressure is of great importance to petroleum science, geoscience, planetary science, chemistry, and bioscience. It is the key step in the C–H circulation inside the earth, the reaction of organics and inorganics in giant planets, and the synthesis of high-temperature superconductors . Typical H-transfer usually occurs via a hydrogen bond (H-bond), which can be tuned in very small steps but on very large energy scales under high pressure, hence changing the kinetics and even the thermodynamics of the H-transfer.…”
mentioning
confidence: 99%
“…The synthesis process of the BiScO 3 samples of the perovskite phase was carried out using the URS-2 large reactive volume unit produced by the Technological Institute for Superhard and New Carbon Materials (TIS-NUM), Ministry of Science of the Russian Federation, Troitsk, Moscow region. 19 The initial powders used for the synthesis were tightly loaded into a cylindrical steel capsule with a diameter of 8 mm and a height of 5 mm, which was installed inside a toroidal pressure chamber made of calcite. Two resistive heaters made of a mixture of graphite and aluminum oxide were mounted on the upper and lower surfaces of the capsule.…”
mentioning
confidence: 99%