Study of Pocyclic Aromatic Hydrocarbons at a Pressure of 6-9 GPa with X-ray Diffraction and Synchrotron Radiation

被引:3
作者
Chanyshev, A. D. [1 ,2 ]
Litasov, K. D. [1 ,2 ]
Shatskiy, A. F. [1 ,2 ]
Ohtani, E. [3 ]
机构
[1] Russian Acad Sci, Siberian Branch, Sobolev Inst Geol & Mineral, Novosibirsk 630090, Russia
[2] Novosibirsk State Univ, Novosibirsk 630090, Russia
[3] Tohoku Univ, Sendai, Miyagi 9808578, Japan
基金
俄罗斯基础研究基金会;
关键词
O-H FLUID; EARTHS MANTLE;
D O I
10.1134/S1028334X1410016X
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
This work is one of the stages of study of the deep C-O-H fluid and investigates the behavior of polycyclic aromatic hydrocarbons (PAHs) under conditions of the Earth's mantle. The composition of the C-O-H fluid in the upper mantle is estimated as a mixture of H2O and CH4 with a minor amount of H-2 and heavier hydrocarbons. Some theoretical calculations show that the stability of heavy hydrocarbons (alkanes, alkenes, and PAHs) increases with an increase in temperature. This paper presents the results of an XRD study of PAHs stability in multianvil presses on a Spring-8 accelerator (Japan). The primary compositions were chosen according to the abundance of PAHs in nature. In situ diffraction spectrums were recorded to determine the PAHs stability field. It was established that the PAHs become unstable at a pressure of 6-9 GPa and a temperature of 873-1073 K.
引用
收藏
页码:1277 / 1280
页数:4
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