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光谱证据表明,在硅酸盐玻璃和熔体中存在压力诱导的配位变化。

Spectroscopic evidence for pressure-induced coordination changes in silicate glasses and melts.

出版信息

Science. 1988 Feb 19;239(4842):902-5. doi: 10.1126/science.239.4842.902.

Abstract

Infrared spectra demonstrate that at pressures above 20 gigapascals and room temperature the regular tetrahedral coordination of oxygen around both silicon and aluminum ions is severely disrupted in SiO(2), CaMgSi(2)O(6), and CaAlSi(2)O(8) composition glasses. The spectra are consistent with gradual, pressure-induced increases in the coordination numbers of silicon and aluminum. A variety of coordination environments, from sixfold to fourfold, appears to be present at pressures as high as about 40 gigapascals. This apparent change in coordination is not quenchable at room temperature: on decompression, the glasses return to tetrahedral coordination. This continuous and reversible coordination change in amorphous silicates explains the lack of observation of coordination changes in silicate glasses quenched from high pressure, the shallow melting slopes observed for mantle silicates at high pressures, and the possible presence of neutrally buoyant magmas deep within the terrestrial planets.

摘要

红外光谱表明,在 200 吉帕斯卡以上的压力和室温下,SiO2、CaMgSi2O6 和 CaAlSi2O8 组成的玻璃中,硅和铝离子周围的正四面体配位严重受到破坏。这些光谱与硅和铝的配位数逐渐增加的压力诱导效应一致。在高达约 400 吉帕斯卡的压力下,似乎存在各种配位环境,从六配位到四配位。这种配位的明显变化在室温下无法淬灭:减压时,玻璃恢复为四面体配位。非晶态硅酸盐中这种连续的、可逆的配位变化解释了在从高压淬火的硅酸盐玻璃中观察不到配位变化的原因,也解释了在地幔硅酸盐在高压下观察到的浅熔化斜率的原因,还可能解释了在地球行星内部深处存在中性浮力岩浆的原因。

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