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Phase transition in SiC from zinc-blende to rock-salt structure and implications for carbon-rich extrasolar planets

机译:SiC从锌 - 融合到岩盐结构的相转变和碳富碳含量行星的影响

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We have investigated the phase transition in SiC between the zinc-blende and rock-salt structures at high pressure and temperature in a laser-heated diamond-anvil cell. Results demonstrate that the transition occurs at 74 GPa and 2100 K with a 21% density increase, reflecting the coordination number rising from four to six. In addition, our ab initio calculations show that the boundary has a negative Clapeyron slope of -4.0 MPa/K at 2000 K. The experimentally determined phase boundary is located between those predicted by GGA and B3LYP functional. This transition may take place inside carbon-rich extrasolar planets, forming a boundary with a large density jump. Since SiC is rigid and highly thermally conductive, thermal convection in an SiC-dominant layer is not likely to occur. Nevertheless, the convection may be possible if planet interiors include both silicon carbide and silicate, and in this case the phase transition could affect the style of thermal convection.
机译:我们已经研究了在激光加热的金刚石 - 砧座中的高压和温度下锌 - 混合和岩盐结构之间的SiC相过期。 结果表明,过渡发生在74GPa和2100 k下,增加了21%的密度增加,反映了从4到六个上升的配位数量。 此外,我们的AB Initio计算表明,边界在2000K的2000k处具有-4.0MPa / k的负蛋白斜率。实验确定的相边界位于GGA和B3LYP功能预测的那些之间。 这种过渡可以在碳富碳的溢出行星内进行,形成具有大密度跳跃的边界。 由于SiC是刚性和高度导热的,因此不太可能发生SiC-显性层中的热对流。 然而,如果行星室内设计包括碳化硅和硅酸盐,并且在这种情况下,相位过渡可能会影响热对流的风格。

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