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Compression behavior and structure of dense helium at high temperatures by molecular dynamics simulation

机译:分子动力学模拟研究高温下高密度氦的压缩行为和结构

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In this work, the isotherm and energy distribution at T=304 K of dense helium are studied by molecular dynamic (MD) simulations with exp-6 potential r~*=2.967 3 A (the position of the well min- imum) and ε/k_B=10.8 K (ε is the well-depth and k_B is the Boltzmann constant) given by Peter et al., and different values of stiffness parameter α. The optimized value of α=12.7 is deduced that can de- scribe the atomic interactions for dense helium satisfactorily. This optimized αin exp-6 potential is used to conduct MD simulations of two isotherms of dense helium at T=300 K and T=298 K. The calcula- tions are in good agreement with the experimental. We further employed this method to investigate the equation-of-state and structure of dense helium at higher temperatures and found that when the density remained 1.6 g/cm~3, the second peak of the radial distribution function would disappear in the tempera- ture range from 2 000 to 040 K, demonstrating that a solid-liquid transition or decrystallization had oc- curred.
机译:在这项工作中,通过exp-6电位r〜* = 2.967 3 A(最小阱位置)和ε的分子动力学(MD)模拟研究了密集氦在T = 304 K时的等温线和能量分布。 Peter等人给出的/k_B=10.8 K(ε是井深,k_B是玻尔兹曼常数),并且刚度参数α的值不同。推导了α= 12.7的最佳值,可以令人满意地描述稠密氦的原子相互作用。优化的αinexp-6势用于在T = 300 K和T = 298 K时对两个重氦等温线进行MD模拟。计算结果与实验结果吻合良好。我们进一步利用这种方法研究了高温下致密氦的状态方程和结构,发现当密度保持在1.6 g / cm〜3时,径向分布函数的第二个峰值将在温度下消失。范围从2000到040 K,表明发生了固液转变或去结晶。

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