Isentropic Compression of Condensed Hydrogen Up to Megabar Pressure

A. Bykov, N. I. Egorov, G. V. Boriskov, M. I. Dolotenko, Y. Kuropatkin, N. Lukyanov, V. D. Mironenko, S. Belov, V. G. Belyashkin, M. Lomonosov
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Abstract

The paper describes a device for isentropic compression of frozen gases by pressure of the ultra-high magnetic field generated by the cascade magnetocumulative generator MC-1 (MC-1 EMG). The paper provides test data on isentropic compression of solid hydrogen up to ∼ 3 Mbar. Brief description of a technique for the test data analysis is provided as well as the comparison between this data and the computation. The interest to a hydrogen equation of state within the megabar pressure range is caused by wide hydrogen spread in the universe and its presence in stars and giant planets. Also many applied problems as well as metal hydrogen manufacture can be solved by solving the problem of thermonuclear fusion. Though hydrogen has a primitive single-electron structure that in principle allows direct calculations of high-density states to be performed, the difficulties of the correct consideration for strong interparticle interaction result in construction of differing theoretical models. In these conditions it becomes important to get experimental data on hydrogen compression within the wide range of parameters. The hydrogen “cool” equation of state within the megabar pressure range is possible only with the help of anvil static technique and isentropic compression technique using the ultra-high magnetic field that has been developed at our institute. The goal of this work is plotting a “cool” hydrogen equation of state within the pressure range 1 – 4 Mbar, when thermal pressure component is negligibly small as compared to an elastic one, and full pressure in the substance practically matches the elastic pressure. This goal can be reached using the technique of condensed hydrogen isentropic compression by ultra-high magnetic filed generated by MC-1 generator. A principal schematic of the device is provided in Fig. 1.
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百万巴压力下凝聚氢的等熵压缩
本文介绍了一种利用级联磁累积发生器MC-1 (MC-1 EMG)产生的超高磁场的压力对冷冻气体进行等熵压缩的装置。本文提供了固体氢等熵压缩~ 3mbar的实验数据。简要介绍了一种试验数据分析技术,并与计算结果进行了比较。对兆巴压力范围内的氢状态方程的兴趣是由于氢在宇宙中的广泛分布以及它在恒星和巨行星中的存在。通过解决热核聚变问题,可以解决许多应用问题以及金属氢的制造问题。虽然氢具有原始的单电子结构,原则上允许进行高密度态的直接计算,但正确考虑强粒子间相互作用的困难导致了不同理论模型的构建。在这种情况下,在较宽的参数范围内获得氢气压缩的实验数据变得很重要。在兆巴压力范围内的氢“冷”态方程,只有借助我所开发的超高磁场的砧静技术和等熵压缩技术才能实现。这项工作的目标是在1 - 4mbar压力范围内绘制一个“冷”氢状态方程,此时热压力分量与弹性压力相比可以忽略不计,并且物质中的全压力实际上与弹性压力相匹配。利用MC-1发生器产生的超高磁场压缩凝聚氢等熵技术可以实现这一目标。该装置的主要原理图如图1所示。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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