{"title":"Equation of state and Hugoniot of warm dense xenon: Application of average atom-in-jellium model","authors":"Guicun Ma, Jin Qi","doi":"10.1016/j.hedp.2024.101083","DOIUrl":null,"url":null,"abstract":"<div><p>In warm dense xenon, thermally excited and pressure-ionized electrons are essential for calculating the equation of state; however, the classical Thomas Fermi model is unsuitable for describing this state. Therefore it is necessary to find an appropriate theoretical model to express the thermal characteristics of electrons in warm dense Xe. In this study, we use the average atom-in-jellium(AJ) model to compute the contribution of thermally excited and pressure-ionized electrons of Xe over a wide range of temperatures and densities. The electron resonance state in the AJ model is treated by the adaptive mesh movement method. Moreover a method for correcting the cold pressure curve(which is used in the liquid phase calculations) in the AJ model is proposed. For the liquid phase, the ion motion contribution is expressed by the liquid perturbation theory of the corrected rigid-ion sphere model. For the solid phase, the ion motion contribution is described by the Debye model combined with anharmonic correction. Our calculated Hugoniot curve of Xe coincides with those of the experiments, first-principles density functional calculations and other theoretical models. The melting line of Xe is also consistent with the results of first-principle calculations and other theoretical models.</p></div>","PeriodicalId":49267,"journal":{"name":"High Energy Density Physics","volume":"50 ","pages":"Article 101083"},"PeriodicalIF":1.6000,"publicationDate":"2024-02-03","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"High Energy Density Physics","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1574181824000089","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"PHYSICS, FLUIDS & PLASMAS","Score":null,"Total":0}
引用次数: 0
Abstract
In warm dense xenon, thermally excited and pressure-ionized electrons are essential for calculating the equation of state; however, the classical Thomas Fermi model is unsuitable for describing this state. Therefore it is necessary to find an appropriate theoretical model to express the thermal characteristics of electrons in warm dense Xe. In this study, we use the average atom-in-jellium(AJ) model to compute the contribution of thermally excited and pressure-ionized electrons of Xe over a wide range of temperatures and densities. The electron resonance state in the AJ model is treated by the adaptive mesh movement method. Moreover a method for correcting the cold pressure curve(which is used in the liquid phase calculations) in the AJ model is proposed. For the liquid phase, the ion motion contribution is expressed by the liquid perturbation theory of the corrected rigid-ion sphere model. For the solid phase, the ion motion contribution is described by the Debye model combined with anharmonic correction. Our calculated Hugoniot curve of Xe coincides with those of the experiments, first-principles density functional calculations and other theoretical models. The melting line of Xe is also consistent with the results of first-principle calculations and other theoretical models.
期刊介绍:
High Energy Density Physics is an international journal covering original experimental and related theoretical work studying the physics of matter and radiation under extreme conditions. ''High energy density'' is understood to be an energy density exceeding about 1011 J/m3. The editors and the publisher are committed to provide this fast-growing community with a dedicated high quality channel to distribute their original findings.
Papers suitable for publication in this journal cover topics in both the warm and hot dense matter regimes, such as laboratory studies relevant to non-LTE kinetics at extreme conditions, planetary interiors, astrophysical phenomena, inertial fusion and includes studies of, for example, material properties and both stable and unstable hydrodynamics. Developments in associated theoretical areas, for example the modelling of strongly coupled, partially degenerate and relativistic plasmas, are also covered.