Matter and Radiation at Extremes
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2016, 1(5) Column

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Matter and Radiation at Extremes 第1卷 第5期

Author Affiliations
Abstract
1 Macedonian Academy of Sciences and Arts, P.O. Box 428, 1000 Skopje, Macedonia
2 School of Physics and Information Technology, Shaanxi Normal University, Xi'an 710119, China
3 Key Laboratory of Computational Physics, Institute of Applied Physics and Computational Mathematics, P.O. Box 8009, Beijing 100088, China
Hot, dense plasmas exhibit screened Coulomb interactions, resulting from the collective effects of correlated many-particle interactions. In the lowest particle correlation order (pair-wise correlations), the interaction between charged plasma particles reduces to the DebyeeHu¨ckel (Yukawa-type) potential, characterized by the Debye screening length. Due to the importance of Coulomb interaction screening in dense laboratory and astrophysical plasmas, hundreds of theoretical investigations have been carried out in the past few decades on the plasma screening effects on the electronic structure of atoms and their collision processes employing the DebyeeHu¨ckel screening model. The present article aims at providing a comprehensive review of the recent studies in atomic physics in Debye plasmas. Specifically, the work on atomic electronic structure, photon excitation and ionization, electron/positron impact excitation and ionization, and excitation, ionization and charge transfer of ion-atom/ion collisions will be reviewed.
Debye plasmas Debye plasmas Screened Coulomb potential Screened Coulomb potential Atomic structure Atomic structure Collision dynamics Collision dynamics 
Matter and Radiation at Extremes
2016, 1(5): 237
Author Affiliations
Abstract
1 Institute of Applied Physics and Computational Mathematics, Beijing 10094, China
2 Laboratory of Computational Physics, Beijing 100088, China
3 National Hi-Tech Inertial Confinement Fusion Committee of China, Beijing 100088, China
A sharp density increase (referred to as density incrustation) of the Au plasmas in the radiative cooling process of high-Z Au plasmas confined by low-Z CH plasmas is found through the radiative hydrodynamic simulations. The temperature of Au plasmas changes obviously in the cooling layer while the pressure remains constant. Consequently, the Au plasmas in the cooling layer are compressed, and the density incrustation is formed. It is also shown that when the high-Z plasma opacity decreases or the low-Z plasma opacity increases, the peak density of the density incrustation becomes lower and the thickness of the density incrustation becomes wider. This phenomenon is crucial to the RayleigheTaylor instability at the interface of high-Z and low-Z plasmas, since the density variation of Au plasmas has a considerable influence on the Atwood number of the interface.
Density incrustation Density incrustation Radiation hydrodynamics Radiation hydrodynamics Opacity Opacity 
Matter and Radiation at Extremes
2016, 1(5): 249
Author Affiliations
Abstract
Data Center for High Energy Density Physics Research, Institute of Applied Physics and Computational Mathematics, Beijing 100088, PR China
Self-consistent calculations of energy loss for a Ga ion moving in hot Au plasmas are made under the assumption of wide ranges of the projectile energy and the plasma temperature with all important mechanisms considered in detail. The relevant results are found to be quite different from those of an a particle or a proton. One important reason for this is the rapid increasing of the charge state of a Ga ion at plasma temperature. This reason also leads to the inelastic stopping which does not always decrease with the increase of plasma temperature, unlike the case of an a particle. The nuclear stopping becomes very important at high enough plasma temperature due to the heavy reduced mass of a Ga and an Au ion and the above-mentioned reason. The well-known binary collision model [Phys. Rev. 126 (1962) 1] and its revised one [Phys. Rev. A 29 (1984) 2145] are not working or unsatisfactory in this case.
Energy loss Energy loss Hot Au plasma Hot Au plasma Ga ion Ga ion 
Matter and Radiation at Extremes
2016, 1(5): 257
Author Affiliations
Abstract
1 National Research Tomsk State University, Tomsk 634050, Russia
2 Institute of High Current Electronics, Russian Academy of Sciences, SB, Tomsk 634055, Russia
The results of theoretical simulation of runaway electron generation in high-pressure pulsed gas discharge with inhomogeneous electric field are presented. Hydrodynamic and kinetic approaches are used simultaneously to describe the dynamics of different components of lowtemperature discharge plasma. Breakdown of coaxial diode occurs in the form of a dense plasma region expanding from the cathode. On this background there is a formation of runaway electrons that are initiated by the ensemble of plasma electrons generated in the place locally enhanced electric field in front of dense plasma. It is shown that the power spectrum of fast electrons in the discharge contains electron group with the so-called “anomalous” energy.
Pulsed gas discharge Pulsed gas discharge High-pressure gas breakdown High-pressure gas breakdown Fast electron in gas discharge Fast electron in gas discharge Runaway electron in plasma Runaway electron in plasma 
Matter and Radiation at Extremes
2016, 1(5): 264
Qiang He 1,2,3Xi Liu 1,2,*Baosheng Li 4Liwei Deng 5[ ... ]Liping Wang 6
Author Affiliations
Abstract
1 Key Laboratory of Orogenic Belts and Crustal Evolution, Ministry of Education of China, Beijing 100871, China
2 School of Earth and Space Sciences, Peking University, Beijing 100871, China
3 Institute of Fluid Physics, China Academy of Engineering Physics, Mianyang 621900, China
4 Mineral Physics Institute, Stony Brook University, Stony Brook, NY 11794-2100, USA
5 Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China
6 High Pressure Science and Engineering Center and Department of Physics and Astronomy, University of Nevada, Las Vegas, NV 89154, USA
The thermal equation of state of a natural kyanite has been investigated with a DIA-type, cubic-anvil apparatus (SAM85) combined with an energy-dispersive synchrotron X-ray radiation technique up to 8.55 GPa and 1273 K. No phase transition was observed in the studied pressuretemperature (P-T ) range. The Le Bail full profile refinement technique was used to derive the unit-cell parameters. By fixing the bulk modulus K0 as 196 GPa and its pressure derivative K'0 as 4, our P-V (volume)-T data were fitted to the high temperature BircheMurnaghan equation of state. The obtained parameters for the kyanite are: V0=294.05(9)(10-10)3, α02.53(11)× 10-5K-1 and (?K/?T )P =-0.021(8) GPa?K-1. These parameters have been combined with other experimentally-measured thermodynamic data for the relevant phases to calculate the P-T locus of the reaction kyanite = stishovite+ corundum. With this thermodynamically constrained phase boundary, previous high-pressure phase equilibrium experimental studies with the multi-anvil press have been evaluated.
Kyanite Kyanite X-ray diffraction X-ray diffraction Thermal equation of state Thermal equation of state High-pressure and high-temperature High-pressure and high-temperature Kyanite decomposition Kyanite decomposition Thermodynamic calculation Thermodynamic calculation 
Matter and Radiation at Extremes
2016, 1(5): 269

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