Planetary physics research programme at the Facility for Antiprotons and Ion Research at Darmstadt

被引：13

作者：

Tahir, N. A. ^{[1
]}

Lomonosov, I. V. ^{[2
,3
,4
,5
]}

Borm, B. ^{[6
]}

Piriz, A. R. ^{[7
]}

Neumayer, P. ^{[1
]}

Shutov, A. ^{[2
]}

Bagnoud, V. ^{[1
]}

Piriz, S. A. ^{[7
]}

机构：

[1] GSI Helmholtzzentrum Schwerionenforsch, Dept Plasma Phys, Darmstadt, Germany

[2] Russian Acad Sci, Inst Problems Chem Phys, Chernogolovka, Russia

[3] Tomsk Univ, Tomsk, Russia

[4] Lomonosov Moscow State Univ, Moscow, Russia

[5] Moscow Inst Phys & Technol, Dolgoprudnyi, Russia

[6] Goethe Univ Frankfurt, Dept Phys, Frankfurt, Germany

[7] Univ Castilla La Mancha, ETSI Ind, Ciudad Real, Spain

来源：

CONTRIBUTIONS TO PLASMA PHYSICS | 2017年 / 57卷 / 10期

关键词：

equation of state; high energy density physics; planetary physics; warm dense matter; HIGH-ENERGY-DENSITY; EQUATION-OF-STATE; NUMERICAL SIMULATIONS; INERTIAL FUSION; DRIVEN; MATTER; HEDGEHOB; GAIN;

D O I：

10.1002/ctpp.201700076

中图分类号：

O35 [流体力学]; O53 [等离子体物理学];

学科分类号：

070204 ; 080103 ; 080704 ;

摘要：

Planetary physics research is an important part of the high energy density (HED) physics programme at the Facility for Antiprotons and Ion Research (FAIR) at Darmstadt. In this paper, we report numerical simulations of a proposed experiment named LAboratory PLAnetary Sciences (LAPLAS). These simulations show that in such experiments, an Fe sample can be imploded to extreme physical conditions that are expected to exist in the interior of the Earth and in the interior of more massive rocky planets named, super-Earths. The LAPLAS experiments will thus provide very valuable information on the equation-of-state (EOS) and transport properties of HED Fe, which will help the scientists to understand the structure and evolution of the planets in our solar system and of the extrasolar system planets.

引用

页码：493 / 498

页数：6

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