Planetary physics research programme at the Facility for Antiprotons and Ion Research at Darmstadt
Planetary physics research programme at the Facility for Antiprotons and Ion Research at Darmstadt
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DOI：
10.1002/ctpp.201700076
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发表时间：
2017-11
影响因子：
1.6
通讯作者：
N. Tahir;I. Lomonosov;B. Borm;A. R. Piriz;P. Neumayer;A. Shutov;V. Bagnoud;S. Piriz
中科院分区：
文献类型：
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作者：
N. Tahir;I. Lomonosov;B. Borm;A. R. Piriz;P. Neumayer;A. Shutov;V. Bagnoud;S. Piriz
行星物理研究是达姆施塔特反质子和离子研究设施高能密度物理方案的一个重要部分。在本文中，我们报告了一个拟议的实验命名为实验室PLANETAL科学（LAPLAS）的数值模拟。这些模拟表明，在这样的实验中，铁样品可以内爆到极端的物理条件，预计存在于地球内部和更大质量的岩石行星内部，称为超级地球。因此，LAPLAS实验将提供关于HED Fe的状态方程（EOS）和输运性质的非常有价值的信息，这将有助于科学家了解太阳系行星和太阳系外行星的结构和演化。
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.