Shock equation of state experiments in MgO up to 1.5 TPa and the effects of optical depth on temperature determination

Author:

Ye Zixuan1,Smith Raymond F.2ORCID,Millot Marius2ORCID,Sims Melissa1ORCID,Tsapetis Dimitrios3ORCID,Shields Michael D.3ORCID,Singh Saransh2ORCID,Hari Anirudh145ORCID,Wicks June K.6ORCID

Affiliation:

1. Department of Earth and Planetary Sciences, Division of Mechanical Engineering, Johns Hopkins University 1 , Baltimore, Maryland 21218, USA

2. Lawrence Livermore National Laboratory 2 , Livermore, California 94550, USA

3. Department of Civil and Systems Engineering, Johns Hopkins University 3 , Baltimore, Maryland 21218, USA

4. Department of Materials Science and Engineering and PULSE Institute, Stanford University 4 , Stanford, California 94305, USA

5. SLAC National Accelerator Laboratory 5 , Menlo Park, California 94025, USA

6. Department of Earth and Planetary Sciences, Johns Hopkins University 6 , Baltimore, Maryland 21218, USA

Abstract

Laser-driven shock compression enables an experimental study of phase transitions at unprecedented pressures and temperatures. One example is the shock Hugoniot of magnesium oxide (MgO), which crosses the B1–B2-liquid triple point at 400–600 GPa, 10 000–13 000 K (0.86–1.12 eV). MgO is a major component within the mantles of terrestrial planets and has long been a focus of high-pressure research. Here, we combine time-resolved velocimetry and pyrometry measurements with a decaying shock platform to obtain pressure–temperature data on MgO from 300 to 1500 GPa and 9000 to 50 000 K. Pressure–temperature–density Hugoniot data are reported at 1500 GPa. These data represent the near-instantaneous response of an MgO [100] single crystal to shock compression. We report on a prominent temperature anomaly between 400 and 460 GPa, in general agreement with previous shock studies, and draw comparison with equation-of-state models. We provide a detailed analysis of the decaying shock compression platform, including a treatment of a pressure-dependent optical depth near the shock front. We show that if the optical depth of the shocked material is larger than 1 μm, treating the shock front as an optically thick gray body will lead to a noticeable overestimation of the shock temperature.

Funder

U.S. Department of Energy

Laboratory Directed Research and Development

Defense Threat Reduction Agency

Publisher

AIP Publishing

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