MHz free electron laser x-ray diffraction and modeling of pulsed laser heated diamond anvil cell

Author:

Jaisle Nicolas1ORCID,Cébron David1ORCID,Konôpková Zuzana2ORCID,Husband Rachel J3ORCID,Prescher Clemens4ORCID,Cerantola Valerio2ORCID,Dwivedi Anand2ORCID,Kaa Johannes M.5ORCID,Appel Karen2ORCID,Buakor Khachiwan2ORCID,Ball Orianna B.6ORCID,McWilliams Ryan S.6,Strohm Cornelius3ORCID,Nakatsutsumi Motoaki2ORCID,Zastrau Ulf2ORCID,Baehtz Carsten2ORCID,Anna Baron Marzena7ORCID,Edmund Eric8ORCID,Biswas Joydipa4ORCID,McHardy James D.9ORCID,Sturtevant Blake T.10ORCID,Ehm Lars11ORCID,Goncharov Alexander F.8ORCID,McMahon Malcolm I.9ORCID,Buchen Johannes12ORCID,Cynn Hyunchae13ORCID,Pace Edward J.9ORCID,Liermann Hanns-Peter3ORCID,Sneed Daniel T.13ORCID,Cooper Samantha C.10,Anae Madison11ORCID,Kim Jaeyong14ORCID,Wu Zhongyan14ORCID,Lee Yongjae15ORCID,Hwang Huijeong J.15,Kim Taehyun15ORCID,Choi Jinhyuk15,Lee Jeongmin15ORCID,Merkel Sébastien7ORCID,Chantel Julien7ORCID,Koemets Egor G.12,Marquardt Hauke12ORCID,Prakapenka Vitali B.16ORCID,Chariton Stella16ORCID,Shevchenko Elena16,Fiquet Guillaume17ORCID,Rosa Angelika D.18ORCID,Mezouar Mohamed18,Garbarino Gaston18ORCID,Morard Guillaume1ORCID

Affiliation:

1. Université Grenoble Alpes, Université Savoie Mont Blanc, CNRS, IRD, Université Gustave Eiffel, ISTerre 1 , 38000 Grenoble, France

2. European XFEL GmbH 2 , Holzkoppel 4, Schenefeld, Germany

3. DESY Deutsches Elektronen-Synchrotron 3 , Notkestr. 85, Hamburg, Germany

4. Institute of Earth and Environmental Sciences, Albert-Ludwigs University of Freiburg 4 , Freiburg, Germany

5. Technische Universität Dortmund, Fakultät Physik/DELTA 5 , Maria-Goeppert-Mayer-Straße 2, 44227 Dortmund, Germany

6. School of Physics and Astronomy, University of Edinburgh 6 , Edinburgh, United Kingdom

7. Univ. Lille, CNRS, INRAE, Centrale Lille, UMR 8207 - UMET - Unité Matériaux et Transformations 7 , F-59000 Lille, France

8. Earth and Planets Laboratory, Carnegie Institution for Science 8 , Washington, DC 20015, USA

9. School of Physics and Astronomy, University of Edinburgh 9 , Edinburgh, Unite Kingdom

10. Los Alamos National Laboratory 10 , Los Alamos 87545, USA

11. Department of Geosciences, Stony Brook University 11 , 255 Earth and Space Sciences Building, Stony Brook, New York 11794, USA

12. Department of Earth Sciences, University of Oxford 12 , Oxford OX1 3AN, United Kingdom

13. Lawrence Livermore National Laboratory 13 , Livermore 94550, USA

14. Department of Physics, Hanyang University 14 , Haengdang dong, Seoul, South Korea

15. Yonsei University, Department of Earth System Sciences 15 , Yonsei, South Korea

16. University of Chicago, CNM, ANL 16 , Chicago 60637, USA

17. Institut Minéralogie, de Physique des Matériaux et de Cosmochimie, Sorbonne Université 17 , 4 Place Jussieu, Paris, France

18. European Synchrotron Radiation Facility 18 , Grenoble, France

Abstract

A new diamond anvil cell experimental approach has been implemented at the European x-ray Free Electron Laser, combining pulsed laser heating with MHz x-ray diffraction. Here, we use this setup to determine liquidus temperatures under extreme conditions, based on the determination of time-resolved crystallization. The focus is on a Fe-Si-O ternary system, relevant for planetary cores. This time-resolved diagnostic is complemented by a finite-element model, reproducing temporal temperature profiles measured experimentally using streaked optical pyrometry. This model calculates the temperature and strain fields by including (i) pressure and temperature dependencies of material properties, and (ii) the heat-induced thermal stress, including feedback effect on material parameter variations. Making our model more realistic, these improvements are critical as they give 7000 K temperature differences compared to previous models. Laser intensities are determined by seeking minimal deviation between measured and modeled temperatures. Combining models and streak optical pyrometry data extends temperature determination below detection limit. The presented approach can be used to infer the liquidus temperature by the appearance of SiO2 diffraction spots. In addition, temperatures obtained by the model agree with crystallization temperatures reported for Fe–Si alloys. Our model reproduces the planetary relevant experimental conditions, providing temperature, pressure, and volume conditions. Those predictions are then used to determine liquidus temperatures at experimental timescales where chemical migration is limited. This synergy of novel time-resolved experiments and finite-element modeling pushes further the interpretation capabilities in diamond anvil cell experiments.

Funder

HORIZON EUROPE European Research Council

European Research Council

Publisher

AIP Publishing

Subject

General Physics and Astronomy

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