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Heuser B, Bergermann A, Stevenson MG, Ranjan D, He Z, Lütgert J, Schumacher S, Bethkenhagen M, Descamps A, Galtier E, Gleason AE, Khaghani D, Glenn GD, Cunningham EF, Glenzer SH, Hartley NJ, Hernandez JA, Humphries OS, Katagiri K, Lee HJ, McBride EE, Miyanishi K, Nagler B, Ofori-Okai B, Ozaki N, Pandolfi S, Qu C, May PT, Redmer R, Schoenwaelder C, Sueda K, Yabuuchi T, Yabashi M, Lukic B, Rack A, Zinta LMV, Vinci T, Benuzzi-Mounaix A, Ravasio A, Kraus D. Release dynamics of nanodiamonds created by laser-driven shock-compression of polyethylene terephthalate. Sci Rep 2024; 14:12239. [PMID: 38806565 PMCID: PMC11133328 DOI: 10.1038/s41598-024-62367-7] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/20/2024] [Accepted: 05/16/2024] [Indexed: 05/30/2024] Open
Abstract
Laser-driven dynamic compression experiments of plastic materials have found surprisingly fast formation of nanodiamonds (ND) via X-ray probing. This mechanism is relevant for planetary models, but could also open efficient synthesis routes for tailored NDs. We investigate the release mechanics of compressed NDs by molecular dynamics simulation of the isotropic expansion of finite size diamond from different P-T states. Analysing the structural integrity along different release paths via molecular dynamic simulations, we found substantial disintegration rates upon shock release, increasing with the on-Hugnoiot shock temperature. We also find that recrystallization can occur after the expansion and hence during the release, depending on subsequent cooling mechanisms. Our study suggests higher ND recovery rates from off-Hugoniot states, e.g., via double-shocks, due to faster cooling. Laser-driven shock compression experiments of polyethylene terephthalate (PET) samples with in situ X-ray probing at the simulated conditions found diamond signal that persists up to 11 ns after breakout. In the diffraction pattern, we observed peak shifts, which we attribute to thermal expansion of the NDs and thus a total release of pressure, which indicates the stability of the released NDs.
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Affiliation(s)
- Ben Heuser
- Institut für Physik, Universität Rostock, Albert-Einstein-Str. 23-24, 18059, Rostock, Germany.
- Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, 01328, Germany.
| | - Armin Bergermann
- Institut für Physik, Universität Rostock, Albert-Einstein-Str. 23-24, 18059, Rostock, Germany
| | - Michael G Stevenson
- Institut für Physik, Universität Rostock, Albert-Einstein-Str. 23-24, 18059, Rostock, Germany
| | - Divyanshu Ranjan
- Institut für Physik, Universität Rostock, Albert-Einstein-Str. 23-24, 18059, Rostock, Germany
- Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, 01328, Germany
| | - Zhiyu He
- Institut für Physik, Universität Rostock, Albert-Einstein-Str. 23-24, 18059, Rostock, Germany
- China Academy of Engineering Physics, Shanghai Institute of Laser Plasma, Shanghai, 201800, China
| | - Julian Lütgert
- Institut für Physik, Universität Rostock, Albert-Einstein-Str. 23-24, 18059, Rostock, Germany
| | - Samuel Schumacher
- Institut für Physik, Universität Rostock, Albert-Einstein-Str. 23-24, 18059, Rostock, Germany
| | - Mandy Bethkenhagen
- LULI, CNRS, CEA, Ecole Polytechnique-Institut Polytechnique de Paris, Sorbonne Université, Palaiseau, 91128, France
| | - Adrien Descamps
- School of Mathematics and Physics, Queen's University Belfast, Belfast, Northern Ireland, BT7 1NN, UK
| | - Eric Galtier
- SLAC National Accelerator Laboratory, Menlo Park, CA, 94025, USA
| | | | - Dimitri Khaghani
- SLAC National Accelerator Laboratory, Menlo Park, CA, 94025, USA
| | - Griffin D Glenn
- SLAC National Accelerator Laboratory, Menlo Park, CA, 94025, USA
- Stanford University, Stanford, CA, 94305, USA
| | | | | | | | - Jean-Alexis Hernandez
- European Synchrotron Radiation Facility, 71 avenue des Martyrs, CS 40220, 38043, Grenoble, France
- The Centre for Earth Evolution and Dynamics (CEED), University of Oslo, Oslo, 0371, Norway
| | - Oliver S Humphries
- Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, 01328, Germany
- European XFEL, Schenefeld, 22869, Germany
| | - Kento Katagiri
- Materials Science and Engineering, Stanford University, Stanford, CA, 94305, USA
| | - Hae Ja Lee
- SLAC National Accelerator Laboratory, Menlo Park, CA, 94025, USA
| | - Emma E McBride
- School of Mathematics and Physics, Queen's University Belfast, Belfast, Northern Ireland, BT7 1NN, UK
| | | | - Bob Nagler
- SLAC National Accelerator Laboratory, Menlo Park, CA, 94025, USA
| | | | - Norimasa Ozaki
- Graduate School of Engineering, Osaka University, Suita, Osaka, 565-0871, Japan
- Photon Pioneers Center, Osaka University, Suita, Osaka, 565-0087, Japan
| | - Silvia Pandolfi
- SLAC National Accelerator Laboratory, Menlo Park, CA, 94025, USA
- Sorbonne Université, Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, IMPMC, Muséum National d'Histoire Naturelle, UMR CNRS 7590, 75005, Paris, France
| | - Chongbing Qu
- Institut für Physik, Universität Rostock, Albert-Einstein-Str. 23-24, 18059, Rostock, Germany
| | - Philipp Thomas May
- Institut für Physik, Universität Rostock, Albert-Einstein-Str. 23-24, 18059, Rostock, Germany
| | - Ronald Redmer
- Institut für Physik, Universität Rostock, Albert-Einstein-Str. 23-24, 18059, Rostock, Germany
| | | | | | - Toshinori Yabuuchi
- RIKEN SPring-8 Center, Hyogo, 679-5148, Japan
- Japan Synchrotron Radiation Research Institute (JASRI), Hyogo, 679-5198, Japan
| | - Makina Yabashi
- RIKEN SPring-8 Center, Hyogo, 679-5148, Japan
- Japan Synchrotron Radiation Research Institute (JASRI), Hyogo, 679-5198, Japan
| | - Bratislav Lukic
- European Synchrotron Radiation Facility, 71 avenue des Martyrs, CS 40220, 38043, Grenoble, France
| | - Alexander Rack
- European Synchrotron Radiation Facility, 71 avenue des Martyrs, CS 40220, 38043, Grenoble, France
| | - Lisa M V Zinta
- Institut für Physik, Universität Rostock, Albert-Einstein-Str. 23-24, 18059, Rostock, Germany
| | - Tommaso Vinci
- LULI, CNRS, CEA, Ecole Polytechnique-Institut Polytechnique de Paris, Sorbonne Université, Palaiseau, 91128, France
| | - Alessandra Benuzzi-Mounaix
- LULI, CNRS, CEA, Ecole Polytechnique-Institut Polytechnique de Paris, Sorbonne Université, Palaiseau, 91128, France
| | - Alessandra Ravasio
- LULI, CNRS, CEA, Ecole Polytechnique-Institut Polytechnique de Paris, Sorbonne Université, Palaiseau, 91128, France
| | - Dominik Kraus
- Institut für Physik, Universität Rostock, Albert-Einstein-Str. 23-24, 18059, Rostock, Germany
- Helmholtz-Zentrum Dresden-Rossendorf, Institute of Radiation Physics, Dresden, 01328, Germany
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Shim SH, Ko B, Sokaras D, Nagler B, Lee HJ, Galtier E, Glenzer S, Granados E, Vinci T, Fiquet G, Dolinschi J, Tappan J, Kulka B, Mao WL, Morard G, Ravasio A, Gleason A, Alonso-Mori R. Ultrafast x-ray detection of low-spin iron in molten silicate under deep planetary interior conditions. SCIENCE ADVANCES 2023; 9:eadi6153. [PMID: 37862409 PMCID: PMC10588943 DOI: 10.1126/sciadv.adi6153] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/07/2023] [Accepted: 09/20/2023] [Indexed: 10/22/2023]
Abstract
The spin state of Fe can alter the key physical properties of silicate melts, affecting the early differentiation and the dynamic stability of the melts in the deep rocky planets. The low-spin state of Fe can increase the affinity of Fe for the melt over the solid phases and the electrical conductivity of melt at high pressures. However, the spin state of Fe has never been measured in dense silicate melts due to experimental challenges. We report detection of dominantly low-spin Fe in dynamically compressed olivine melt at 150 to 256 gigapascals and 3000 to 6000 kelvin using laser-driven shock wave compression combined with femtosecond x-ray diffraction and x-ray emission spectroscopy using an x-ray free electron laser. The observation of dominantly low-spin Fe supports gravitationally stable melt in the deep mantle and generation of a dynamo from the silicate melt portion of rocky planets.
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Affiliation(s)
- Sang-Heon Shim
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA
| | - Byeongkwan Ko
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA
| | - Dimosthenis Sokaras
- SLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA
| | - Bob Nagler
- SLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA
| | - He Ja Lee
- SLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA
| | - Eric Galtier
- SLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA
| | - Siegfried Glenzer
- SLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA
| | - Eduardo Granados
- SLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA
| | - Tommaso Vinci
- Laboratoire pour l’Utilisation des Lasers Intenses (LULI), Ecole Polytechnique, CNRS, CEA, UPMC, 91128 Palaiseau, France
| | - Guillaume Fiquet
- Sorbonne Université, Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, IMPMC, Museum National d’Histoire Naturelle, UMR CNRS 7590, 4 Place Jussieu, 75005 Paris, France
| | - Jonathan Dolinschi
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA
| | - Jackie Tappan
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA
| | - Britany Kulka
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ 85287, USA
| | - Wendy L. Mao
- SLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA
- Department of Earth and Planetary Sciences, Stanford University, Stanford CA 94305, USA
| | - Guillaume Morard
- Sorbonne Université, Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, IMPMC, Museum National d’Histoire Naturelle, UMR CNRS 7590, 4 Place Jussieu, 75005 Paris, France
- Université Grenoble Alpes, Universé Savoie Mont Blanc, CNRS, IRD, Université Gustave Eiffel, ISTerre, 38000 Grenoble, France
| | - Alessandra Ravasio
- Laboratoire pour l’Utilisation des Lasers Intenses (LULI), Ecole Polytechnique, CNRS, CEA, UPMC, 91128 Palaiseau, France
| | - Arianna Gleason
- SLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA
- Department of Earth and Planetary Sciences, Stanford University, Stanford CA 94305, USA
| | - Roberto Alonso-Mori
- SLAC National Accelerator Laboratory, 2575 Sand Hill Rd., Menlo Park, CA 94025, USA
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Mishra A, Kunka C, Echeverria MJ, Dingreville R, Dongare AM. Fingerprinting shock-induced deformations via diffraction. Sci Rep 2021; 11:9872. [PMID: 33972567 PMCID: PMC8111029 DOI: 10.1038/s41598-021-88908-y] [Citation(s) in RCA: 3] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/07/2021] [Accepted: 04/13/2021] [Indexed: 11/17/2022] Open
Abstract
During the various stages of shock loading, many transient modes of deformation can activate and deactivate to affect the final state of a material. In order to fundamentally understand and optimize a shock response, researchers seek the ability to probe these modes in real-time and measure the microstructural evolutions with nanoscale resolution. Neither post-mortem analysis on recovered samples nor continuum-based methods during shock testing meet both requirements. High-speed diffraction offers a solution, but the interpretation of diffractograms suffers numerous debates and uncertainties. By atomistically simulating the shock, X-ray diffraction, and electron diffraction of three representative BCC and FCC metallic systems, we systematically isolated the characteristic fingerprints of salient deformation modes, such as dislocation slip (stacking faults), deformation twinning, and phase transformation as observed in experimental diffractograms. This study demonstrates how to use simulated diffractograms to connect the contributions from concurrent deformation modes to the evolutions of both 1D line profiles and 2D patterns for diffractograms from single crystals. Harnessing these fingerprints alongside information on local pressures and plasticity contributions facilitate the interpretation of shock experiments with cutting-edge resolution in both space and time.
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Affiliation(s)
- Avanish Mishra
- Department of Materials Science and Engineering, University of Connecticut, Storrs, CT, 06269, USA.,Institute of Materials Science, University of Connecticut, Storrs, CT, 06269, USA
| | - Cody Kunka
- Center for Integrated Nanotechnologies, Sandia National Laboratories, Albuquerque, NM, 87123, USA
| | - Marco J Echeverria
- Department of Materials Science and Engineering, University of Connecticut, Storrs, CT, 06269, USA
| | - Rémi Dingreville
- Center for Integrated Nanotechnologies, Sandia National Laboratories, Albuquerque, NM, 87123, USA.
| | - Avinash M Dongare
- Department of Materials Science and Engineering, University of Connecticut, Storrs, CT, 06269, USA. .,Institute of Materials Science, University of Connecticut, Storrs, CT, 06269, USA.
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Fei Y, Seagle CT, Townsend JP, McCoy CA, Boujibar A, Driscoll P, Shulenburger L, Furnish MD. Melting and density of MgSiO 3 determined by shock compression of bridgmanite to 1254GPa. Nat Commun 2021; 12:876. [PMID: 33563984 PMCID: PMC7873221 DOI: 10.1038/s41467-021-21170-y] [Citation(s) in RCA: 12] [Impact Index Per Article: 4.0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/31/2020] [Accepted: 01/11/2021] [Indexed: 12/03/2022] Open
Abstract
The essential data for interior and thermal evolution models of the Earth and super-Earths are the density and melting of mantle silicate under extreme conditions. Here, we report an unprecedently high melting temperature of MgSiO3 at 500 GPa by direct shockwave loading of pre-synthesized dense MgSiO3 (bridgmanite) using the Z Pulsed Power Facility. We also present the first high-precision density data of crystalline MgSiO3 to 422 GPa and 7200 K and of silicate melt to 1254 GPa. The experimental density measurements support our density functional theory based molecular dynamics calculations, providing benchmarks for theoretical calculations under extreme conditions. The excellent agreement between experiment and theory provides a reliable reference density profile for super-Earth mantles. Furthermore, the observed upper bound of melting temperature, 9430 K at 500 GPa, provides a critical constraint on the accretion energy required to melt the mantle and the prospect of driving a dynamo in massive rocky planets.
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Affiliation(s)
- Yingwei Fei
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA.
| | | | | | - Chad A McCoy
- Sandia National Laboratories, Albuquerque, NM, USA
| | - Asmaa Boujibar
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA
| | - Peter Driscoll
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA
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