Diffuse scattering from dynamically compressed single-crystal zirconium following the pressure-induced alpha-to-omega phase transition

Physical Review B: Condensed Matter and Materials Physics American Physical Society

Authors:

Patrick Heighway, Saransh Singh, Martin Gorman, David McGonegle, Jon Eggert, Ray Smith

Abstract:

The prototypical α → ω phase transition in zirconium is an ideal test-bed for our understanding of polymorphism under extreme loading conditions. After half a century of study, a consensus had emerged that the transition is realized via one of two distinct displacive mechanisms, depending on the nature of the compression path. However, recent dynamic-compression experiments equipped with in situ diffraction diagnostics performed in the past few years have revealed new transition mechanisms, demonstrating that our understanding of the underlying atomistic dynamics and transition kinetics is in fact far from complete. We present classical molecular dynamics simulations of the α → ω phase transition in single-crystal zirconium shock-compressed along the [0001] axis using a machine-learning-class potential. The transition is predicted to proceed primarily via a modified version of the two-stage Usikov-Zilberstein mechanism, whereby the high-pressure ω-phase heterogeneously nucleates at boundaries between grains of an intermediate β-phase. We further observe the fomentation of atomistic disorder at the junctions between β grains, leading to the formation of highly defective interstitial material between the ω grains. We directly compare synthetic x-ray diffraction patterns generated from our simulations with those obtained using femtosecond diffraction in recent dynamic-compression experiments, and show that the simulations produce the same unique, anisotropic diffuse scattering signal unlike any previously seen from an elemental metal. Our simulations suggest that the diffuse signal arises from a combination of thermal diffuse scattering, nanoparticle-like scattering from residual kinetically stabilized α and β grains, and scattering from interstitial defective structures.

Driving Iron plasmas to stellar core conditions using extreme x-ray radiation

Authors:

Hae Ja Lee, Sam Vinko, Oliver Humphries, Eric Galtier, Ryan Royle, Muhammad Kasim, Shenyuan Ren, Roberto Alonso-Mori, Phillip Heimann, Mengning Liang, Matt Seaberg, Sébastien Boutet, Andrew A Aquila, Shaughnessy Brown, Akel Hashim, Mikako Makita, Christian David, Gediminas Seniutinas, Hyun-Kyung Chung, Gilliss Dyer, Justin Wark, Bob Nagler

Dynamical development of strength and stability of asteroid material under 440 GeV proton beam irradiation

Nature Communications Nature Research (part of Springer Nature)

Authors:

M Bochmann, K-G Schlesinger, C Arrowsmith, P Alexaki, M Alfonso Poza, M Ambarki, E Andersen, P Bilbao, R Bingham, F Cruz, A Ebn Rahmoun, A Goillot, J Halliday, Bt Huffman, E Kamenicka, M Lazzaroni, E Los, Jm Quetsch, B Reville, P Rousiadou, S Sarkar, L Silva, P Simon, E Soria, V Stergiou, S Zhang, N Charitonidis, Gianluca Gregori

Dynamical development of strength and stability of asteroid material under 440 GeV proton beam irradiation

Authors:

Melanie Bochmann, Karl-Georg Schlesinger, Charles Arrowsmith, Paraskevi Alexaki, Marta Alfonso Poza, Mohamed Ambarki, Emily Andersen, Pablo Bilbao, Robert Bingham, Filipe Cruz, Aboubakr Ebn Rahmoun, Alice Goillot, Jonathan Halliday, Brian Huffman, Eva Kamenicka, Michael Lazzaroni, Eva Los, Jean-Marc Quetsch, Brian Reville, Panagiota Rousiadou, Subir Sarkar, Luis Silva, Pascal Simon, Enrica Soria, Vasiliki Stergiou, Sifei Zhang, Nikolaos Charitonidis, Gianluca Gregori

Enabling the Realisation of Proton Tomography

Authors:

Ben T Spiers, Ramy Aboushelbaya, Qingsong Feng, Marko W Mayr, Iustin Ouatu, Robert W Paddock, Robin Timmis, Robin HW Wang, Peter A Norreys