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Recent experiments on in-situ high-energy self-ion irradiation of tungsten (W) show the occurrence of unusual cascade damage effects resulting from single ion impacts, shedding light on the nature of radiation damage expected in the…

Materials Science · Physics 2014-05-02 A. E. Sand , S. L. Dudarev , K. Nordlund

The impact of nanoparticles (NPs) comprised of atoms with covalent bonding is investigated numerically and theoretically. We use recent models of covalent bonding of carbon atoms and elaborate a numerical model of amorphous carbon (a-C)…

Mesoscale and Nanoscale Physics · Physics 2022-02-01 Alexey A. Tsukanov , Nikolai V. Brilliantov

Superconductor based quantum computing has the major drawback of working temperatures which require liquid helium for cooling. A promising approach to overcome this obstacle for quantum technologies is based on deep level defects in…

Materials Science · Physics 2019-06-19 Michael Schöler , Maximilian W. Lederer , Philipp Schuh , Peter J. Wellmann

Shear stresses are the driving forces for the creation of both point and extended defects in crystals subjected to high pressures and temperatures. Recently, we observed anomalous elastic materials response in shock-compressed silicon and…

Materials Science · Physics 2009-11-11 I. I. Oleynik , S. V. Zybin , M. L. Elert , C. T. White

We implement a multi-group and discrete-ordinate neutrino transport model in spherical symmetry which allows to simulate collective neutrino oscillations by including realistic collisional rates in a self-consistent way. We utilize this…

High Energy Astrophysical Phenomena · Physics 2023-04-13 Zewei Xiong , Meng-Ru Wu , Gabriel Martínez-Pinedo , Tobias Fischer , Manu George , Chun-Yu Lin , Lucas Johns

Single-phase, multi-elements (three or more) with high concentrations show exceptional tensile strength up to ~ 0.8-1.2 GPa. However, they possess a very low 0.2% yield strength (YS), i.e., they can be permanently deformed at very…

We investigate the hydrodynamics of the interaction of two supersonic winds in binary systems. The collision of the winds creates two shocks separated by a contact discontinuity. The overall structure depends on the momentum flux ratio eta…

Solar and Stellar Astrophysics · Physics 2015-05-30 Astrid Lamberts , Sebastien Fromang , Guillaume Dubus

The relevance of the standing accretion shock instability (SASI) compared to neutrino-driven convection in three-dimensional (3D) supernova-core environments is still highly controversial. Studying a 27 Msun progenitor, we demonstrate, for…

Solar and Stellar Astrophysics · Physics 2015-06-15 F. Hanke , B. Mueller , A. Wongwathanarat , A. Marek , H. -Th. Janka

Formation of the complex structure with 16 atoms in the orthorhombic cell, space group Cmca (Pearson symbol oC16) was experimentally found under high pressure in the alkali elements (K, Rb, Cs) and polyvalent elements of groups IV (Si, Ge)…

Materials Science · Physics 2013-05-24 Valentina F. Degtyareva

The role of phase separation in the emergence of superconductivity in alkali metal doped iron selenides A$_{x}$Fe$_{2-y}$Se$_{2}$ (A = K, Rb, Cs) is revisited. High energy X-ray diffraction and Monte Carlo simulation were used to…

Superconductivity · Physics 2018-05-23 Chunruo Duan , Junjie Yang , Yang Ren , Despina Louca

Aluminum alloys, the most widely utilized lightweight structural materials, predominantly depend on coherent complex-structured nano-plates to enhance their mechanical properties. Despite several decades of research, the atomic-scale…

Materials Science · Physics 2024-10-22 Junyuan Bai , Gaowu Qin , Xueyong Pang , Zhihao Zhao

Core-collapse supernovae produce elements between Fe and Ag depending on the properties of the ejected matter. Despite the fast progress in supernova simulations in the last decades, there are still uncertainties in the astrophysical…

High Energy Astrophysical Phenomena · Physics 2018-04-04 Julia Bliss , Maximilian Witt , Almudena Arcones , Fernando Montes , Jorge Pereira

We carry out direct numerical simulations of turbulent astrophysical media that explicitly track ionizations, recombinations, and species-by-species radiative cooling. The simulations assume solar composition and follows the evolution of…

Astrophysics of Galaxies · Physics 2015-06-23 William J Gray , Evan Scannapieco , Daniel Kasen

Radiation creep and swelling are irreversible deformation phenomena occurring in materials irradiated even at low temperatures. On the microscopic scale, energetic particles initiate collision cascades, generating and eliminating defects…

Materials Science · Physics 2024-09-23 Luca Reali , Max Boleininger , Daniel R. Mason , Sergei L. Dudarev

We study the phase behaviour of the Al$_x$CrFeCoNi high-entropy alloy. Our approach is based on a perturbative analysis of the internal energy of the paramagnetic solid solution as evaluated within the Korringa-Kohn-Rostoker formulation of…

Materials Science · Physics 2024-12-02 Christopher D. Woodgate , George A. Marchant , Livia B. Pártay , Julie B. Staunton

Ni/Al reactive multilayers are promising materials for applications requiring controlled local energy release and superior mechanical performance. This study systematically investigates the impact of compositional variations, ranging from…

Materials Science · Physics 2026-04-14 Nensi Toncich , Fabian Schwarz , Rebecca A. Gallivan , Jemma Gillon , Ralph Spolenak

It is widely thought that core-collapse supernovae (CCSNe), the explosions of massive stars following the collapse of the stars' iron cores, is obtained due to energy deposition by neutrinos. So far, this scenario was not demonstrated from…

High Energy Astrophysical Phenomena · Physics 2015-02-12 Doron Kushnir

The interactions between chemical phase fields and structural defects play a key role in the properties of alloys. We illustrate the importance of these interactions in driven alloys, where defects are continuously being created, with…

Materials Science · Physics 2026-02-16 Amit Verma , Yen-Ting Chang , Marie Charpagne , Pascal Bellon , Robert S. Averback

Energetic atom collisions in solids induce shockwaves with complex morphologies. In this paper, we establish the existence of a morphological transition in such cascades. The order parameter of the morphology is defined as the exponent,…

Details of the core-collapse supernova (CCSN) explosion mechanism still need to be fully understood. There is an increasing number of successful examples of reproducing explosions in multidimensional hydrodynamic simulations, but subsequent…

High Energy Astrophysical Phenomena · Physics 2023-01-11 Ryo Sawada , Yudai Suwa