| Literature DB >> 31574771 |
G Rigon, A Casner1, B Albertazzi, Th Michel, P Mabey, E Falize2, J Ballet3, L Van Box Som2, S Pikuz4,5, Y Sakawa6, T Sano6, A Faenov4,7, T Pikuz4,7, N Ozaki6,8, Y Kuramitsu8, M P Valdivia9, P Tzeferacos10, D Lamb10, M Koenig8.
Abstract
We describe a platform developed on the LULI2000 laser facility to investigate the evolution of Rayleigh-Taylor instability (RTI) in scaled conditions relevant to young supernova remnants (SNRs) up to 200 years. An RT unstable interface is imaged with a short-pulse laser-driven (PICO2000) x-ray source, providing an unprecedented simultaneous high spatial (24μm) and temporal (10 ps) resolution. This experiment provides relevant data to compare with astrophysical codes, as observational data on the development of RTI at the early stage of the SNR expansion are missing. A comparison is also performed with FLASH radiative magnetohydrodynamic simulations.Entities:
Year: 2019 PMID： 31574771 DOI： 10.1103/PhysRevE.100.021201
Source DB: PubMed Journal: Phys Rev E ISSN： 2470-0045 Impact factor: 2.529