Abstract Type Ia supernovae (SNe) are believed to be caused by the thermonuclear
explosion of a white dwarf (WD), but the nature of the progenitor system (s) is still unclear …

We carry out a systematic study of the response of companion stars in massive binaries after
being impacted by supernova (SN) ejecta. A total of 720 1D stellar evolution calculations are …

We report on the design and first results from experiments looking at the formation of
radiative shocks on the Shenguang-II (SG-II) laser at the Shanghai Institute of Optics and …

We report new experimental results on radiative shocks obtained in Xenon and Argon in gas
cells at two different pressures below 1bar. These shock waves are generated by the …

In this paper we present the modelling work currently performed at the Instituto de Fusión
Nuclear “Guillermo Velarde”(Universidad Politécnica de Madrid) in the field of plasma …

In this article, we will show recent hydrodynamic simulations of quasi-steady state (QSS)
plasma-based amplifiers of soft X-rays. These simulations are being performed with the 2D …

La investigación en la fusión nuclear por confinamiento inercial (FCI) sigue sin pausa, con
sus avatares, su desarrollo en diversos laboratorios en el mundo en ocasiones muy …