Now showing items 1-2 of 2

    • The Nuclear Reaction Network WinNet 

      Reichert, M.; Winteler, C.; Korobkin, O.; Arcones, A.; Bliss, J.; Eichler, M.; Frischknecht, U.; Fröhlich, C.; Hirschi, R.; Jacobi, M.; Kuske, J.; Martínez-Pinedo, G.; Martin, D.; Mocelj, D.; Rauscher, T.; Thielemann, F.-K. (2023-10-11)
      We present the state-of-the-art single-zone nuclear reaction network WinNet, which is capable of calculating the nucleosynthetic yields of a large variety of astrophysical environments and conditions. This ranges from the ...
    • Silicon carbide grains of type C provide evidence for the production of the unstable isotope Si in supernovae 

      Pignatari, M.; Zinner, E.; Bertolli, M.G.; Trappitsch, R.; Hoppe, P.; Rauscher, T.; Fryer, C.; Herwig, F.; Hirschi, R.; Timmes, F.X.; Thielemann, F.-K. (2013-07-01)
      Carbon-rich grains are observed to condense in the ejecta of recent core-collapse supernovae (SNe) within a year after the explosion. Silicon carbide grains of type X are C-rich grains with isotopic signatures of explosive ...