Browsing University of Hertfordshire by Author "Fischer, T."

Now showing items 1-3 of 3

    • Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase 

      Fischer, T.; Sagert, I.; Pagliara, G.; Hempel, M.; Schaffner-Bielich, J.; Rauscher, T.; Thielemann, Friedrich-Karl; Kaeppeli, R.; Martinez-Pinedo, G.; Liebendoerfer, M. (2011-06)
      We explore explosions of massive stars, which are triggered via the quark-hadron phase transition during the early post-bounce phase of core-collapse supernovae. We construct a quark equation of state, based on the bag ...

    • The r-, p-, and nu p-Process 

      Thielemann, Friedrich-Karl; Dillmann, I.; Farouqi, K.; Fischer, T.; Froehlich, C.; Kelic-Heil, A.; Korneev, I.; Kratz, K.L.; Langanke, K.; Liebendoerfer, M.; Panov, I. V.; Martinez-Pinedo, G.; Rauscher, T. (IOP Publishing Ltd., 2010)
      The processes discussed in this review are three of the four nucleosynthesis processes involved in producing heavy nuclei beyond Fe (not counting the rp-process in Xray bursts). Opposite to the fourth process (the s-process), ...

    • What are the astrophysical sites for the r-process and the production of heavy elements? 

      Thielemann, Friedrich-Karl; Arcones, A.; Kaeppeli, R.; Liebendoerfer, M.; Rauscher, T.; Winteler, C.; Froehlich, C.; Dillmann, I.; Fischer, T.; Martinez-Pinedo, G.; Langanke, K.; Farouqi, K.; Kratz, K. -L.; Panov, I.; Korneev, I. K. (2011-04)
      This article addresses three of the four nucleosynthesis processes involved in producing heavy nuclei beyond Fe (with a main focus on the r-process). Opposite to the fourth process (the s-process), which operates in stellar ...