SFB 1245
Atomic Nuclei: From Fundamental Interactions to Structure and Stars

B06: Nucleosynthesis in core-collapse supernovae

In project B06, we have made important advances in the investigation of critical microphysics aspects for supernova explosions and nucleosynthesis. We will use multi-dimensional supernova simulations to test the impact of new developments on the nuclear equation of state and neutrino-matter interactions. These microphysics inputs affect the neutron star evolution and thus the neutrino energies and luminosities that determine the nucleosynthesis. We will combine supernova simulations and state-of-the-art microphysics investigated in the CRC with nucleosynthesis calculations to gain new insights into supernova explosions and their contribution to the chemical history of the Universe.

Principal Investigators

  Name Working area(s) Contact
Prof. Dr. Almudena Arcones
B06, B07
+49 6151 16-21547
S2|11 105
Prof. Dr Gabriel Martinez-Pinedo
B01, B06
+49 6159 71 2750
GSI KBW 2.09