Sprecher
Prof.
Friedrich Thielemann
(University of Basel)
Beschreibung
We give a short review on necessary conditions in order to achieve a sufficient neutron/seed ratio for an r-process to occur, what are the candidate astrophysical sites to fulfill such conditions (supernovae, magnetar-forming supernovae, quark (super-)novae, neutron star mergers,...), what is their role in the chemical evolution of galaxies, and whether there existed a chance to produce superheavy elements in nature.
Autor
Prof.
Friedrich Thielemann
(University of Basel)
