Place and time: New Bulgarian University, 07.06.2019 /Friday/, 11:20, Hall 607 II
Abstract: The high density of nuclei in the cores of massive stars during a supernova explosion leads to enhanced rates of different reactions in this region. In this lecture we recall several well-known important case in which the nucleon correlations beyond the mean-field approximation are important as well as several yet unexplored cases.
Biosketch.
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