Generalized relativistic mean-field model with non-linear derivative nucleon-meson couplings for nuclear matter and finite nuclei

Sofija Antic
The equation of state (EOS) for highly compressed dense matter is one of the main concerns of nuclear astrophysics in recent years. It is essential for modeling compact astrophysical objects like neutron stars (NS), their mergers and core-collapse supernovae (CCSN). It also sets the conditions for the creation of chemical elements in the universe, in particular for the r-process whose astrophysical site is still under debate. Therefore, it is an active theoretical and experimental research...
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