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Nucleosynthesis of Heavy Elements in Neutrino-Driven Winds and Neutron-Star Mergers



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PIRSA Number: 
11060027

Abstract

The energy generated by the r-process can impact the dynamics of neutron star mergers. Solving a full r-process network coupled with the hydrodynamics becomes the necessary but it is computational very expensive. We have developed a simple model that can be implemented into hydrodynamic simulations and gives a very good estimate of the r-process heating.