PIRSA:11060027

Video URL

https://pirsa.org/11060027

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

Arcones, A. (2011). Nucleosynthesis of Heavy Elements in Neutrino-Driven Winds and Neutron-Star Mergers. Perimeter Institute for Theoretical Physics. https://pirsa.org/11060027

Arcones, Almudena. Nucleosynthesis of Heavy Elements in Neutrino-Driven Winds and Neutron-Star Mergers. Perimeter Institute for Theoretical Physics, Jun. 22, 2011, https://pirsa.org/11060027 

          @misc{ scivideos_PIRSA:11060027,
            doi = {10.48660/11060027},
            url = {https://pirsa.org/11060027},
            author = {Arcones, Almudena},
            keywords = {Particle Physics},
            language = {en},
            title = {Nucleosynthesis of Heavy Elements in Neutrino-Driven Winds and Neutron-Star Mergers},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2011},
            month = {jun},
            note = {PIRSA:11060027 see, \url{https://scivideos.org/index.php/pirsa/11060027}}
          }

Almudena Arcones Universität Basel

Talk numberPIRSA:11060027
DOI10.48660/11060027
Source RepositoryPIRSA
Collection
Talk Type Conference
Subject

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.