Nov 20

Modelling of early stage kilonova ejecta opacity in the multi-messenger era: the selenium case

Giovedì 27 novembre alle ore 14:00, il Dott. Matteo Bezmalinovich (INAF – Osservatorio Astronomico d’Abruzzo, IT) terrà il seminario dal titolo “Modelling of early-stage kilonova ejecta opacity in the multi-messenger era: the selenium case”. Abstract: In the multi-messenger era, kilonovae (KNe) represent key sites of rapid (r-) neutron capture process nucleosynthesis. KNe are quasi-thermal electromagnetic […]

Set 12

Kilonova modelling: from r-process yields in binary neutron star mergers to population studies

Giovedì 18 settembre aprile alle ore 15:00, la Dott.ssa Eleonora Loffredo, dell’INAF-Osservatorio Astronomico d’Abruzzo, terrà il seminario dal titolo “Kilonova modelling: from r-process yields in binary neutron star mergers to population studies”. Abstract: Binary neutron star (BNS) mergers eject neutron-rich matter, providing ideal conditions for the nucleosynthesis of heavy elements via the r-process. The radioactive […]