Orateur
Sofia Bisero
(GEPI, Observatoire de Paris, Université PSL, CNRS)
Description
I will discuss the key ingredients required to model the multi-messenger emission from binary neutron star mergers, from gravitational waves to electromagnetic radiation, highlighting the main degeneracies and open questions. I will then move from individual events to populations, describing how synthetic populations can be constructed, from astrophysical assumptions to observational predictions.