Relatore
Michal Stanislaw Bejger
(Istituto Nazionale di Fisica Nucleare)
Descrizione
Gravitational wave events involving neutron stars provide interesting information of their interiors. In this talk I will not focus on the compact binary inspirals (GW170817-type events), related to the measurements of the tidal deformability of the components, but present instead other types of observations expected in the future: r-modes from rotating neutron stars, as well as the signals related to post-merger emission.
Autore principale
Michal Stanislaw Bejger
(Istituto Nazionale di Fisica Nucleare)
