When performing parameter estimation for gravitational-wave (GW) data, Bayesian techniques provide a powerful framework to describe said parameters. These techniques are consistent with both our prior [...]
Gravitational wave radiation is only unambiguously defined at future null infinity - the location in spacetime where light rays arrive and where global properties of [...]
Doctoranda: Luana Michela Modafferi Títol: Searching for long-duration transient gravitational waves from spinning neutron stars. Directors: Dr. David Benjamin Keitel i Dra. Alicia Magdalena Sintes Olives Programa [...]
Accurate modeling of neutrino transport plays a crucial role in understanding astrophysical phenomena such as core-collapse supernovae and neutron star mergers. This talk will review [...]