Conveners
Session XI
- Juan Calderon Bustillo (University of Santiago de Compostela)
The yet-to-be-detected gravitational wave signal from core-collapse supernovae is expected to be dominated by oscillation modes of the newly born proto-neutron star (PNS). I am going to present a new general relativistic framework for computing the oscillation modes of a PNS, including, for the first time, an accretion flow and a surrounding stalled accretion shock. The oscillations can be...
The accurate modelling of neutron star oscillations is essential as we prepare for the next generation of gravitational-wave detectors, which will be able to probe the rich astrophysical content of post-merger signals. In this talk, I will present recent updates to ROXAS, a spectral code to numerically simulate the dynamical evolution of perturbed rotating neutron stars. ROXAS uses a...
