Relatore
Dr.
Alessandro Nagar
(INFN sezione di Torino, Centro Fermi and IHES)
Descrizione
I will review the status of TEOBResumS, that is a state of the art effective-one-body based waveform model for spin-aligned coalescing compact binaries, e.g. black hole binaries and neutron star binaries. I will focus on the impact of the numerical relativity information needed to complete the analytical model and focus on the performance of the model for gravitational wave data-analytsis purposes.
Autore principale
Dr.
Alessandro Nagar
(INFN sezione di Torino, Centro Fermi and IHES)
