Speaker
Krishnendu Naderi Varium
(University of Birmingham)
Description
Quantify the capabilities of third-generation gravitational wave detector network to probe the properties of first star remnants, population III remnants, in the Universe. Simulating the sources from astrophysically motivated pop III remnant binary black holes and performing full Bayesian inference using \texttt{IMRPHenomXPHM} waveform model, we estimate the accuracy at which the redshift is measured. Compare the performance of the detector network performances with $f_{\rm{low}}=5\rm{Hz}$ and $f_{\rm{low}}=10\rm{Hz}$.
Author
Krishnendu Naderi Varium
(University of Birmingham)
Co-authors
Prof.
Alberto Vecchio
(University of Birmingham)
Prof.
Geraint Pratten
(University of Birmingham)
Prof.
Patricia Schmidt
(University of Birmingham)