Authors: Alberto Sesana, Jonathan Gair, Ilya Mandel, Alberto Vecchio
Date: 24 Mar 2009
Abstract: The properties of the first generation of black-hole seeds trace and distinguish different models of formation of cosmic structures in the high-redshift universe. The observational challenge lies in identifying black holes in the mass range ~100-1000 solar masses at redshift z~10. Here we show that future ground-based laser interferometers could observe gravitational waves produced by the coalescence of the first generation of light seed black-hole binaries and provide, possibly unique, information on the evolution of structures in this era. Using galaxy merger trees and four different models of black hole accretion we find that future detectors could study a few to a few tens of seed black-hole merger events in three years. We show further that a network of detectors will be able to measure the luminosity distance to typical sources to a precision of ~30%, allowing us to be confident of the high-redshift nature of the sources.
© M. Vallisneri 2012 — last modified on 2010/01/29
Tantum in modicis, quantum in maximis