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2016

Determining the progenitors of merging black-hole binaries

Raccanelli, Alvise, Kovetz, Ely D., Bird, Simeon et al.

Understand

We investigate a possible method for determining the progenitors of black hole (BH) mergers observed via their gravitational wave (GW) signal.

We argue that measurements of the cross-correlation of the GW events with overlapping galaxy catalogs may provide an additional tool in determining if BH mergers trace the stellar mass of the Universe, as would be expected from mergers of the endpoints of stellar evolution.
If on the other hand the BHs are of primordial origin, as has been recently suggested, their merging would be preferentially hosted by lower biased objects, and thus have a lower cross-correlation with luminous galaxies.
Here we forecast the expected precision of the cross-correlation measurement for current and future GW detectors such as LIGO and the Einstein Telescope.