Constraining the mass of the graviton using coalescing black-hole binaries
Constraining the mass of the graviton using coalescing black-hole binaries
We study how well the mass of the graviton can be constrained from gravitational-wave (GW) observations of coalescing binary black holes. Whereas the previous investigations employed post-Newtonian (PN) templates describing only the inspiral part of the signal, the recent progress in analytical and numerical relativity has provided analytical waveform templates …