Inferred Hâ‚€ from GW Data
About Standard Sirens
Gravitational wave (GW) detections from binary mergers provide "standard sirens" - direct distance measurements from the GW strain amplitude without needing a cosmic distance ladder.
The GW strain amplitude h ~ Mchirp/DL, where Mchirp is the chirp mass (determined from the frequency evolution) and DL is the luminosity distance. Combined with redshift z from an EM counterpart (like GW170817's kilonova), this directly measures Hâ‚€.
At low redshift: H₀ ≈ cz/DL. With many detections, statistical uncertainties shrink as 1/√N, providing an independent probe of the Hubble tension.
Reference Values
- Planck CMB: H₀ = 67.4 ± 0.5 km/s/Mpc
- SH0ES (Cepheids): H₀ = 73.0 ± 1.0 km/s/Mpc
- GW170817: H₀ = 70 ± 12 km/s/Mpc
- Future: 50+ events → σ(H₀) ~ 2%