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: Hâ‚€ = 67.4 ± 0.5 km/s/Mpc
  • SH0ES (Cepheids): Hâ‚€ = 73.0 ± 1.0 km/s/Mpc
  • GW170817: Hâ‚€ = 70 ± 12 km/s/Mpc
  • Future: 50+ events → σ(Hâ‚€) ~ 2%