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Cosmology and modified gravity with dark sirens from GWTC-3
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abstract
We present the latest measurements of the Hubble parameter and of the parameter $\Xi_0$ describing modified gravitational wave propagation, obtained from the third gravitational wave transient catalog, GWTC-3, using the correlation with galaxy catalogs and information from the source-frame mass distribution of binary black holes. The latter leads to the tightest bound on $\Xi_0$ so far, i.e. $\Xi_0 = 1.2^{+0.7}_{-0.7}$ with a flat prior on $\Xi_0$, and $\Xi_0 = 1.0^{+0.4}_{-0.8}$ with a prior uniform in $\log\Xi_0$ (Max posterior and $68\%$ HDI). The measurement of $H_0$ is dominated by the single bright siren GW170817, resulting in $H_0=67^{+9}_{-6} \, \rm km \, s^{-1} \, Mpc$ when combined with the galaxy catalog.
Forward citations
Cited by 2 Pith papers
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A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events
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Dynamical Barbero--Immirzi field coupled to quintessence: gravitational-wave propagation constraints and next-generation forecasts
A model coupling the Barbero-Immirzi field to quintessence adds a second redshift-dependent term to gravitational-wave propagation, yielding bounds xi_BI<0.7 and xi_coup<0.13 from GWTC-3 data.
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