Edwin Genoud-Prachex

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.

A joint hierarchical Bayesian analysis of the binary black hole (BBH) mass function, merger rate evolution, and cosmological parameters can be used to extract information on both the cosmological and population parameters. We extend this technique to include the effect of modified gravitational wave (GW) propagation. We discuss the constraints on the parameter ${\mathrm{\Xi }}_0$ that describe this phenomenon [with ${\mathrm{\Xi }}_0=1$ in general relativity (GR)] using the data from the third gravitational wave transient catalog. We find the constraints ${\mathrm{\Xi }}_0=1.2_{-0.7}^{+0.7}$ with a flat prior on ${\mathrm{\Xi }}_0$, and ${\mathrm{\Xi }}_0=1.0_{-0.8}^{+0.4}$ with a prior uniform in $\log {\mathrm{\Xi }}_0$ (68% C.L., maximum posterior and highest-density interval), which only rely on the presence of a feature in the BBH mass distribution around $\sim 30–45M_{\odot }$ and are robust to whether or not the event GW190521 is considered an outlier of the population. We then study in more detail the effects of modified GW propagation on population and cosmological analyses for LIGO/Virgo at design sensitivity. We find that, for a given data-taking period, the relative error $\mathrm{\Delta }{\mathrm{\Xi }}_0/{\mathrm{\Xi }}_0$ has a significant dependence on the fiducial value of ${\mathrm{\Xi }}_0$, since the latter has a strong influence on the detection rate. For five years of data, the accuracy ranges from $\sim 10\%$ on ${\mathrm{\Xi }}_0$ when ${\mathrm{\Xi }}_0=1$ to $\mathrm{\Delta }{\mathrm{\Xi }}_0/{\mathrm{\Xi }}_0\sim 20\%$ for ${\mathrm{\Xi }}_0=1.8$, which represents a large deviation from GR, still consistent with current limits and predicted by viable cosmological models. For the Hubble parameter, we forecast an accuracy of $\mathrm{\Delta }{H}_0/H_0\sim 20\%$ and an accuracy on $H(z)$ of $\sim 7\%$ at a pivot redshift $z_{*}\sim 0.8$; this updates the results found in previous studies, by making use of a population model compatible with current observations, and is about a factor 2 worse, in twice the observing time. We finally show that, if nature is described by a modified gravity theory with a large deviation from the GR value ${\mathrm{\Xi }}_0=1$, such as ${\mathrm{\Xi }}_0=1.8$, analyzing the data assuming GR produces a significant bias in the inferred values of the mass scales, Hubble constant, and particularly the BBH merger rate.

A joint hierarchical Bayesian analysis of the binary black hole (BBH) mass function, merger rate evolution and cosmological parameters can be used to extract information on both the cosmological and population parameters. We extend this technique to include the effect of modified gravitational wave (GW) propagation. We discuss the constraints on the parameter $\Xi_0$ that describes this phenomenon (with $\Xi_0=1$ in General Relativity, GR) using the data from the GWTC-3 catalog. We find the constraints $\Xi_0 = 1.2^{+0.7}_{-0.7}$ with a flat prior on $\Xi_0$, and $\Xi_0 = 1.0^{+0.4}_{-0.8}$ with a prior uniform in $\log\Xi_0$ ($68\%$ C.L., maximum posterior and HDI), which only rely on the presence of a feature in the BBH mass distribution around $\sim 30-45 M_{\odot}$, and are robust to whether or not the event GW190521 is considered an outlier of the population. We then study in more detail the effects of modified GW propagation on population and cosmological analyses for LIGO/Virgo at design sensitivity. For a given data-taking period, the relative error $\Delta\Xi_0/\Xi_0$ has a significant dependence on the fiducial value of $\Xi_0$, since the latter has a strong influence on the detection rate. For five years of data, the accuracy ranges from $\sim 10\%$ on $\Xi_0$ when $\Xi_0=1$ to $\Delta\Xi_0/\Xi_0\sim 20\%$ for $\Xi_0=1.8$ - a large deviation from GR, still consistent with current limits and predicted by viable cosmological models. For the Hubble parameter, we forecast an accuracy of $\Delta H_0/H_0 \sim 20\%$, and an accuracy on $H(z)$ of $\sim7\%$ at a pivot redshift $z_*\sim 0.8$. We finally show that, if Nature is described by a modified gravity theory with a large deviation from the GR value $\Xi_0=1$, such as $\Xi_0=1.8$, analysing the data assuming GR produces a significant bias in the inferred values of the mass scales, Hubble constant, and BBH merger rate.