Cosmology and modified GW propagation from the BNS mass function at third-generation detector networks
Dounia Nanadoumgar-Lacroze, Niccol\`o Muttoni, Michele Maggiore, Michele Mancarella

TL;DR
This paper forecasts how third-generation gravitational wave detectors can constrain the Hubble constant and modified gravity parameters using binary neutron star observations, highlighting the potential for high-precision cosmology.
Contribution
It introduces a comprehensive Bayesian inference framework for joint cosmology and population analysis with third-generation GW detectors, assessing their capabilities to measure H_0 and modified gravity parameters.
Findings
ET alone constrains H_0 to 11-12% and Xi_0 to 18%.
ET+CE network improves constraints to 6% on Xi_0 and 9% on H_0.
High SNR selection yields conservative but promising precision estimates.
Abstract
We perform forecasts for the Hubble parameter H_0 and for the parameter Xi_0 that describes modified gravitational-wave propagation, using information from the binary neutron star (BNS) mass function, for Einstein Telescope (ET), taken either in the triangle or in the ``2L'' configuration, as well as for detector network made by ET together with a 40-km Cosmic Explorer (CE). We restrict ourselves to BNSs with a large signal-to-noise ratio, SNR>50, which still give O(10^3) events yr-1, and we perform a full joint cosmology-population Bayesian inference. We find that, for ET in isolation, the two ET configurations perform comparably, yielding uncertainties of 12% and 11% on H_0 for the triangular and 2L designs, respectively, and 18% uncertainty on Xi_0 in both cases. For networks including ET and CE, we can constrain H_0 and Xi_0 to precisions of 9% and 6%, respectively. These results…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Cosmology and Gravitation Theories · Particle physics theoretical and experimental studies
