Cosmological constraints from gas mass fractions of massive, relaxed galaxy clusters. Issue 1 (26th November 2021)

• Record Type: Journal Article
• Authors: Mantz, Adam B; Morris, R Glenn; Allen, Steven W; Canning, Rebecca E A; Baumont, Lucie; Benson, Bradford; Bleem, Lindsey E; Ehlert, Steven R; Floyd, Benjamin; Herbonnet, Ricardo; Kelly, Patrick L; Liang, Shuang; von der Linden, Anja; McDonald, Michael; Rapetti, David A; Schmidt, Robert W; Werner, Norbert; Wright, Adam
• Is Part Of: Monthly notices of the Royal Astronomical Society. Volume 510:Issue 1(2022)
• Page Start: 131
• Page End: 145
• Publication Date: 2021-11-26
• Subjects: cosmological parameters -- cosmology: observations -- dark matter -- distance scale -- galaxies: clusters: general -- X-rays: galaxies: clusters; Astronomy -- Periodicals; Periodicals; 520.5
• DOI: 10.1093/mnras/stab3390
• Languages: English
• ISSNs: 0035-8711

Abstract

ABSTRACT: We present updated cosmological constraints from measurements of the gas mass fractions ( f gas ) of massive, dynamically relaxed galaxy clusters. Our new data set has greater leverage on models of dark energy, thanks to the addition of the Perseus cluster at low redshifts, two new clusters at redshifts z ≳ 1, and significantly longer observations of four clusters at 0.6 < z < 0.9. Our low-redshift ( z < 0.16) f gas data, combined with the cosmic baryon fraction measured from the cosmic microwave background (CMB), imply a Hubble constant of h = 0.722 ± 0.067. Combining the full f gas data set with priors on the cosmic baryon density and the Hubble constant, we constrain the dark energy density to be ΩΛ = 0.865 ± 0.119 in non-flat Lambda cold dark matter (cosmological constant) models, and its equation of state to be $w=-1.13_{-0.20}^{+0.17}$ in flat, constant- w models, respectively 41 per cent and 29 per cent tighter than our previous work, and comparable to the best constraints available from other probes. Combining f gas, CMB, supernova, and baryon acoustic oscillation data, we also constrain models with global curvature and evolving dark energy. For the massive, relaxed clusters employed here, we find the scaling of f gas with mass to be consistent with a constant, with an intrinsic scatter that corresponds to just ∼3 per cent in distance.