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• W4367319044 abstract "We explore a reparametrization of the lensing amplitude tension between weak lensing (WL) and cosmic microwave background (CMB) data and its implications for a joint resolution with the Hubble tension. Specifically, we focus on the lensing amplitude over a scale of 12 Mpc in absolute distance units using a derived parameter ${S}_{12}$ and show its constraints from recent surveys in comparison with Planck 2018. In WL alone, we find that the absolute distance convention correlates ${S}_{12}$ with ${H}_{0}$. Accounting for this correlation in the 3D space ${S}_{12}ifmmodetimeselsetexttimesfi{}{ensuremath{omega}}_{m}ifmmodetimeselsetexttimesfi{}h$ reproduces the usual levels of $2ensuremath{sim}3ensuremath{sigma}$ tension inferred from ${S}_{8}ifmmodetimeselsetexttimesfi{}{mathrm{ensuremath{Omega}}}_{m}$. Additionally, we derive scaling relations in the ${S}_{8}ifmmodetimeselsetexttimesfi{}h$ and ${S}_{12}ifmmodetimeselsetexttimesfi{}h$ planes that are allowed by $mathrm{ensuremath{Lambda}}mathrm{CDM}$ and extrapolate target scalings needed to solve the ${H}_{0}$ and lensing-amplitude tensions jointly in a hypothetical beyond-$mathrm{ensuremath{Lambda}}mathrm{CDM}$ model. As a test example, we quantify how the early dark energy scenario compares with these target scalings. Useful fitting formulas for ${S}_{8}$ and ${S}_{12}$ as a function of other cosmological parameters in $mathrm{ensuremath{Lambda}}mathrm{CDM}$ are provided, with 1% precision." @default.
• W4367319044 created "2023-04-29" @default.
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• W4367319044 date "2023-04-28" @default.
• W4367319044 modified "2023-10-17" @default.
• W4367319044 title "Role of the Hubble scale in the weak lensing versus CMB tension" @default.
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• W4367319044 doi "https://doi.org/10.1103/physrevd.107.083532" @default.
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