The integrated three-point correlation function of cosmic shear
Autor: | Oliver Friedrich, Anik Halder, Stella Seitz, T. N. Varga |
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Rok vydání: | 2021 |
Předmět: |
Physics
010308 nuclear & particles physics Matter power spectrum Equation of state (cosmology) Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Correlation function (quantum field theory) 01 natural sciences Redshift Space and Planetary Science 0103 physical sciences Content (measure theory) Dark energy 010303 astronomy & astrophysics Bispectrum Weak gravitational lensing Mathematical physics |
Zdroj: | Monthly Notices of the Royal Astronomical Society. 506:2780-2803 |
ISSN: | 1365-2966 0035-8711 |
DOI: | 10.1093/mnras/stab1801 |
Popis: | We present the integrated 3-point shear correlation function $i\zeta_{\pm}$ -- a higher-order statistic of the cosmic shear field -- which can be directly estimated in wide-area weak lensing surveys without measuring the full 3-point shear correlation function, making this a practical and complementary tool to 2-point statistics for weak lensing cosmology. We define it as the 1-point aperture mass statistic $M_{\mathrm{ap}}$ measured at different locations on the shear field correlated with the corresponding local 2-point shear correlation function $\xi_{\pm}$. Building upon existing work on the integrated bispectrum of the weak lensing convergence field, we present a theoretical framework for computing the integrated 3-point function in real space for any projected field within the flat-sky approximation and apply it to cosmic shear. Using analytical formulae for the non-linear matter power spectrum and bispectrum, we model $i\zeta_{\pm}$ and validate it on N-body simulations within the uncertainties expected from the sixth year cosmic shear data of the Dark Energy Survey. We also explore the Fisher information content of $i\zeta_{\pm}$ and perform a joint analysis with $\xi_{\pm}$ for two tomographic source redshift bins with realistic shape-noise to analyse its power in constraining cosmological parameters. We find that the joint analysis of $\xi_{\pm}$ and $i\zeta_{\pm}$ has the potential to considerably improve parameter constraints from $\xi_{\pm}$ alone, and can be particularly useful in improving the figure of merit of the dynamical dark energy equation of state parameters from cosmic shear data. |
Databáze: | OpenAIRE |
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