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ABSTRACT Using redshift space distortion data, we perform model-independent reconstructions of the growth history of matter inhomogeneity in the expanding Universe using two methods: crossing statistics and Gaussian processes. We then reconstruct the corresponding history of the Universe background expansion and fit it to Type Ia supernovae data, putting constraints on (Ωm, 0, σ8, 0). The results obtained are consistent with the concordance flat-ΛCDM model and General Relativity as the gravity theory given the current quality of the inhomogeneity growth data.
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Benjamin L’Huillier
Korea Institute for Advanced Study
Arman Shafieloo
Korea Astronomy and Space Science Institute
David Polarski
Centre National de la Recherche Scientifique
Monthly Notices of the Royal Astronomical Society
Centre National de la Recherche Scientifique
Yonsei University
Université de Montpellier
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L’Huillier et al. (Fri,) studied this question.
synapsesocial.com/papers/6a0fafe54fb650da4ffe655a — DOI: https://doi.org/10.1093/mnras/staa633