(A13) using the 3 + 1 formalism and linear perturbation theory for matter density fluctuations

Derivation of the effective curvatureδK D In this subsection, we derive the effective curvatureδK D in Eq

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astro-ph.CO · 2026-04-07 · unverdicted · novelty 5.0

An eight top-hat shell model of large-scale inhomogeneity reconciles the Hubble parameters measured by DESI DR2 BAO and Pantheon+ supernovae.

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Reconstructing a large-scale matter-density contrast profile to reconcile Pantheon+ supernovae with DESI DR2 BAO in an inhomogeneous universe astro-ph.CO · 2026-04-07 · unverdicted · none · ref 3
An eight top-hat shell model of large-scale inhomogeneity reconciles the Hubble parameters measured by DESI DR2 BAO and Pantheon+ supernovae.