No-go guide for the Hubble tension: late-time or local-scale new physics
arxiv(2024)
摘要
The standard model of modern cosmology might be cracked by the recent
persistent hot debate on the Hubble-constant (H_0) tension, which manifests
itself as the sound-horizon (r_s) tension or absolute-magnitude (M_B)
tension if deeming the origin of the Hubble tension from modifying the early or
late Universe, respectively. In this Letter, we achieve a fully
model-independent constraint (fitting a model-independent global
parameterization to a model-independent inverse distant ladder with a
model-independent high-redshift calibration) on late-time models with strong
evidence against homogeneous new physics over the Λ-cold-dark
(ΛCDM) model. Further using this model-independent constraint to
calibrate sufficiently local supernovae with corresponding late-time models
extrapolated below the homogeneity scale, we find surprisingly that, although
both H_0 tension and M_B tension are absent in our local Universe, a
combination of H_0 and M_B as the intercept a_B of the magnitude-redshift
relation exhibits 3∼ 7σ tension even for the ΛCDM model. This
a_B tension seems to call for local-scale inhomogeneous new physics disguised
as local observational systematics.
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