A hint of matter underdensity at low ?
arXiv:1903.11743 · doi:10.1088/1475-7516/2019/09/006
Abstract
The CDM cosmological model provides to first approximation a good description of the universe, but various tensions with data, most notably Hubble tension, persist. In this work we confront CDM with the Pantheon Type Ia supernovae dataset and perform a two-parameter fit of the distance modulus for a running cut-off . We observe that in a window between and there is a 1 - 2 discrepancy with the Planck value , which points to a potential matter underdensity. For high-energy theorists, the analysis appears to support the de Sitter Swampland conjecture.
9 pages, my first foray into astro-ph, feedback welcome; v2 11 pages, analysis improved, references updated; v3 corrections to statistical significance, version to appear in JCAP
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