Hints of FLRW Breakdown from Supernovae
arXiv:2106.02532 · doi:10.1103/PhysRevD.105.063514
Abstract
A 10\% difference in the scale for the Hubble parameter constitutes a clear problem for cosmology. Here, considering angular distribution of Type Ia supernovae (SN) within the Pantheon compilation and working within flat CDM cosmology, we observe a correlation between higher and the CMB dipole direction, confirming our previous results for strongly-lensed quasars \cite{Krishnan:2021dyb}. Concretely, we record a km/s/Mpc variation in at antipodal points on the sky within the Pantheon sample, which is evident in the Low subsample () and gets enhanced by higher redshift SN. Our work raises the possibility that we may be at the precision required to probe anisotropic Hubble expansions, while providing a concrete prediction for future inferences of .
5 pages, 5 figures, comments are most welcome; v2 appendix added on general trend; v3 presentation improved and streamlined; v4 references and appendix added, to appear in PRD
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