Fetching the paper…
Reading the bibliography…
We have shown (Colin et al., 2019) that the acceleration of the Hubble expansion rate inferred from Type Ia supernovae (SNe Ia) is, at $3.9\sigma$ significance, a dipole approximately aligned with the CMB dipole, while its monopole component, which can be interpreted as due to a Cosmological Constant or dark energy, is consistent with zero at $1.4\sigma$.
Nothing clear enough to list yet.
Nothing clear enough to list yet.
Nothing clear enough to list yet.
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…