REVIEW 1 cited by
Axial Bianchi I meets drifting extragalactic sources
Not yet reviewed by Pith; the record is open.
This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.
SPECIMEN: schema-true, not a live event
T0 review · schema-true
One-sentence machine reading of the paper's core claim.
pith:XXXXXXXX · record.json · timestamp
Axial Bianchi I meets drifting extragalactic sources
read the original abstract
We recompute {\it ab initio} the drift of comoving sources in axial Bianchi I universes. Our result resolves the long-standing disagreement between the computations by Quercellini et al. from 2009 and by Marcori et al. from 2018 in favour of the latter. These computations have a potential impact on Gaia data analysis and cosmological parameter estimation.
Forward citations
Cited by 1 Pith paper
-
Axial Bianchi IX meets Gaia data
In axial Bianchi IX universes with dust and a cosmological constant, the linearized cosmic drift equals that of axial Bianchi I, so curvature drops out of the drift at first order.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.