Cosmology with the cosmic rest frame
G\"unter Scharf

TL;DR
This paper explores a spherically symmetric inhomogeneous universe model assuming a direct link between comoving coordinates and the cosmic rest frame, leading to a unique solution that can fit the Hubble diagram without a cosmological constant.
Contribution
It introduces a specific inhomogeneous cosmological model based on the cosmic rest frame, deriving a unique solution that challenges the necessity of a cosmological constant.
Findings
The pressure must be zero in this model.
The metric is independent of the radial coordinate.
The model can fit the Hubble diagram without a cosmological constant.
Abstract
We assume a one-to-one correspondence between comoving coordinates and the cosmic rest frame in a spherically symmetric inhomogeneous universe. This strongly restricts the solutions of Einstein's equations: (i) The pressure must be zero. (ii) The metric does not depend on the radial coordinate, the FLRW cosmology is excluded (strong homogeneity). (iii) The unique solution corresponds to the Datt-Ruban solution. Beside the Hubble constant it contains one free constant of integration which can be chosen in order to represent the measured Hubble diagram without using a cosmological constant.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Relativity and Gravitational Theory
