Can rotation solve the Hubble Puzzle?
ABSTRACT The discrepancy between low and high redshift Hubble constant $H_0$ measurements is the highest significance tension within the concordance Lambda cold dark matter paradigm. If not due to unknown systematics, the Hubble Puzzle suggests a lack of understanding of the universe’s expansion history despite the otherwise spectacular success of the theory. We show that a Gödel inspired slowly rotating dark-fluid variant of the concordance model resolves this tension with an angular velocity today $\omega _0 \simeq 2\times 10^{-3}$ Gyr−1. Curiously, this is close to the maximal rotation, avoiding closed time-like loops with a tangential velocity less than the speed of light at the horizon.
Authors
- Balázs Endre Szigeti (ORCID: https://orcid.org/0000-0002-8028-962X)
- István Szapudi (ORCID: https://orcid.org/0000-0003-2274-0301)
- Imre Ferenc Barna
- G. G. Barnaföldi (ORCID: https://orcid.org/0000-0001-9223-6480)
Institutions
- Eötvös Loránd University (HU)
- University of Hawaii System (US)
- Université Bourgogne Franche-Comté (FR)
- FZU ‒ Institute of Physics of the Academy of Sciences of the Czech Republic (CZ)
- HUN-REN Wigner Research Centre for Physics (HU)
Publication Details
- Journal
- Monthly Notices of the Royal Astronomical Society
- Published
- 2025-03-21
- DOI
- https://doi.org/10.1093/mnras/staf446
- Citations
- 6
- Primary Topic
- Relativity and Gravitational Theory
- Type
- article
- Field-Weighted Citation Impact
- 6.93