Phenomenological Gravitational Phase Transition: Reconciliation between the Late and Early Universe
Marzieh Farhang, Nima Khosravi

TL;DR
This paper explores a phenomenological gravitational phase transition in the universe that transitions from an early to a late phase, aiming to reconcile discrepancies in cosmological measurements such as the Hubble constant and matter distribution.
Contribution
It introduces a new model with a transition in gravitational behavior characterized by a tanh function, and demonstrates its effectiveness in resolving multiple cosmological tensions.
Findings
A recent transition at redshift z_t ≈ 0.9 is preferred by data.
The transition relaxes the Hubble tension and matter distribution inconsistencies.
The model is consistent with various datasets and does not conflict with existing measurements.
Abstract
In this work we investigate whether a certain phenomenological extension to the general relativity (GR), in the form of a gravitational phase transition (GPT) in the Universe, can reduce the external tensions with the local Hubble measurements and the distribution of matter, characterized by , as well as its internal inconsistencies in the lensing amplitude and the low--high parameter estimates. We introduce new degrees of freedom into the background and the two scalar perturbation equations in the Newtonian gauge, with simultaneous transitions from an early gravitational phase equivalent to GR toward a late phase. We model the transition as a "tanh" parametrized by the transition redshift and width , with amplitudes and for the background and perturbations respectively. We verify the consistency of the…
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