Did the Universe Experienced a Pressure non-Crushing Type Cosmological Singularity in the Recent Past?
S.D. Odintsov, V.K. Oikonomou

TL;DR
This paper explores the hypothesis that a pressure finite-time cosmological singularity in the recent past may have influenced Earth's climate and trajectories, potentially resolving the H_0 tension and leaving observable imprints.
Contribution
It proposes that a pressure singularity caused by smooth passage through a non-crushing cosmological event can impact cosmic and local dynamics, modeled via $F(R)$ gravity without exotic matter.
Findings
Pressure singularity can alter gravitational constant in $F(R)$ gravity.
Numerical simulations show distorted planetary trajectories during the singularity.
The scenario could explain past climate and trajectory disruptions on Earth.
Abstract
In the recent literature it has been shown that the tension may be eliminated if an abrupt physics transition changed the Cepheid parameters in the near past of the Universe, nearly Myrs ago. In this letter we stress the possibility that this abrupt transition was caused by the smooth passage of our Universe through a pressure finite-time cosmological singularity. Being a non-crushing type singularity the pressure singularity can leave its imprints in the Universe, since it occurs globally and literally everywhere. We discuss how this scenario could easily be realized by gravity, with the strong energy conditions being satisfied without the need for a scalar field or specific matter fluids. We also stress the fact that the pressure singularity can affect the effective gravitational constant of gravity. Moreover, we stress the fact that pressure…
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