Did the Universe experience a pressure non-crushing type cosmological singularity in the recent past?

In the recent literature it has been shown that the H-0 tension may be eliminated if an abrupt physics transition changed the Cepheid parameters in the near past of the Universe, nearly 70-150 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 F(R) 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 F(R) gravity. Moreover, we stress the fact that pressure singularities can disrupt the trajectories of bound objects in the Universe, which is also pointed out in the literature, even in the context of general relativity. We also show numerically in a general relativistic framework that elliptic trajectories are distorted and changed to different elliptic trajectories when the Universe passes through the pressure singularity. Such a disruption of the trajectories could have tidal effects on the surface of the Earth, for example on sea waters and oceans, regarding the distortion of Moon's elliptic trajectory. Accordingly, the distortion of Earth's trajectory around the Sun could have affected climatologically the Earth 70-150 Myrs ago. Copyright (C) 2022 EPLA

Automated summary

Recent literature suggests that the H-0 tension could be resolved if there was an abrupt physics transition that altered the Cepheid parameters in the recent past of the Universe (approximately 70-150 million years ago). This study explores the possibility that this transition was caused by the smooth passage of the Universe through a pressure finite-time cosmological singularity. The authors discuss how this scenario can be realized using F(R) gravity, without the need for a scalar field or specific matter fluids, and highlight the potential effects of the pressure singularity on the gravitational constant and trajectories of bound objects in the Universe.