Is the future universe singular: Dark Matter versus modified gravity?
Shin'ichi Nojiri, Sergei D. Odintsov

TL;DR
This paper investigates whether future universe singularities can be avoided through dark matter interactions or modified gravity, proposing mechanisms that could resolve various types of cosmological singularities.
Contribution
It demonstrates that specific initial conditions, coupled dark energy, and modified gravity models can potentially prevent or resolve future cosmological singularities.
Findings
Existence of de Sitter solutions can mitigate certain singularities.
Coupling with dark matter may help resolve the coincidence problem.
Modified gravity can universally address multiple singularity types.
Abstract
The fundamental problem of the occurrence/removal of finite-time future singularity in the universe evolution for coupled dark energy (DE) is addressed. It is demonstrated the existence of the (instable or local minimum) de Sitter space solution which may cure the Type II or Type IV future singularity for DE coupled with DM as the result of tuning the initial conditions. In case of phantom DE, the corresponding coupling may help to resolve the coincidence problem but not the Big Rip (Type I) singularity issue. We show that modified gravity of special form or inhomogeneous DE fluid may offer the universal scenario to cure the Type I,II,III or IV future singularity of coupled (fluid or scalar) DE evolution.
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