Quantum Spacetime Instability and Breakdown of Semiclassical Gravity
Hiroki Matsui, Naoki Watamura

TL;DR
This paper demonstrates that semiclassical gravity models are fundamentally unstable in cosmological settings, leading to rapid spacetime curvatures and inconsistencies with observations, questioning their validity for describing our Universe.
Contribution
The study reveals the inherent instabilities in semiclassical gravity and shows that such models cannot reliably describe the Universe's evolution.
Findings
Homogeneous and isotropic flat Universe solutions are unstable.
Instabilities lead to Planck-scale curvatures in short times.
Semiclassical solutions conflict with Planck data and observations.
Abstract
The semiclassical gravity describes gravitational back-reactions of the classical spacetime interacting with quantum matter fields but the quantum effects on the background is formally defined as higher derivative curvatures. These induce catastrophic instabilities and classic solutions become unstable under small perturbations or their evolutions. In this paper we discuss validity of the semiclassical gravity from the perspective of the spacetime instabilities and consider cosmological dynamics of the Universe in this theory. We clearly show that the homogenous and isotropic flat Universe is unstable and the solutions either grow exponentially or oscillate even in Planckian time . The subsequent curvature evolution leads to Planck-scale spacetime curvature in a short time and causes a catastrophe of the Universe…
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