Dark Energy from Entanglements with Mirror Universe
Merab Gogberashvili, Tinatin Tsiskaridze

TL;DR
This paper proposes a novel framework where the Universe's dark energy arises from entanglement with a mirror universe, avoiding fine-tuning and linking dark energy to boundary conditions in a pair-universe model.
Contribution
It introduces a pair-universe model with entanglement energy as the source of dark energy, eliminating the need for vacuum fluctuation explanations and fixing the cosmological constant via boundary conditions.
Findings
Effective entanglement energy accounts for observed dark energy density.
Global zero-energy condition cancels vacuum energy contributions.
Boundary conditions at the horizon determine the cosmological constant.
Abstract
We investigate a possible resolution of the dark energy problem within a pair-universe framework, in which the Universe emerges as an entangled pair of time-reversed sectors. In this setting, a global zero-energy condition allows vacuum energy contributions from the two sectors to cancel, alleviating the need for extreme fine-tuning. We propose that the observed dark energy does not originate from vacuum fluctuations but instead arises as an effective entanglement energy between the visible universe and its mirror counterpart. Treating the cosmological constant as an integration constant fixed by boundary conditions rather than a fundamental parameter, we show that the cosmological equations can be formulated without explicitly introducing vacuum energy. By imposing physically motivated boundary conditions at the cosmological event horizon, we obtain an integration constant consistent…
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Taxonomy
TopicsCosmology and Gravitation Theories · Dark Matter and Cosmic Phenomena · Galaxies: Formation, Evolution, Phenomena
