Cosmological constant, inflation and no-cloning theorem
Qing-Guo Huang, Feng-Li Lin

TL;DR
This paper explores a theoretical link between the universe's accelerated expansion phases and the no-cloning theorem, deriving a lower bound on the cosmological constant consistent with observations.
Contribution
It proposes a novel relation between cosmic inflation, late-time acceleration, and quantum no-cloning, providing a new perspective on the cosmological constant.
Findings
Derives a lower bound on the cosmological constant from no-cloning constraints.
Suggests the universe's fate is an eternally accelerating expansion.
Connects quantum information principles with cosmological evolution.
Abstract
From the viewpoint of no-cloning theorem we postulate a relation between the current accelerated expansion of our universe and the inflationary expansion in the very early universe. It implies that the fate of our universe should be in a state with accelerated expansion. Quantitatively we find that the no-cloning theorem leads to a lower bound on the cosmological constant which is compatible with observations.
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