Quantum Gravity and the Cosmological Constant Problem
J. W. Moffat

TL;DR
This paper presents a nonlocal quantum gravity model that suppresses the vacuum energy, addressing the cosmological constant problem by aligning theoretical predictions with observations.
Contribution
It introduces a finite, unitary nonlocal quantum gravity framework that effectively reduces the cosmological constant to observed levels.
Findings
Exponential suppression of vacuum density achieved
Agreement with observational bounds on cosmological constant
A novel nonlocal approach to quantum gravity
Abstract
A finite and unitary nonlocal formulation of quantum gravity is applied to the cosmological constant problem. The entire functions in momentum space at the graviton-standard model particle loop vertices generate an exponential suppression of the vacuum density and the cosmological constant to produce agreement with their observational bounds.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories
