# Quantum Aspects of Nonlocal Approach to the Cosmological Constant Problem

## TL;DR

This paper examines quantum effects on a nonlocal approach to the cosmological constant problem, revealing that radiative corrections destabilize the effective cosmological constant unless a new scale-invariant model is introduced for stability.

## Contribution

It provides a quantum analysis of a nonlocal cosmological constant approach and proposes a scale-invariant model to achieve stability against quantum corrections.

## Key findings

- Quantum effects cause radiative corrections to the cosmological constant.
- The original nonlocal model is unstable under quantum corrections.
- A new scale-invariant model stabilizes the effective cosmological constant.

## Abstract

We have recently presented a manifestly local and general coordinate invariant formulation of a nonlocal approach to the cosmological constant problem which has been proposed by Carroll and Remmen. In this article, based on our formulation, we investigate some quantum aspects of this approach to the cosmological constant problem. In particular, we explicitly evaluate quantum effects to the effective cosmological constant from matter fields at one-loop level, and show that the effective cosmological constant receives radiative corrections and is not stable against quantum corrections so that it must be fine-tuned at every stage in the loop expansion. Next, we will propose a new scale-invariant model of a nonlocal approach to the cosmological constant problem, and show explicitly that in this new model the effective cosmological constant is indeed stable against radiative corrections.