Cosmological constant and renormalization of gravity
Shin'ichi Nojiri

TL;DR
This paper extends a topological model addressing the cosmological constant problem by incorporating quantum correction divergences and explores its implications for cosmology.
Contribution
It introduces an extended topological gravity model that absorbs quantum divergences, offering a novel approach to the cosmological constant problem.
Findings
Vacuum energy divergences can be absorbed into scalar field redefinition.
The extended model provides a new framework for quantum corrections in cosmology.
Potential implications for resolving the cosmological constant problem.
Abstract
In arXiv:1601.02203 and arXiv:1702.07063, we have proposed a topological model with a simple Lagrangian density and have tried to solve one of the cosmological constant problems. The Lagrangian density is the BRS exact and therefore the model can be regarded as a topological theory. In this model, the divergence of the vacuum energy coming from the quantum corrections from matters can be absorbed into the redefinition of the scalar field. In this paper, we consider the extension of the model in order to apply the mechanism to other kinds of divergences coming from the quantum correction and consider the cosmology in an extended model.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories
