Three-Form Gauging of axion Symmetries and Gravity
Gia Dvali

TL;DR
This paper reformulates axion and certain Standard Model symmetries as gauge theories involving three-form fields, providing new insights into the strong CP problem, gravitational effects, and the stability of axion solutions.
Contribution
It introduces a three-form gauge field framework for understanding axion symmetries and gravity's impact on the strong CP problem, offering a novel perspective on symmetry breaking and vacuum structure.
Findings
Reformulation of axion and anomalous symmetries as three-form gauge theories.
Identification of gravitational effects as potential threats to axion solutions.
Insight into how additional massless three-forms can reintroduce the strong CP problem.
Abstract
Nonlinearly realized Abelian global symmetries can be reformulated as local shift symmetries gauged by three-form gauge fields. The anomalous symmetries of the Standard Model (such as Peccei-Quinn or ) can be dualized to local symmetries gauged by the Chern-Simons three-forms of the Standard Model gauge group. In this description the strong CP problem can be reformulated as the problem of a massless three-form field in QCD, which creates an arbitrary CP-violating constant four-form electric field in the vacuum. Both the axion as well as the massless quark solutions amount to simply Higgsing the three-form gauge field, hence screening the electric field in the vacuum. This language gives an alternative way for visualizing the physics of the axion solution as well as the degree of its vulnerability due to gravitational corrections. Any physics that can jeopardize the axion solution…
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
TopicsParticle physics theoretical and experimental studies · Dark Matter and Cosmic Phenomena · Black Holes and Theoretical Physics
