pith. sign in

arxiv: 1503.01015 · v2 · pith:3YQOXXFHnew · submitted 2015-03-03 · ✦ hep-th · astro-ph.CO· hep-ph

Widening the Axion Window via Kinetic and St\"uckelberg Mixings

classification ✦ hep-th astro-ph.COhep-ph
keywords axiondecaykineticuckelbergconstantmixingsonlywindow
0
0 comments X
read the original abstract

We point out that kinetic and St\"uckelberg mixings that are generically present in the low energy effective action of axions can significantly widen the window of axion decay constants. We show that an effective super-Planckian decay constant can be obtained even when the axion kinetic matrix has only sub-Planckian entries. Our minimal model involves only two axions, a St\"uckelberg U(1) and a modest rank instanton generating non-Abelian group. Below the mass of the St\"uckelberg U(1), there is only a single axion with a non-perturbatively generated potential. In contrast to previous approaches, the enhancement of the axion decay constant is not tied to the number of degrees of freedom introduced. We also discuss how kinetic mixings can lower the decay constant to the desired axion dark matter window. String theory embeddings of this scenario and their phenomenological features are briefly discussed.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.