Dynamics of the Peccei-Quinn scale

Linda M. Carpenter, Michael Dine, and Guido Festuccia
Phys. Rev. D 80, 125017 – Published 15 December 2009

Abstract

Invoking the Peccei-Quinn (PQ) solution to the strong CP problem substitutes the puzzle of why θqcd is so small with the puzzle of why the PQ symmetry is of such high quality. Cosmological and astrophysical considerations raise further puzzles. This paper explores these issues in several contexts: string theory and field theory, and theories without and with low energy supersymmetry. Among the questions studied are whether requiring axion dark matter can account for the quality of the PQ symmetry, to which the answer is sometimes yes. In nonsupersymmetric theories, we find fa=1012GeV is quite plausible. In gauge mediation, cosmological constraints on pseudomoduli place fa in this range, and require that the gravitino mass be of order an MeV.

  • Figure
  • Received 17 August 2009

DOI:https://doi.org/10.1103/PhysRevD.80.125017

©2009 American Physical Society

Authors & Affiliations

Linda M. Carpenter, Michael Dine, and Guido Festuccia

  • Santa Cruz Institute for Particle Physics and Department of Physics, University of California, Santa Cruz, California 95064, USA

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 80, Iss. 12 — 15 December 2009

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×