Wall of fundamental constants

Keith A. Olive, Marco Peloso, and Jean-Philippe Uzan
Phys. Rev. D 83, 043509 – Published 9 February 2011

Abstract

We consider the signatures of a domain wall produced in the spontaneous symmetry breaking involving a dilatonlike scalar field coupled to electromagnetism. Domains on either side of the wall exhibit slight differences in their respective values of the fine-structure constant, α. If such a wall is present within our Hubble volume, absorption spectra at large redshifts may or may not provide a variation in α relative to the terrestrial value, depending on our relative position with respect to the wall. This wall could resolve the contradiction between claims of a variation of α based on Keck/Hires data and of the constancy of α based on Very Large Telescope data. We derive the properties of the wall and the parameters of the underlying microscopic model required to reproduce the possible spatial variation of α. We discuss the constraints on the existence of the low-energy domain wall and describe its observational implications concerning the variation of the fundamental constants.

  • Figure
  • Figure
  • Figure
  • Received 12 November 2010

DOI:https://doi.org/10.1103/PhysRevD.83.043509

© 2011 American Physical Society

Authors & Affiliations

Keith A. Olive1,2, Marco Peloso2, and Jean-Philippe Uzan3,4,5

  • 1William I. Fine Theoretical Physics Institute, University of Minnesota, Minneapolis, Minnesota, 55455, (USA)
  • 2School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota, 55455 (USA)
  • 3Institut d’Astrophysique de Paris, UMR-7095 du CNRS, Université Pierre et Marie Curie, 98 bis bd Arago, 75014 Paris (France)
  • 4Department of Mathematics and Applied Mathematics, Cape Town University, Rondebosch 7701 (South Africa)
  • 5National Institute for Theoretical Physics (NITheP), Stellenbosch 7600 (South Africa).

See Also

Where are the walls? Spatial variation in the fine-structure constant

Keith A. Olive, Marco Peloso, and Adam J. Peterson
Phys. Rev. D 86, 043501 (2012)

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 83, Iss. 4 — 15 February 2011

Reuse & Permissions
Access Options
CHORUS

Article Available via CHORUS

Download Accepted Manuscript
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
×