Published March 6, 2008 | Version v1
Journal article

Phase transition in the fine structure constant

  • 1. Department of Physics, University of Wisconsin-Milwaukee, Milwaukee, WI 53201 (United States)
  • 2. Department of Physics, University of Wisconsin, Madison, WI 53706 (United States)
  • 3. Department of Physics, Northeastern University, Boston, MA 02115 (United States)
  • 4. Department of Physics and Astronomy, University of Kansas, Lawrence, KS 66045 (United States)

Description

Within the context of mass-varying neutrinos, we construct a cosmological model that has a phase transition in the electromagnetic fine structure constant α at a redshift of 0.5. The model accommodates hints of a time variable α in quasar spectra and the nonobservance of such an effect at very low redshifts. It is consistent with limits from the recombination and primordial nucleosynthesis eras and is free of instabilities

Availability note (English)

Available from http://dx.doi.org/10.1016/j.physletb.2008.01.047

Additional details

Identifiers

DOI
10.1016/j.physletb.2008.01.047;
arXiv
arXiv:0711.4055v2;
PII
S0370-2693(08)00143-3;

Publishing Information

Journal Title
Physics Letters. Section B
Journal Volume
660
Journal Issue
5
Journal Page Range
p. 529-533
ISSN
0370-2693
CODEN
PYLBAJ

INIS

Optional Information

Copyright
Copyright (c) 2008 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.