Published April 4, 2008 | Version v1
Journal article

How changing physical constants and violation of local position invariance may occur?

  • 1. School of Physics, University of New South Wales, Sydney NSW 2052 (Australia) and Institute for Advanced Study, Massey University (Albany campus), Privite Bag 102904, North Shore MSC, Auckland (New Zealand)
  • 2. Department of Physics and Astronomy, State University of New York, Stony Brook NY 11794-3800 (United States)

Description

Light scalar fields very naturally appear in modern cosmological models, affecting such parameters of Standard Model as electromagnetic fine structure constant α, dimensionless ratios of electron or quark mass to the QCD scale, me,q/ΛQCD. Cosmological variations of these scalar fields should occur because of drastic changes of matter composition in Universe: the latest such event is rather recent (redshift z∼0.5), from matter to dark energy domination. In a two-brane model (we use as a pedagogical example) these modifications are due to changing distance to ''the second brane'', a massive companion of 'our brane'. Back from extra dimensions, massive bodies (stars or galaxies) can also affect physical constants. They have large scalar charge Qd proportional to number of particles which produces a Coulomb-like scalar field φ = Qd/r. This leads to a variation of the fundamental constants proportional to the gravitational potential, e.g. δα/α = kαδ(GM/rc2). We compare different manifestations of this effect, which is usually called violation of local position invariance. The strongest limits kα+0.17ke (-3.5±6)*10-7 are obtained from the measurements of dependence of atomic frequencies on the distance from Sun (the distance varies due to the ellipticity of the Earth's orbit)

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
995
Journal Issue
1
Journal Page Range
p. 1-11
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
Workshop on nuclei and mesoscopic physics
Acronym
WNMP 2007
Dates
20-22 Oct 2007
Place
East Lansing, MI (United States)

Optional Information

Notes
(c) 2008 American Institute of Physics