How changing physical constants and violation of local position invariance may occur?
Creators
- 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
- DOI
- 10.1063/1.2915601;
- arXiv
- arXiv:physics/0701220v2;
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)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 40017644
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BRANES; COMPARATIVE EVALUATIONS; COSMOLOGICAL MODELS; COSMOLOGY; D QUARKS; ELECTRONS; FINE STRUCTURE; FUNDAMENTAL CONSTANTS; NONLUMINOUS MATTER; POTENTIALS; QUANTUM CHROMODYNAMICS; RED SHIFT; SCALAR FIELDS; SCALARS; STANDARD MODEL; STRING MODELS; STRING THEORY; UNIVERSE; VARIATIONS
- Descriptors DEC
- COMPOSITE MODELS; ELEMENTARY PARTICLES; EVALUATION; EXTENDED PARTICLE MODEL; FERMIONS; FIELD THEORIES; GRAND UNIFIED THEORY; LEPTONS; M-THEORY; MATHEMATICAL MODELS; MATTER; PARTICLE MODELS; QUANTUM FIELD THEORY; QUARK MODEL; QUARKS; UNIFIED GAUGE MODELS
Optional Information
- Notes
- (c) 2008 American Institute of Physics