Further Evidence for Cosmological Evolution of the Fine Structure Constant
arXiv:astro-ph/0012539 · doi:10.1103/PhysRevLett.87.091301
Abstract
We describe the results of a search for time variability of the fine structure constant, alpha, using absorption systems in the spectra of distant quasars. Three large optical datasets and two 21cm/mm absorption systems provide four independent samples, spanning 23% to 87% of the age of the universe. Each sample yields a smaller alpha in the past and the optical sample shows a 4-sigma deviation: da/a = -0.72 +/- 0.18 x 10^{-5} over the redshift range 0.5 < z < 3.5. We find no systematic effects which can explain our results. The only potentially significant systematic effects push da/a towards positive values, i.e. our results would become more significant were we to correct for them.
5 pages, 1 figure. Published in Phys. Rev. Lett. Small changes to discussion, added an acknowledgement and a reference
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- A homogeneous and isotropic universe must have a time varying light speed
- Invariance of the fine structure constant with temperature of the expanding universe
- Sensitivity Parameter and Time Variations of Fundamental Constants
- Very Light Cosmological Scalar Fields from a Tiny Cosmological Constant
- Cosmological solutions of Tensor-Vector theories of gravity with varying the space-time-matter coupling constant
- Analysing the Effect on CMB in a Parity and Charge Parity Violating Varying Alpha Theory
- A Mathematica Notebook for Alpha Decay Using an Exponentially Diffuse Boundary Potential
- The Relation Between Fundamental Constants and Particle Physics Parameters
- Does the QCD Scale vary in time?
- Extra Dimensions, Dual Relation and the Cosmological Constant
- On Generalized Theories of Varying Fine Structure Constant
- Avoiding unrealistic priors: the case of dark energy constraints from the time variation of the fine-structure constant
- 133Cs87Rb Laser Cooled Dual Fountain
- Dark Energy and the Time Dependence of Fundamental Particle Constants