Linearized Bekenstein Varying Alpha Models
arXiv:astro-ph/0402379 · doi:10.1103/PhysRevD.70.083506
Abstract
We study the simplest class of Bekenstein-type, varying models, in which the two available free functions (potential and gauge kinetic function) are Taylor-expanded up to linear order. Any realistic model of this type reduces to a model in this class for a certain time interval around the present day. Nevertheless, we show that no such model is consistent with all existing observational results. We discuss possible implications of these findings, and in particular clarify the ambiguous statement (often found in the literature) that ``the Webb results are inconsistent with Oklo''.
7 pages, 4 figures
References in corpus (33)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results
- Cosmological Results from High-z Supernovae
- The fundamental constants and their variation: observational status and theoretical motivations
- Further Evidence for Cosmological Evolution of the Fine Structure Constant
- The Confrontation between General Relativity and Experiment
- Further evidence for a variable fine-structure constant from Keck/HIRES QSO absorption spectra
- Constraints on the equation of state of dark energy and the Hubble constant from stellar ages and the CMB
- The State of the Dark Energy Equation of State
- A Simple Varying-alpha Cosmology
- A Search for Variations of Fundamental Constants using Atomic Fountain Clocks
- Probing the cosmological variation of the fine-structure constant: Results based on VLT-UVES sample
- Probing the dark side: Constraints on the dark energy equation of state from CMB, large scale structure and Type Ia supernovae
- Varying Alpha in a More Realistic Universe
- Evolution of the Fine Structure Constant Driven by Dark Matter and the Cosmological Constant
- Early-universe constraints on a time-varying fine structure constant
- Models of quintessence coupled to the electromagnetic field and the cosmological evolution of alpha
- A Re-examination of the Re Bound on the Variation of Fundamental Couplings
- Time Variation of the Fine Structure Constant Driven by Quintessence
- Reconstructing the dark energy equation of state with varying alpha
- Neutron Moderation in the Oklo Natural Reactor and the Time Variation of alpha
- WMAP Constraints on varying and the Promise of Reionization
- Mapping the Dark Energy with Varying Alpha
- Scalar-Tensor Cosmologies and their Late Time Evolution
- Measuring in the Early Universe: CMB Temperature, Large-Scale Structure and Fisher Matrix Analysis
- Condensate cosmology -- dark energy from dark matter
- Gauge-Invariant Perturbations of Varying-Alpha Cosmologies
- The onset of the non-linear regime in unified dark matter models
- Cosmology with Varying Constants
- Cosmology with Varying Constants
- Does the proton-to-electron mass ratio vary in the course of cosmological evolution?
- Galaxy Clustering and Dark Energy
- New constraints on varying
- Varying Fine-Structure Constant and the Cosmological Constant Problem
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- Environmental Dependence of Masses and Coupling Constants
- Is there Correlation between Fine Structure and Dark Energy Cosmic Dipoles?
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- General Dynamics of Varying-Alpha Universes
- Explicit Integration of Friedmann's Equation with Nonlinear Equations of State
- Varying Constants
- Cosmological Bounds on Spatial Variations of Physical Constants
- The Wall of Fundamental Constants
- The thawing dark energy dynamics: Can we detect it?
- The coincidence problem in linear dark energy models
- The transient and the late time attractor tachyon dark energy: Can we distinguish it from quintessence ?
- Varying Couplings in Electroweak Theory
- Varying-Alpha Cosmologies with Potentials
- Cosmological evolution of Alpha driven by a general coupling with Quintessence
- The Local Effects of Cosmological Variations in Physical 'Constants' and Scalar Fields I. Spherically Symmetric Spacetimes
- The Local Effects of Cosmological Variations in Physical 'Constants' and Scalar Fields II. Quasi-Spherical Spacetimes
- Anthropic versus cosmological solutions to the coincidence problem
- On the cosmological evolution of alpha and mu and the dynamics of dark energy
- Where are the Walls?
- Evolution of the fine-structure constant in the non-linear regime
- Cosmic Variation of Proton to Electron Mass Ratio with an interacting Higgs Scalar Field
- Varying Alpha Monopoles
- Cosmic strings in Bekenstein-type models
- Impact of the matter density uncertainty on the dark energy reconstruction
- Estimations of the cosmological parameters from the observational variation of the fine structure constant
- Assessing the viability of successful reconstruction of the dynamics of dark energy using varying fundamental couplings
- Gravitational Effects of Varying Alpha Strings
- Spacetime variation of and the CMB power spectra after the recombination
- Cosmological Consequences of Topological Defects: Dark Energy and Varying Fundamental Constants