Cosmology with Varying Constants
arXiv:astro-ph/0008287 · doi:10.1142/9789812811110_0003
Abstract
I motivate and discuss some recent work on theories with varying constants, and consider some possible observational consequences and tests. Particular emphasis is given to models which can (almost) exactly mimic the predictions of standard inflationary models.
6 pages; Based on talks given at the Cosmology2000 and X ENAA workshops, July 2000
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Cited by in corpus (18)
- The fundamental constants and their variation: observational status and theoretical motivations
- New varying speed of light theories
- Measuring in the Early Universe: CMB Polarization, Reionization and the Fisher Matrix Analysis
- WMAP Constraints on varying and the Promise of Reionization
- Constraints on the CMB Temperature Evolution using Multi-Band Measurements of the Sunyaev Zel'dovich Effect with the South Pole Telescope
- Constraints on the CMB temperature redshift dependence from SZ and distance measurements
- Variation of fundamental parameters and dark energy. A principal component approach
- Linearized Bekenstein Varying Alpha Models
- New constraints on varying
- Dark Energy Models With Variable Equation Of State Parameter
- A stellar test of the physics of unification
- Constraints on extended Bekenstein models from cosmological, astrophysical, and local data
- Cosmic strings in Bekenstein-type models
- Scenario of Accelerating Universe from the Phenomenological Λ- Models
- Notes on several phenomenological laws of quantum gravity
- Is Quintessence an Indication of a Time-Varying Gravitational Constant?
- A reciprocal Wald theorem for varying gravitational function
- Astrophysical Probes of Fundamental Physics