Varying Constants
Thibault Damour
Abstract
We review some string-inspired theoretical models which incorporate a correlated spacetime variation of coupling constants while remaining naturally compatible both with phenomenological constraints coming from geochemical data (Oklo; Rhenium decay) and with present equivalence principle tests. Barring unnatural fine-tunings of parameters, a variation of the fine-structure constant as large as that recently ``observed'' by Webb et al. in quasar absorption spectra appears to be incompatible with these phenomenological constraints. Independently of any model, it is emphasized that the best experimental probe of varying constants are high-precision tests of the universality of free fall, such as MICROSCOPE and STEP. Recent claims by Bekenstein that fine-structure-constant variability does not imply detectable violations of the equivalence principle are shown to be untenable.
Create a lesson
Related papers
Scale-Dependent Weak-Field Dynamics in Horndeski Theory: Galaxy Rotation Curves and Turnaround Scales
Hatice Özer
Mixed-Order Parity-Violating Corrections to Rotating Black Holes in Combined Scalar Gauss-Bonnet and Dynamical Chern-Simons Gravity
Abhishek Rout, Brett Altschul
On the Motion of a Point Electric Charge in the Field of Wu-Yang Monopoles in Bertotti-Robinson Spacetimes
Tekin Dereli, Yorgo Senikoglu
Particle dynamics in rotating charged Bumblebee black holes: An analytical correspondence with Kerr-Newman
Deyou Chen, Chuang Yang
A Unified AI Framework for Rapid and Accurate Waveform Generation of Compact Binary Coalescences
Mengfei Sun, Jin Li, Yuanhong Zhong et al.
Final state of superradiant instability in Einstein-Maxwell-dilaton black hole
Afsaneh Rahmani, Samaneh Oghbaiee