We explore the possibility that the reported time variation of the fine structure constant α is due to a coupling between electromagnetism and gravitation. We predict such a coupling from a very simple effective theory of physical interactions, under the form of an improved version of the Kaluza-Klein theory. We show that it precisely leads to a variation of the effective fine structure constant with cosmic conditions, and thus with cosmic time. The comparison with the recent data from distant quasars absorption line spectra gives a good agreement; moreover, this may reconcile the claimed results on α with the upper limit from the Oklo naturel Uranium fission reactor
It has been a notably elusive task to find a remotely sensical ansatz for a calculation of Sommerfel...
We consider astronomical and local bounds on the time variation of fundamental constants to test som...
In the present work, we consider the cosmological constant model $$\Lambda \propto \alpha ^{-6}$$, w...
We explore the possibility that the reported time variation of the fine structure constant α is due ...
Recently, evidence indicating cosmological variations of the fine structure constant, α, has been re...
Review of recent works devoted to the temporal and spatial variation of the fundamental constants an...
This is an articleWithout veering off the shores of conventional physics and without making any exog...
Abstract A new method based on large scale structure observations is proposed to probe a possible te...
We review properties of theories for the variation of the gravitation and fine structure 'constants'...
AbstractWithin the context of mass-varying neutrinos, we construct a cosmological model that has a p...
The fine structure constant at red shifts Δλ / λ≈0.2, corresponding to an epoch around two billion y...
56 pages, l7 figuresThis article describes the various experimental bounds on the variation of the f...
AbstractUnification of the gauge couplings would imply that time variations of the fine structure co...
Aims. We analyze the consistency of different astronomical data of the variation in the fine-structu...
Current theories that seek to unify gravity with the other fundamental interactions suggest that spa...
It has been a notably elusive task to find a remotely sensical ansatz for a calculation of Sommerfel...
We consider astronomical and local bounds on the time variation of fundamental constants to test som...
In the present work, we consider the cosmological constant model $$\Lambda \propto \alpha ^{-6}$$, w...
We explore the possibility that the reported time variation of the fine structure constant α is due ...
Recently, evidence indicating cosmological variations of the fine structure constant, α, has been re...
Review of recent works devoted to the temporal and spatial variation of the fundamental constants an...
This is an articleWithout veering off the shores of conventional physics and without making any exog...
Abstract A new method based on large scale structure observations is proposed to probe a possible te...
We review properties of theories for the variation of the gravitation and fine structure 'constants'...
AbstractWithin the context of mass-varying neutrinos, we construct a cosmological model that has a p...
The fine structure constant at red shifts Δλ / λ≈0.2, corresponding to an epoch around two billion y...
56 pages, l7 figuresThis article describes the various experimental bounds on the variation of the f...
AbstractUnification of the gauge couplings would imply that time variations of the fine structure co...
Aims. We analyze the consistency of different astronomical data of the variation in the fine-structu...
Current theories that seek to unify gravity with the other fundamental interactions suggest that spa...
It has been a notably elusive task to find a remotely sensical ansatz for a calculation of Sommerfel...
We consider astronomical and local bounds on the time variation of fundamental constants to test som...
In the present work, we consider the cosmological constant model $$\Lambda \propto \alpha ^{-6}$$, w...