Light scalar fields coupled to matter are a common consequence of theories of dark energy and attempts to solve the cosmological constant problem. The chameleon screening mechanism is commonly invoked in order to suppress the fifth forces mediated by these scalars, sufficiently to avoid current experimental constraints, without fine tuning. The force is suppressed dynamically by allowing the mass of the scalar to vary with the local density. Recently it has been shown that near future cold atoms experiments using atom-interferometry have the ability to access a large proportion of the chameleon parameter space. In this work we demonstrate how experiments utilising asymmetric parallel plates can push deeper into the remaining parameter space...
Chameleon scalar fields can screen their associated fifth forces from detection by changing their ma...
AbstractLight scalar fields can drive the accelerated expansion of the universe. Hence, they are obv...
AbstractChameleons can play a role in the recent acceleration of the expansion of the Universe. We p...
Light scalar fields coupled to matter are a common consequence of theories of dark energy and attemp...
Theories of dark energy require a screening mechanism to explain why the associated scalar fields do...
We review the tantalising prospect that the first evidence for the dark energy driving the observed ...
A light scalar field framework of dark energy, sometimes referred to as quintessence, introduces a f...
If dark energy, which drives the accelerated expansion of the universe, consists of a light scalar f...
We have calculated the chameleon pressure between two parallel plates in the presence of an interven...
The chameleon model is a scalar field theory with a screening mechanism that explains how a cosmolog...
Light scalar fields can drive the accelerated expansion of the universe. Hence, they are obvious dar...
Dynamically screened scalar field theories form an attractive collection of models that were introdu...
Scalar fields with a"chameleon" property, in which the effective particle mass is a functi...
We apply the new constraints from atom-interferometry searches for screening mechanisms to the symme...
Chameleon scalar fields can screen their associated fifth forces from detection by changing their ma...
AbstractLight scalar fields can drive the accelerated expansion of the universe. Hence, they are obv...
AbstractChameleons can play a role in the recent acceleration of the expansion of the Universe. We p...
Light scalar fields coupled to matter are a common consequence of theories of dark energy and attemp...
Theories of dark energy require a screening mechanism to explain why the associated scalar fields do...
We review the tantalising prospect that the first evidence for the dark energy driving the observed ...
A light scalar field framework of dark energy, sometimes referred to as quintessence, introduces a f...
If dark energy, which drives the accelerated expansion of the universe, consists of a light scalar f...
We have calculated the chameleon pressure between two parallel plates in the presence of an interven...
The chameleon model is a scalar field theory with a screening mechanism that explains how a cosmolog...
Light scalar fields can drive the accelerated expansion of the universe. Hence, they are obvious dar...
Dynamically screened scalar field theories form an attractive collection of models that were introdu...
Scalar fields with a"chameleon" property, in which the effective particle mass is a functi...
We apply the new constraints from atom-interferometry searches for screening mechanisms to the symme...
Chameleon scalar fields can screen their associated fifth forces from detection by changing their ma...
AbstractLight scalar fields can drive the accelerated expansion of the universe. Hence, they are obv...
AbstractChameleons can play a role in the recent acceleration of the expansion of the Universe. We p...