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Chameleons are scalar fields whose mass depends on the environment, specifically on the ambient matter density. While nearly massless in the cosmos, where the matter density is tiny, their mass is of order of an inverse millimeter on Earth,…

Astrophysics · Physics 2009-11-10 Ph. Brax , C. van de Bruck , A. C. Davis , J. Khoury , A. Weltman

Chameleon scalar field is a new model, which introduced to provide a mechanism for exhibiting accelerating universe. Chameleon field has several interesting aspects, such as field dependence on the local matter density. For this model we…

General Physics · Physics 2014-01-21 Kh. Saaidi , H. Sheikhahmadi , J. Afzali

The chameleon is a scalar field whose mass depends on the density of its environment. Chameleons are necessarily coupled to matter particles and will excite transitions between atomic energy levels in an analogous manner to photons. When…

High Energy Physics - Phenomenology · Physics 2010-12-23 Philippe Brax , Clare Burrage

In the chameleon mechanism, a field (typically scalar) has a mass that depends on the matter density of the environment: the larger is the matter density, the larger is the mass of the chameleon. We briefly review some aspects of…

General Relativity and Quantum Cosmology · Physics 2016-02-12 Andrea Zanzi

In conventional approach to the chameleon mechanism, by assuming a static and spherically symmetric solutions in which matter density and chameleon field are given by $\rho=\rho(r)$ and $\phi=\phi(r)$, it has been shown that mass of…

General Relativity and Quantum Cosmology · Physics 2015-06-05 H. Farajollahi , A. Salehi

Light scalar fields can drive the accelerated expansion of the universe. Hence, they are obvious dark energy candidates. To make such models compatible with tests of General Relativity in the solar system and "fifth force" searches on…

Instrumentation and Methods for Astrophysics · Physics 2014-11-07 S. Baum , G. Cantatore , D. H. H. Hoffmann , M. Karuza , Y. K. Semertzidis , A. Upadhye , K. Zioutas

Chameleons are a well motivated scalar field that might explain the observed late time accelerated expansion of the universe. Chameleons possess the interesting property that their mass, and hence interaction range, is dependent on the…

Cosmology and Nongalactic Astrophysics · Physics 2013-09-27 Robert Poltis

A scalar field is a favorite candidate for the particle responsible for dark energy. However, few theoretical means exist that can simultaneously explain the observed acceleration of the Universe and evade tests of gravity. The chameleon…

High Energy Physics - Experiment · Physics 2019-08-15 Jason H. Steffen

Chameleon dark energy is a matter-coupled scalar field which hides its fifth forces locally by becoming massive. We estimate torsion pendulum constraints on the residual fifth forces due to models with gravitation-strength couplings.…

High Energy Physics - Phenomenology · Physics 2012-12-03 Amol Upadhye

In chameleon field theories a scalar field can couple to matter with gravitational strength and still evade local gravity constraints due to a combination of self-interactions and the couplings to matter. Originally, these theories were…

Cosmology and Nongalactic Astrophysics · Physics 2011-05-02 David F. Mota , Hans A. Winther

Starting from the assumption that the present accelerated expansion of the Universe is driven by a chameleon scalar field, the function describing a direct coupling between the matter content of the Universe and the scalar field is derived…

Solar and Stellar Astrophysics · Physics 2012-09-21 Vladimir Folomeev

We have investigated a brane world model in which the gravitational field in the bulk is described both by a metric tensor and a minimally coupled scalar field. This scalar field is taken to be a chameleon with an appropriate potential…

General Relativity and Quantum Cosmology · Physics 2017-12-12 Y. Bisabr , F. Ahmadi

The chameleon mechanism appearing in massive tensor-scalar theory of gravity can effectively reduce the nonminimal coupling between the scalar field and matter. This mechanism is invoked to reconcile cosmological data requiring introduction…

General Relativity and Quantum Cosmology · Physics 2017-02-22 A. Hees , A. Füzfa

Certain scalar-tensor theories exhibit the so-called chameleon mechanism, whereby observational signatures of scalar fields are hidden by a combination of self-interactions and interactions with ambient matter. Not all scalar-tensor…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-21 Philippe Brax , Carsten van de Bruck , David F. Mota , Nelson J. Nunes , Hans A. Winther

We show that the chameleon scalar field can drive the current phase of cosmic acceleration for a large class of scalar potentials that are also consistent with local tests of gravity. These provide explicit realizations of a quintessence…

Theories of dark energy require a screening mechanism to explain why the associated scalar fields do not mediate observable long range fifth forces. The archetype of this is the chameleon field. Here we show that individual atoms are too…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-31 Clare Burrage , Edmund J. Copeland , E. A. Hinds

The physics of the "dark energy" that drives the current cosmological acceleration remains mysterious, and the dark sector may involve new light dynamical fields. If these light scalars couple to matter, a screening mechanism must prevent…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-15 Adrienne L. Erickcek , Neil Barnaby , Clare Burrage , Zhiqi Huang

The chameleon scalar field is considered as a possible cause of accelerated expansion of the Universe. The chameleon field induces an interaction potential between a particle and a massive body. Previous experiments with falling cold…

Nuclear Experiment · Physics 2015-06-18 Yu. N. Pokotilovski

The chameleon model is a scalar field theory with a screening mechanism that explains how a cosmologically relevant light scalar can avoid the constraints of intra-solar-system searches for fifth-forces. The chameleon is a popular dark…

Cosmology and Nongalactic Astrophysics · Physics 2016-11-23 Clare Burrage , Jeremy Sakstein

Recent developments in the theory of extra dimensions have opened up avenues to confront such theories with cosmological tests. We discuss a brane-world model with a bulk scalar field, motivated by supergravity. The low-energy effective…

Astrophysics · Physics 2009-11-10 A. -C. Davis , Ph. Brax , C. van de Bruck
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