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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,…

天体物理学 · 物理学 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…

综合物理 · 物理学 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…

高能物理 - 唯象学 · 物理学 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…

广义相对论与量子宇宙学 · 物理学 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…

广义相对论与量子宇宙学 · 物理学 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…

天体物理仪器与方法 · 物理学 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…

宇宙学与河外天体物理 · 物理学 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…

高能物理 - 实验 · 物理学 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.…

高能物理 - 唯象学 · 物理学 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…

宇宙学与河外天体物理 · 物理学 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…

太阳与恒星天体物理 · 物理学 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…

广义相对论与量子宇宙学 · 物理学 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…

广义相对论与量子宇宙学 · 物理学 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…

宇宙学与河外天体物理 · 物理学 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…

天体物理学 · 物理学 2008-11-26 Philippe Brax , Carsten van de Bruck , Anne-Christine Davis , Justin Khoury , Amanda Weltman

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…

宇宙学与河外天体物理 · 物理学 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…

宇宙学与河外天体物理 · 物理学 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…

核实验 · 物理学 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…

宇宙学与河外天体物理 · 物理学 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…

天体物理学 · 物理学 2009-11-10 A. -C. Davis , Ph. Brax , C. van de Bruck
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