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Observational evidence implying the accelerated expansion of the universe has been the motivation to develop various classes of modified gravity theories. One of them uses the so-called "screening mechanism", which is successful in…

广义相对论与量子宇宙学 · 物理学 2019-11-18 Noshad Khosravi Largani , Mohammad Taghi Mirtorabi

The chameleon is a theorised scalar field that couples to matter and possess a screening mechanism, which weakens observational constraints from experiments performed in regions of higher matter density. One consequence of this screening…

广义相对论与量子宇宙学 · 物理学 2023-08-03 Chad Briddon , Clare Burrage , Adam Moss , Andrius Tamosiunas

We study the field profile of a scalar field $\phi$ that couples to a matter fluid (dubbed a chameleon field) in the relativistic gravitational background of a spherically symmetric spacetime. Employing a linear expansion in terms of the…

广义相对论与量子宇宙学 · 物理学 2010-04-14 Shinji Tsujikawa , Takashi Tamaki , Reza Tavakol

We investigate cosmological solutions of the chameleon model with a non-minimal coupling between the matter and the scalar field through a conformal factor with gravitational strength. By considering the spatially flat FLRW metric and the…

广义相对论与量子宇宙学 · 物理学 2023-11-01 Raziyeh Zaregonbadi , Nasim Saba , Mehrdad Farhoudi

Theories of modified gravity where light scalars with non-trivial self-interactions and non-minimal couplings to matter-chameleon and symmetron theories-dynamically suppress deviations from general relativity in the solar system. On other…

宇宙学与河外天体物理 · 物理学 2018-03-20 Clare Burrage , Jeremy Sakstein

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

Following work by Khoury and Weltman, we introduce a scalar field phi, the chameleon, which is conformally coupled to matter. That is, matter experiences a metric which is a conformal transform (parametrized by phi) of the Einstein metric.…

天体物理学 · 物理学 2007-05-23 T. P. Waterhouse

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

We derive analytic solutions of a chameleon scalar field $\phi$ that couples to a non-relativistic matter in the weak gravitational background of a spherically symmetric body, paying particular attention to a field mass $m_A$ inside of the…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Takashi Tamaki , Shinji Tsujikawa

We consider $f(R)$ modified gravity theory incorporating the chameleon mechanism to address galactic dynamics. By employing the metric formalism and utilizing a conformal transformation, we simplify the field equations and describe the…

广义相对论与量子宇宙学 · 物理学 2024-09-04 Gayatri Mohan , Umananda Dev Goswami

Aims. We investigated the gravitational effects of a scalar field within scalar-tensor gravity as an alternative to dark matter. Motivated by chameleon, symmetron and f(R)-gravity models, we studied a phenomenological scenario where the…

宇宙学与河外天体物理 · 物理学 2014-01-24 David F. Mota , Vincenzo Salzano , Salvatore Capozziello , Nicola R. Napolitano

We study the gravitational collapse of an overdensity of nonrelativistic matter under the action of gravity and a chameleon scalar field. We show that the spherical collapse model is modified by the presence of a chameleon field. In…

宇宙学与河外天体物理 · 物理学 2015-03-17 Ph. Brax , R. Rosenfeld , D. A. Steer

We investigate the dynamics and the phase-space evolution for the scalar nonmetricity cosmology with a Chameleon mechanism. In particular, we consider a spatially flat Friedmann--Lema\^{\i}tre--Robertson--Walker geometry and within the…

广义相对论与量子宇宙学 · 物理学 2024-07-09 Andronikos Paliathanasis

In this article we discuss some aspects of solar physics from the standpoint of the so-called chameleon fields (i.e. quantum fields, typically scalar, where the mass is an increasing function of the matter density of the environment).…

高能物理 - 唯象学 · 物理学 2016-04-05 Andrea Zanzi , Barbara Ricci

We analyse the phenomenology of a self-interacting scalar field in the context of the chameleon scenario originally proposed by Khoury and Weltman. In the absence of self-interactions, this type of scalar field can mediate long range…

广义相对论与量子宇宙学 · 物理学 2014-11-18 Hillary Sanctuary , Riccardo Sturani

Chameleon and similar (symmetron and dilation) theories of gravity can exhibit new and interesting features on cosmological scales whilst screening the modifications on small scales thereby satisfying solar system tests of general…

宇宙学与河外天体物理 · 物理学 2015-02-17 Jeremy Sakstein

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

Chameleon scalar fields can screen their associated fifth forces from detection by changing their mass with the local density. These models are an archetypal example of a screening mechanism, and have become an important target for both…

宇宙学与河外天体物理 · 物理学 2018-03-14 Clare Burrage , Edmund J. Copeland , Adam Moss , James A. Stevenson

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

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…

宇宙学与河外天体物理 · 物理学 2016-09-07 Clare Burrage , Edmund J. Copeland , James A. Stevenson
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