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相关论文: Solar system and equivalence principle constraints…

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Experiments on the violation of equivalence principle (EP) and solar system give a number of constraints in which any modified gravity model must satisfy them. We study these constraints on a kind of $f(R)$ gravity as $f(R) = R(1\pm…

广义相对论与量子宇宙学 · 物理学 2014-01-20 Kh. Saaidi , A. Aghamohammadi

We investigate the solar-system constraint on the f(R) theory of modified gravity with chameleon mechanism, where f(R) represents the deviation from general relativity in the gravity action. We obtain a stringent bound to a general,…

广义相对论与量子宇宙学 · 物理学 2011-08-09 Je-An Gu , Wei-Ting Lin

We analyse f(R) modifications of Einstein's gravity as dark energy models in the light of their connection with chameleon theories. Formulated as scalar-tensor theories, the f(R) theories imply the existence of a strong coupling of the…

天体物理学 · 物理学 2009-02-23 Philippe Brax , Carsten van de Bruck , Anne-Christine Davis , Douglas J. Shaw

Recently, a model $f(R)$ theory is proposed \cite{recent} which is cosmologically viable and distinguishable from $\Lambda$CDM. We use chameleon mechanism to investigate viability of the model in terms of Solar System experiments.

广义相对论与量子宇宙学 · 物理学 2010-01-15 Yousef Bisabr

Using a novel and self-consistent approach that avoids the scalar-tensor identification in the Einstein frame, we reanalyze the viability of f(R) gravity within the context of solar-system tests. In order to do so, we depart from a simple…

广义相对论与量子宇宙学 · 物理学 2020-03-06 Carolina Negrelli , Lucila Kraiselburd , Susana J. Landau , Marcelo Salgado

The $f(R)$ gravity can be cast into the form of a scalar-tensor theory, and scalar degree of freedom can be suppressed in high-density regions by the chameleon mechanism. In this article, for the general $f(R)$ gravity, using a…

宇宙学与河外天体物理 · 物理学 2018-01-04 Tan Liu , Xing Zhang , Wen Zhao

In this paper, we revisit the solar system tests of f(R) gravity. When the Sun sits in a vacuum, the field f' is light, which leads to a metric different from the observations. We reobtain this result in a simpler way by directly focusing…

宇宙学与河外天体物理 · 物理学 2014-03-24 Jun-Qi Guo

In chameleon $f(R)$-gravity, the fifth force will lead to `upturns' in galaxy rotation curves near the screening radius. The location of the upturn depends on the cosmic background value of the scalar field $f_{R0}$, as well as the mass,…

宇宙学与河外天体物理 · 物理学 2019-08-06 Aneesh P. Naik , Ewald Puchwein , Anne-Christine Davis , Debora Sijacki , Harry Desmond

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 show that Solar System tests can place very strong constraints on K-mouflage models of gravity, which are coupled scalar field models with nontrivial kinetic terms that screen the fifth force in regions of large gravitational…

宇宙学与河外天体物理 · 物理学 2015-07-28 Alexandre Barreira , Philippe Brax , Sebastien Clesse , Baojiu Li , Patrick Valageas

Light scalar fields are expected to arise in theories of high energy physics (such as string theory), and find phenomenological motivations in dark energy, dark matter, or neutrino physics. However, the coupling of light scalar fields to…

宇宙学与河外天体物理 · 物理学 2015-05-30 R. Pourhasan , N. Afshordi , R. B. Mann , A. C. Davis

We search for viable f(R) theories of gravity, making use of the equivalence between such theories and scalar-tensor gravity. We find that models can be made consistent with solar system constraints either by giving the scalar a high mass…

天体物理学 · 物理学 2008-11-26 Thomas Faulkner , Max Tegmark , Emory F. Bunn , Yi Mao

Chameleon mechanism appearing in massive tensor-scalar theory of gravity can effectively reduce locally the non-minimal coupling between the scalar field and matter. This mechanism is invoked to reconcile large-scale departures from general…

广义相对论与量子宇宙学 · 物理学 2015-03-19 A. Hees , A. Füzfa

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

There is a conformal equivalence between power law $f(R)$ theories and scalar field theories in which the scalar degree of freedom evolves under the action of an exponential potential function. In the scalar field representation there is a…

广义相对论与量子宇宙学 · 物理学 2014-11-21 Yousef Bisabr

The Solar System bounds on R^n gravity are often ignored in the literature by invoking the chameleon mechanism. We show that in order for the latter to work, the exponent n must be ridicolously close to unity and, therefore, these theories…

广义相对论与量子宇宙学 · 物理学 2011-07-08 Valerio Faraoni

Since last two decades $f(R)$ gravity theory has been extensively used as a serious alternative of general relativity to mimic the effects of dark energy. The theory presents a Yukawa correction to Newtonian gravitational potential, acting…

广义相对论与量子宇宙学 · 物理学 2025-05-02 Debojit Paul , Sanjeev Kalita

Future space-based tests of relativistic gravitation-laser ranging to Phobos, accelerometers in orbit, and optical networks surrounding Earth-will constrain the theory of gravity with unprecedented precision by testing the inverse-square…

宇宙学与河外天体物理 · 物理学 2018-03-28 Jeremy Sakstein

In most studies of equivalence principle violation by solar system bodies, it is assumed that the ratio of gravitational to inertial mass for a given body deviates from unity by a parameter Delta which is proportional to its gravitational…

广义相对论与量子宇宙学 · 物理学 2009-12-30 J. M. Overduin

We show that, as a result of non-linear self-interactions, it is feasible, at least in light of the bounds coming from terrestrial tests of gravity, measurements of the Casimir force and those constraints imposed by the physics of compact…

高能物理 - 唯象学 · 物理学 2008-11-26 David F. Mota , Douglas J. Shaw
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