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相关论文: Non-minimally coupled tachyon field with Noether s…

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A model for a spatially flat homogeneous and isotropic Universe whose gravitational sources are a pressureless matter field and a tachyon field non-minimally coupled to the gravitational field is analyzed. Noether symmetry is used to find…

广义相对论与量子宇宙学 · 物理学 2010-04-30 Rudinei C. de Souza , Gilberto M. Kremer

An action of general form is proposed for a Universe containing matter, radiation and dark energy. The latter is interpreted as a tachyon field non-minimally coupled to the scalar curvature. The Palatini approach is used when varying the…

广义相对论与量子宇宙学 · 物理学 2017-04-28 Lucas Gardai Collodel , Gilberto Medeiros Kremer

We analyse a scalar field non-minimally coupled to gravity in the context of a Universe described by the flat Friedmann-Robertson-Walker (F-R-W) metric. The adopted model comprises a Universe filled by the scalar field and standard matter…

广义相对论与量子宇宙学 · 物理学 2013-09-16 Rudinei C. de Souza , Raíla André , Gilberto M. Kremer

A model for a flat homogeneous and isotropic Universe composed of dark energy, dark matter, neutrinos, radiation and baryons is analyzed. The fields of dark matter and neutrinos are supposed to interact with the dark energy. The dark energy…

广义相对论与量子宇宙学 · 物理学 2008-11-26 G. M. Kremer

A cosmological model where a fermion field is non-minimally coupled with the gravitational field is studied. By applying Noether symmetry the possible functions for the potential density of the fermion field and for the coupling are…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Rudinei C. de Souza , Gilberto M. Kremer

This study explores the plausibility of an interacting tachyonic scalar, homogeneous in nature, as a promising candidate for dynamic dark energy, offering insights into the observed accelerated expansion of the universe. The…

广义相对论与量子宇宙学 · 物理学 2025-07-16 Tanisha Joshi , S. D Pathak

In this work we investigate the evolution of a Universe consisted of a scalar field, a dark matter field and non-interacting baryonic matter and radiation. The scalar field, which plays the role of dark energy, is non-minimally coupled to…

广义相对论与量子宇宙学 · 物理学 2007-05-23 J. B. Binder , G. M. Kremer

We use Noether symmetry approach to find spherically symmetric static solutions of the non-minimally coupled electromagnetic fields to gravity. We construct the point-like Lagrangian under the spherical symmetry assumption. Then we…

广义相对论与量子宇宙学 · 物理学 2020-07-28 Özcan Sert , Fatma Çeliktaş

In the framework of scalar-tensor gravity, we consider non-flat interacting quintessence cosmology where a scalar field is interacting with dark matter. Such a scalar field can be a standard or a phantom one. We use the Noether Symmetry…

广义相对论与量子宇宙学 · 物理学 2023-07-06 Ester Piedipalumbo , Stefano Vignolo , Pasquale Feola , Salvatore Capozziello

A detailed dynamical analysis of the tachyonic teleparallel dark energy model, in which a non-canonical scalar field (tachyon field) is non-minimally coupled to gravitation, is performed. It is found that, when the non-minimal coupling is…

广义相对论与量子宇宙学 · 物理学 2013-09-06 G. Otalora

We consider a model where a light scalar field (with mass $\lesssim 30\, {\rm eV}$), conjectured to be dark matter, has a non-minimal coupling to gravity. In the non-relativistic limit, this new coupling introduces a self-interaction term…

宇宙学与河外天体物理 · 物理学 2021-06-24 Lingyuan Ji

Toy cosmological models based on non-minimal coupling between gravity and scalar dilaton-like field are presented in the framework of Palatini formalism. They have the following property: preceding to a given cosmological epoch is a dark…

广义相对论与量子宇宙学 · 物理学 2008-12-24 A. Borowiec

The paper deals with a non--minimally coupled scalar field in the background of homogeneous but anisotropic Kantowski--Sachs space--time model. The form of the coupling function of the scalar field with gravity and the potential function of…

广义相对论与量子宇宙学 · 物理学 2018-05-23 Sourav Dutta , Muthusamy Lakshmanan , Subenoy Chakraborty

In this paper we consider Tachyonic scalar field as dark energy with interaction between components in the case of variable $G$ and $\Lambda$. We assume a flat Universe with specific form of scale factor and study cosmological parameters…

广义相对论与量子宇宙学 · 物理学 2015-02-03 J. Sadeghi , M. Khurshudyan , M. Hakobyan , H. Farahani

In this work it is investigated general models with interactions between two canonical scalar fields and between one non-canonical (tachyon-type) and one canonical scalar field. The potentials and couplings to the gravity are selected…

广义相对论与量子宇宙学 · 物理学 2013-10-15 Rudinei C. de Souza , Gilberto M. Kremer

In this work it is investigated the evolution of a Universe where a scalar field, non-minimally coupled to space-time curvature, plays the role of quintessence and drives the Universe to a present accelerated expansion. A non-relativistic…

广义相对论与量子宇宙学 · 物理学 2009-11-11 J. B. Binder , G. M. Kremer

The existence of dark energy is essential to explain the cosmic accelerated expansion. We consider a homogenous interacting tachyonic scalar field as a possible candidate for the dynamical dark energy. The interaction between the tachyonic…

广义相对论与量子宇宙学 · 物理学 2023-05-02 V K Ojha , Adithya A Rao , S D Pathak

We study a tachyon model with non-minimal derivative coupling to gravity in the Friedmann-Robertson-Walker flat cosmology. We propose the special re-definition of the tachyon field which allows us to represent tachyon field equation…

广义相对论与量子宇宙学 · 物理学 2012-09-13 V. K. Shchigolev , M. P. Rotova

We show that dark energy and dark matter can be described simultaneously by ordinary Einstein gravity interacting with a single scalar field provided the scalar field Lagrangian couples in a symmetric fashion to two different spacetime…

广义相对论与量子宇宙学 · 物理学 2016-11-29 Eduardo Guendelman , Emil Nissimov , Svetlana Pacheva

We present a detailed study of cosmological effects of homogeneous tachyon matter coexisting with non-relativistic matter and radiation, concentrating on the inverse square potential and the exponential potential for the tachyonic scalar…

天体物理学 · 物理学 2011-05-05 J. S. Bagla , H. K. Jassal , T. Padmanabhan
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