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相关论文: Anisotropic Scalar Field Dark Energy with a Disfor…

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In this work we consider a cosmological model in which dark energy is portrayed by a canonical scalar field which is allowed to couple to the other species by means of a disformal transformation of the metric. We revisit the current…

广义相对论与量子宇宙学 · 物理学 2020-04-06 Elsa M. Teixeira , Ana Nunes , Nelson J. Nunes

We study the dynamics of the universe with a scalar field and an SU(2) non-Abelian Gauge (Yang-Mills) field. The scalar field has an exponential potential and the Yang-Mills field is coupled to the scalar field with an exponential function…

宇宙学与河外天体物理 · 物理学 2013-04-09 Kei-ichi Maeda , Kei Yamamoto

Interactions between dark matter and dark energy, allowing both conformal and and disformal couplings, are studied in detail. We discuss the background evolution, anisotropies in the cosmic microwave background and large scale structures.…

广义相对论与量子宇宙学 · 物理学 2015-06-23 C. van de Bruck , J. Morrice

Disformal transformations have proven to be very useful to devise models of the dark sector. In the present paper we apply such transformation to a single scalar field theory as a way to drive the field into a slow roll phase. The canonical…

宇宙学与河外天体物理 · 物理学 2012-06-04 M. Zumalacarregui , T. S. Koivisto , D. F. Mota , P. Ruiz-Lapuente

Many theories of dark energy and modified gravity give rise to scalar fields that couple derivatively to the energy momentum tensor of matter. This is known as disformal coupling. I will show that laboratory searches for axions are ideally…

高能物理 - 唯象学 · 物理学 2013-01-09 Clare Burrage

Disformally coupled, light scalar fields arise in many of the theories of dark energy and modified gravity that attempt to explain the accelerated expansion of the universe. They have proved difficult to constrain with precision tests of…

高能物理 - 唯象学 · 物理学 2015-08-26 Philippe Brax , Clare Burrage , Christoph Englert

Non-Abelian gauge fields are traditionally not coupled to torsion due to violation of gauge invariance. However, it is possible to couple torsion to Yang-Mills fields while maintaining gauge invariance provided one accepts that the gauge…

广义相对论与量子宇宙学 · 物理学 2007-05-23 C. Mukku

An anisotropic cosmological model with a gauge field, presented by spatially homogeneous SU(2)-symmetric Yang-Mills potentials, is considered. Bianchi-I model with axial symmetry is analyzed; a new exact solution, which describes the early…

广义相对论与量子宇宙学 · 物理学 2025-05-06 Alexander B. Balakin , Gleb B. Kiselev

Cosmology with a three-form field interacting with cold dark matter is considered. In particular, the mass of the dark matter particles is assumed to depend upon the amplitude of the three-form field invariant. In comparison to coupled…

宇宙学与河外天体物理 · 物理学 2015-06-12 Tomi S. Koivisto , Nelson J. Nunes

We establish a nonminimal Einstein-Yang-Mills-Higgs model, which contains six coupling parameters. First three parameters relate to the nonminimal coupling of non-Abelian gauge field and gravity field, two parameters describe the so-called…

广义相对论与量子宇宙学 · 物理学 2008-11-07 A. B. Balakin , H. Dehnen , A. E. Zayats

We revisit the dynamics of the axial coupling between many N-flatons and an Abelian gauge field, with special attention to its statistically anisotropic signal. The anisotropic power spectrum of curvature perturbations associated to the…

宇宙学与河外天体物理 · 物理学 2013-10-02 Federico R. Urban

We consider a cosmology in which dark matter and a quintessence scalar field responsible for the acceleration of the Universe are allowed to interact. Allowing for both conformal and disformal couplings, we perform a global analysis of the…

宇宙学与河外天体物理 · 物理学 2017-02-22 Carsten van de Bruck , Jurgen Mifsud , Jack Morrice

We discuss the possibility that dark energy arises from a strongly-coupled Higgs-Yang-Mills set of interacting fields in the non-perturbative regime. We choose the simplest $SU(2)$ representation, which is compatible with the Cosmological…

宇宙学与河外天体物理 · 物理学 2025-05-20 Marco Frasca , Anish Ghoshal , Massimilano Rinaldi

We discuss cosmological model with homogeneous and isotropic Yang-Mills field non-minimally coupled to gravity through an effective mass term. In this model conformal symmetry is violated which leads to possibility of inflationary…

高能物理 - 理论 · 物理学 2013-12-24 Evgeny A. Davydov , Dmitry V. Gal'tsov

It is shown that extensions to General Relativity, which introduce a strongly coupled scalar field, can be viable if the interaction has a non-conformal form. Such disformal coupling depends upon the gradients of the scalar field. Thus, if…

宇宙学与河外天体物理 · 物理学 2012-12-11 Tomi S. Koivisto , David F. Mota , Miguel Zumalacarregui

Scalar fields coupled to dark matter by conformal or disformal transformations give rise to a general class of scalar-tensor theories which leads to a rich phenomenology in a cosmological setting. While this possibility has been studied…

广义相对论与量子宇宙学 · 物理学 2023-08-23 Gabriel Gómez

In this short review, I discuss basic qualitative characteristics of quantum non-Abelian gauge dynamics in the non-stationary background of the expanding Universe in the framework of the standard Einstein--Yang--Mills formulation. A brief…

广义相对论与量子宇宙学 · 物理学 2016-05-26 Roman Pasechnik

We study a theory in which the electromagnetic field is disformally coupled to a scalar field, in addition to a usual non-minimal electromagnetic coupling. We show that disformal couplings modify the expression for the fine-structure…

宇宙学与河外天体物理 · 物理学 2015-12-16 Carsten van de Bruck , Jurgen Mifsud , Nelson J. Nunes

Non-Abelian dark gauge forces that do not couple directly to ordinary matter may be realized in nature. The minimal form of such a dark force is a pure Yang-Mills theory. If the dark sector is reheated in the early universe, it will be…

高能物理 - 唯象学 · 物理学 2018-05-02 Lindsay Forestell , David E. Morrissey , Kris Sigurdson

We discuss cosmological models involving homogeneous and isotropic Yang-Mills (YM) fields. Such models were proposed recently as an alternative to scalar models of cosmic acceleration. There exists a unique SU(2) YM configuration…

广义相对论与量子宇宙学 · 物理学 2011-03-22 Dmitry V. Gal'tsov , Evgeny A. Davydov
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