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相关论文: Light mass galileon and late time acceleration of …

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A new cosmological scenario driven by a slow rolling homogeneous scalar field whose exponential potential $V(\Phi)$ has a quadratic dependence on the field $\Phi$ in addition to the standard linear term is discussed. The derived equation of…

天体物理学 · 物理学 2009-11-11 F. C. Carvalho , J. S. Alcaniz , J. A. S. Lima , R. Silva

We study the cosmology of Galileon modified gravity models in the linear perturbation regime. We derive the fully covariant and gauge invariant perturbed field equations using two different methods, which give consistent results, and solve…

宇宙学与河外天体物理 · 物理学 2013-01-22 Alexandre Barreira , Baojiu Li , Carlton Baugh , Silvia Pascoli

We construct a consistent model of Galileon scalar electrodynamics. The model satisfies three essential requirements: (1) The action contains higher-order derivative terms, and obey the Galilean symmetry, (2) Equations of motion also…

高能物理 - 理论 · 物理学 2020-03-25 Ashu Kushwaha , S. Shankaranarayanan

The main aim of this paper is to provide cosmological constraints on the Multi Scalar Field Dark Matter model (MSFDM), in which we assume the dark matter is made up of different ultra-light scalar fields. As a first approximation, we…

宇宙学与河外天体物理 · 物理学 2022-12-05 L. O. Téllez-Tovar , Tonatiuh Matos , J. Alberto Vázquez

It is an accepted practice in cosmology to invoke a scalar field with potential $V(\phi)$ when observed evolution of the universe cannot be reconciled with theoretical prejudices. Since one function-degree-of-freedom in the expansion factor…

高能物理 - 理论 · 物理学 2008-11-26 T. Padmanabhan

Considering the Friedmann--Lema\^{i}tre--Robertson--Walker (FLRW) metric and the Einstein scalar field system as an underlying gravitational model to construct fractional cosmological models has interesting implications in both classical…

广义相对论与量子宇宙学 · 物理学 2024-07-26 S. M. M. Rasouli , S. Cheraghchi , P. V. Moniz

The mystery of dark energy suggests that there is new gravitational physics on long length scales. Yet light degrees of freedom in gravity are strictly limited by Solar System observations. We can resolve this apparent contradiction by…

宇宙学与河外天体物理 · 物理学 2015-03-17 Mark Wyman

We investigate a possible connection between Galileon gravity and teleparallel gravity. We also propose a new type of second order cosmological lagrangian and study a some of its properties.

广义相对论与量子宇宙学 · 物理学 2015-06-15 P. Tretyakov

We investigate the time evolution of the gravitational potential Phi for a special class of non-adiabatic Unified Dark matter Models described by scalar field lagrangians. These models predict the same background evolution as in the…

宇宙学与河外天体物理 · 物理学 2012-08-14 Oliver F. Piattella , Daniele Bertacca

The evidence of the acceleration of universe at present time has lead to investigate modified theories of gravity and alternative theories of gravity, which are able to explain acceleration from a theoretical viewpoint without the need of…

高能物理 - 理论 · 物理学 2011-05-05 Gianluca Allemandi , Andrzej Borowiec , Mauro Francaviglia

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

There can arise ubiquitous ultra-light scalar fields in the Universe, such as the pseudo-Goldstone bosons from the spontaneous breaking of an approximate symmetry, which can make a partial contribution to the dark matter and affect the…

高能物理 - 唯象学 · 物理学 2015-06-18 Kenji Kadota , Yi Mao , Kiyomoto Ichiki , Joseph Silk

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

The recent progress in the study of Galileons, i.e. equations of second order with an action invariant under a Galilean transformation is related to work on `Universal Field Equations' \cite{dbfgov} which are second order equations arising…

高能物理 - 理论 · 物理学 2011-06-28 David Fairlie

In this investigation, we perform an observational statistical analysis in the theory of $ f(R, L_m) $ gravity. The proposed theoretical model is based on the Ricci scalar's non-linear contribution. We use a distinct parameterization for…

广义相对论与量子宇宙学 · 物理学 2024-08-30 J. K. Singh , Shaily , Akanksha Singh , Harshna Balhara , Joao R. L. Santos

We study the most general cosmological model with real scalar field which is minimally coupled to gravity. Our calculations are based on Friedmann-Lemaitre-Robertson-Walker (FLRW) background metric. Field equations consist of three…

广义相对论与量子宇宙学 · 物理学 2023-03-22 Medine Ildes , Metin Arik

In this study, we explored late-time cosmology within an extended class of theories based on $f(Q, L_m)$ gravity. This theory generalizes $f(Q)$ gravity by incorporating a non-minimal coupling between the non-metricity $Q$ and the matter…

宇宙学与河外天体物理 · 物理学 2024-10-07 Kairat Myrzakulov , M. Koussour , O. Donmez , A. Cilli , E. Güdekli , J. Rayimbaev

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

We describe a new type of gravity-matter models where gravity couples in a non-conventional way to two distinct scalar fields providing a unified Lagrangian action principle description of: (a) the evolution of both "early" and "late"…

广义相对论与量子宇宙学 · 物理学 2017-07-25 Eduardo Guendelman , Emil Nissimov , Svetlana Pacheva

We considered the phantom cosmology with a lagrangian $\displaystyle L=\frac{1}{\eta}[1-\sqrt{1+\eta g^{\mu\nu}\phi_{, \mu}\phi_{, \nu}}]-u(\phi)$, which is original from the nonlinear Born-Infeld type scalar field with the lagrangian…

高能物理 - 理论 · 物理学 2007-05-23 Wei Fang , H. Q. Lu , Z. G. Huang , K. F. Zhang