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相关论文: Tracker fields from nonminimally coupled theory

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The relationship between symmetry fields and first integrals of divergence-free vector fields is explored in three dimensions in light of its relevance to plasma physics and magnetic confinement fusion. A Noether-type Theorem is known: for…

微分几何 · 数学 2023-06-07 David Perrella , Nathan Duignan , David Pfefferlé

All degrees of freedom related to the torsion scalar can be explored by analysing, the $f(T,T_G)$ gravity formalism where, $T$ is a torsion scalar and $T_G$ is the teleparallel counterpart of the Gauss-Bonnet topological invariant term. The…

广义相对论与量子宇宙学 · 物理学 2023-03-27 S. A. Kadam , B. Mishra , Jackson Levi Said

A general approach to find out exact cosmological solutions in f(R)-gravity is discussed. Instead of taking into account phenomenological models, we assume, as a physical criterium, the existence of Noether symmetries in the cosmological…

广义相对论与量子宇宙学 · 物理学 2010-02-10 Salvatore Capozziello , Antonio De Felice

The coupling of gravity to a scalar field raises a number of interesting questions of principle since the usual minimal coupling obtained by replacing ordinary derivatives with covariant derivatives is not available -- they are the same…

广义相对论与量子宇宙学 · 物理学 2011-10-26 Y. N. Srivastava , J. Swain , A. Widom

In this paper we propose a quintessence model with the potential $V(\Phi )=V_{o}[ \sinh {(\alpha \sqrt{\kappa_{o}}\Delta \Phi})] ^{\beta}$, which asymptotic behavior corresponds to an inverse power-law potential at early times and to an…

天体物理学 · 物理学 2010-04-06 L. A. Urena-Lopez , T. Matos

A common property of popular models of quintessence dark energy is the convergence to a common solution from a large range of the initial conditions. We re-examine the popular inverse power-law model of quintessence (where the common…

天体物理学 · 物理学 2009-11-07 James P. Kneller , Louis E. Strigari

Quintessence field is a widely-studied candidate of dark energy. There is "tracker solution" in quintessence models, in which evolution of the field $\phi$ at present times is not sensitive to its initial conditions. When the energy density…

天体物理学 · 物理学 2014-11-18 Mingxing Luo , Qiping Su

We consider curvature-teleparallel $F(R,T)$ gravity, where the gravitational Lagrangian density is given by an arbitrary function of the Ricci scalar $R$ and the torsion scalar $T$. Using the Noether Symmetry Approach, we show that the…

广义相对论与量子宇宙学 · 物理学 2015-10-21 Salvatore Capozziello , Mariafelicia De Laurentis , Ratbay Myrzakulov

We have shown that a particular class of non-local free field theory has conformal symmetry in arbitrary dimensions. Using the local field theory counterpart of this class, we have found the Noether currents and Ward identities of the…

高能物理 - 理论 · 物理学 2015-05-27 M. A. Rajabpour

In the framework of f(R) scalar-tensor cosmology, we use the Noether symmetry approach to find the cosmological models consistent with the Noether symmetry. We obtain the functions f(R) and H(a), or the corresponding differential equations,…

广义相对论与量子宇宙学 · 物理学 2015-05-21 F. Darabi , S. Asgharinya

We discuss an extended Teleparallel gravity models comprising functions of scalar invariants constructed by torsion, torsion Gauss-Bonnet and boundary terms. We adopt the Noether Symmetry Approach to select the functional forms, the first…

广义相对论与量子宇宙学 · 物理学 2019-05-22 Sebastian Bahamonde , Ugur Camci , Salvatore Capozziello

The $f(R)$ theory of gravity can be expressed as a scalar tensor theory with a scalar degree of freedom $\phi$. By a conformal transformation, the action and its Gibbons-York-Hawking boundary term are written in the Einstein frame and the…

广义相对论与量子宇宙学 · 物理学 2019-11-27 Roger A. Hurtado , Robel Arenas

The issues of quintessence and cosmic acceleration can be discussed in the framework of theories which do not include necessarily scalar fields. It is possible to define pressure and energy density for new components considering effective…

天体物理学 · 物理学 2008-11-26 S. Capozziello , S. Carloni , A. Troisi

We study the evolution of a two dimensional minisuperspace cosmological model in classical and quantum levels by the Noether symmetry approach. The phase space variables turn out to correspond to the scale factor of a…

广义相对论与量子宇宙学 · 物理学 2012-01-23 Babak Vakili , Farhad Khazaie

We consider the two scalar field cosmology in a FRW spatially flat spacetime where the scalar fields interact both in the kinetic part and the potential. We apply the Noether point symmetries in order to define the interaction of the scalar…

广义相对论与量子宇宙学 · 物理学 2014-09-09 Andronikos Paliathanasis , Michael Tsamparlis

The purpose of this work is to discuss how matter fields are coupled to gravity within the framework of General Relativity. Our particular focus here is on the coupling of scalar field models. In a first step, we suggest a new method for…

广义相对论与量子宇宙学 · 物理学 2026-04-29 Joshua Ritchie

General cosmological models with spinor and scalar fields playing the role of gravitational sources are analyzed. The Noether symmetry approach is taken as a criterion to constrain the undefined potentials and couplings of the generic…

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

We consider generic models of quintessence and we investigate the influence of massive neutrino matter with field-dependent masses on the matter power spectrum. In case of minimally coupled neutrino matter, we examine the effect in tracker…

宇宙学与河外天体物理 · 物理学 2016-01-28 Chao-Qiang Geng , Chung-Chi Lee , R. Myrzakulov , M. Sami , Emmanuel N. Saridakis

A didactic and systematic derivation of Noether point symmetries and conserved currents is put forward in special relativistic field theories, without a priori assumptions about the transformation laws. Given the Lagrangian density, the…

综合物理 · 物理学 2016-03-17 Fernando Haas

We search for spherically symmetric solutions of f(R) theories of gravity via the Noether Symmetry Approach. A general formalism in the metric framework is developed considering a point-like f(R)-Lagrangian where spherical symmetry is…

广义相对论与量子宇宙学 · 物理学 2008-11-26 S. Capozziello , A. Stabile , A. Troisi