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We revisit the concept of turnaround radius in cosmology, in the context of modified gravity. While preliminary analyses were limited to scalar-tensor/$F(R)$ gravity, we extend the definition and the study of this quantity to a much broader…

广义相对论与量子宇宙学 · 物理学 2018-07-11 Shin'ichi Nojiri , Sergei D. Odintsov , Valerio Faraoni

Deformed Reissner-Nordstr\"om, as well as Reissner-Nordstr\"om de Sitter, solutions are obtained in a noncommutative gauge theory of gravitation. The gauge potentials (tetrad fields) and the components of deformed metric are calculated to…

高能物理 - 理论 · 物理学 2008-11-26 M. Chaichian , M. R. Setare , A. Tureanu , G. Zet

We study a recent proposed Ricci-inverse gravity, which is a very novel type of fourth-order gravity. In particular, we are able to figure out both isotropically and anisotropically inflating universes to this model. More interestingly,…

广义相对论与量子宇宙学 · 物理学 2021-05-20 Tuan Q. Do

The effects implied for the structure of compact objects by the modification of General Relativity produced by the generalization of the Lagrangian density to the form f(R)=R+\alpha R^2, where R is the Ricci curvature scalar, have been…

宇宙学与河外天体物理 · 物理学 2013-01-24 Mariana Orellana , Federico García , Florencia Anabella Teppa Pannia , Gustavo Esteban Romero

A recently proposed theory of modified gravity with an explicit ``anomalous'' coupling of the Ricci curvature to matter is discussed, and an inequality is derived which expresses a necessary and sufficient condition to avoid the notorius…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Valerio Faraoni

The Legendre transformation method, applied in 1987 to deal with purely metric gravitational Lagrangians with nonlinear dependence on the Ricci tensor, is extended to metric-affine models and is shown to provide a concise and insightful…

广义相对论与量子宇宙学 · 物理学 2016-09-21 Guido Magnano

In this paper we show how the covariant gauge invariant equations for the evolution of scalar, vector and tensor perturbations for a generic $f(R)$-gravity theory can be recast in order to exploit the power of dynamical system methodology.…

天体物理学 · 物理学 2008-12-12 Sante Carloni , Kishore N. Ananda , Peter K. S. Dunsby , Mohamed E. S. Abdelwahab

We generalize the scale invariant gravity by allowing a negative kinetic energy term for the classical scalar field. This gives birth to a new scalar-tensor theory of gravity, in which the scalar field is in fact an auxiliary field. For a…

高能物理 - 理论 · 物理学 2007-05-23 Shih-Yuin Lin , Kin-Wang Ng

We generalize the known equivalence between higher order gravity theories and scalar tensor theories to a new class of theories. Specifically, in the context of a first order or Palatini variational principle where the metric and connection…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Eanna E. Flanagan

We revisit the issue of the correct Lagrangian description of a perfect fluid (pressure versus minus energy density) in relation with modified gravity theories in which galactic luminous matter couples nonminimally to the Ricci scalar.…

星系天体物理 · 物理学 2010-04-23 Valerio Faraoni

An FLRW reduction of N=1 supergravity is troublesome since spatial isotropy prohibits a non-vanishing Rarita-Schwinger field. In view of this, we consider the quadratic form $\psi_m^{\ \alpha} \psi_{n \alpha}$ arising from a particular…

高能物理 - 理论 · 物理学 2025-10-24 Nephtalí Eliceo Martínez-Pérez , Cupatitzio Ramírez Romero

Recently Penrose, Sorkin and Woolgar have developed a new technique for proving the positive mass theorem in general relativity. We extend their result to produce a new inequality relating the mass, electric and scalar charges in theories…

广义相对论与量子宇宙学 · 物理学 2007-05-23 G. W. Gibbons , C. G. Wells

Dipole charge conservation forces isolated charges to be immobile fractons. These couple naturally to spatial two-index symmetric tensor gauge fields that resemble a spatial metric. We propose a spacetime Lorentz covariant version of dipole…

高能物理 - 理论 · 物理学 2024-03-12 Evangelos Afxonidis , Alessio Caddeo , Carlos Hoyos , Daniele Musso

An extension of unimodular Einsteinian gravity in the context of $F(R)$ gravities is used to construct a class of anisotropic evolution scenarios. In unimodular GR the determinant of the metric is constrained to be a fixed number or a…

广义相对论与量子宇宙学 · 物理学 2022-12-28 A. Costantini , E. Elizalde

We study the self-compactification of extra dimensions via higher curvature gravity, f(R), where f(R) is the generic function of the Ricci scalar R. First, we reduce pure f(R) theory to a scalar-tensor theory by a conformal transformation.…

高能物理 - 理论 · 物理学 2011-02-16 Beyhan Pulice , Sukru Hanif Tanyildizi

Scalar perturbations of Friedmann-Lemaitre cosmologies can be analyzed in a variety of ways using Einstein's field equations, the Ricci and Bianchi identities, or the conservation equations for the stress-energy tensor, and possibly…

广义相对论与量子宇宙学 · 物理学 2015-06-03 Claes Uggla , John Wainwright

We investigate brane world models in higher-derivative gravity theories where the gravitational Lagrangian is an arbitrary function of the Ricci scalar. Making use of the conformal equivalence of such gravity models and Einstein-Hilbert…

高能物理 - 唯象学 · 物理学 2009-11-11 M. Parry , S. Pichler , D. Deeg

We apply cosmological reconstruction methods to the $f(R,T)$ modified gravity, in its recently developed scalar-tensor representation. We do this analysis assuming a perfect fluid in a Friedmann-Lema\^{i}tre-Robsertson-Walker (FLRW)…

广义相对论与量子宇宙学 · 物理学 2024-07-24 Tiago B. Gonçalves , João Luís Rosa , Francisco S. N. Lobo

We investigate the cosmological reconstruction in modified f(R,T) gravity, where R is the Ricci scalar and T the trace of the stress-energy tensor. Special attention is attached to the case in which the function f is given by f (R, T) = f1…

宇宙学与河外天体物理 · 物理学 2015-05-28 M. J. S. Houndjo

We describe a new type of gravity-matter models where modified f(R)=R+R^2 gravity couples non-canonically to a scalar "inflaton", to the bosonic sector of the electroweak particle model and to a special nonlinear gauge field with a…

高能物理 - 理论 · 物理学 2019-03-27 Eduardo Guendelman , Emil Nissimov , Svetlana Pacheva