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相关论文: Non-minimal coupling inspires the Dirac cosmologic…

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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

We numerically construct compact stars in the scalar-tensor theory of gravity with non-minimal derivative coupling of a scalar field to the curvature and nonzero cosmological constant. There are two free parameters in this model of gravity:…

广义相对论与量子宇宙学 · 物理学 2025-04-08 P. E. Kashargin , A. A. Lebedev , S. V. Sushkov

This article surveys the noncommutative-geometric (NCG) approach to fundamental physics, in which geometry is encoded spectrally by a generalized Dirac operator and where dynamics arise from the spectral action. I review historically how…

高能物理 - 理论 · 物理学 2025-11-11 Ali H. Chamseddine

The idea that the seed primordial magnetic fields can be explained by the nonminimal coupling between gravitational and electromagnetic fields is discussed. The predicted values of the magnetic field of the spiral galaxies are in agreement…

广义相对论与量子宇宙学 · 物理学 2007-05-23 R. Opher , U. F. Wichoski

We consider the modified gravity non-minimally coupled with matter Lagrangian for the description of early-time and late-time universe. Such $F(R)$ ($F(G)$) gravity in the absence of non-minimal coupling is viable theory which passes the…

高能物理 - 理论 · 物理学 2008-11-26 Shin'ichi Nojiri , Sergei D. Odintsov , Petr V. Tretyakov

In Newtonian gravity, mass is an intrinsic property of matter while in general relativity (GR), mass is a contextual property of matter, i.e., matter can simultaneously possess two different values of mass when it is responsible for two…

综合物理 · 物理学 2019-01-30 W. M. Stuckey , Timothy McDevitt , A. K. Sten , Michael Silberstein

We consider f(R,T) modified theory of gravity in which, in general, the gravitational Lagrangian is given by an arbitrary function of the Ricci scalar and the trace of the energy-momentum tensor. We indicate that in this type of the theory,…

广义相对论与量子宇宙学 · 物理学 2016-10-05 Raziyeh Zaregonbadi , Mehrdad Farhoudi

Cosmological implications of a generalized Rastall theory where the non-conservation equation is promoted to accepts arbitrary functions of the Ricci scalar is considered. We have obtain the model parameters of the power-law ansatz…

广义相对论与量子宇宙学 · 物理学 2021-10-13 Shahab Shahidi

The "measurability" of the non-minimal coupling is discussed in the context of the effective field theory of gravity. Although there is no obvious motive for excluding a non-minimal scalar coupling from the theory, we conclude that for…

高能物理 - 理论 · 物理学 2009-10-31 A. Flachi , D. J. Toms

Spatially homogeneous models with a scalar field non-minimally coupled to the space-time curvature or to the ordinary matter content are analysed with respect to late-time asymptotic behaviour, in particular to accelerated expansion and…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Roger Bieli

It is pointed out that string-loop modifications of the low-energy matter couplings of the dilaton may provide a mechanism for fixing the vacuum expectation value of a massless dilaton in a way which is naturally compatible with existing…

高能物理 - 理论 · 物理学 2011-05-05 T. Damour , A. M. Polyakov

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

We study extended theories of gravity where nonminimal derivative couplings of the form $R^{kl}\phi_{, k}\phi_{, l}$ are present in the Lagrangian. We show how and why the other couplings of similar structure may be ruled out and then…

广义相对论与量子宇宙学 · 物理学 2017-10-04 S. Capozziello , G. Lambiase , H. -J. Schmidt

We consider the Weyl-Dirac theory within the framework of the weak field approximation and show that the resulting gravitational potential differs from that of Newtonian by a repulsive correction term increasing with distance. The scale of…

广义相对论与量子宇宙学 · 物理学 2010-11-19 S. Mirabotalebi , S. Jalalzadeh , S. Movahed , H. R. Sepangi

We address the challenge, commonly referred to as the cosmological averaging problem, of relating the large-scale evolution of an inhomogeneous universe to that predicted by a homogeneous matter distribution in theories of gravity with…

宇宙学与河外天体物理 · 物理学 2026-05-13 S. R. Pinto , P. P. Avelino

Modified gravity theories with a nonminimal coupling between curvature and matter offer a compelling alternative to dark energy and dark matter by introducing an explicit interaction between matter and curvature invariants. Two of the main…

广义相对论与量子宇宙学 · 物理学 2025-10-29 Francisco S. N. Lobo , Tiberiu Harko , Miguel A. S. Pinto

We discuss a class of exact solutions of a three-parameter non-minimally extended Einstein-Maxwell model, which are attributed to non-minimal magnetic monopoles of the Dirac type. We focus on the investigation of the gravitational field of…

广义相对论与量子宇宙学 · 物理学 2009-02-24 Alexander B. Balakin , Heinz Dehnen , Alexei E. Zayats

This paper explores the evolution of the over-dense region of dark matter in the presence of a non-minimally coupled scalar field which is used to model quintessence and phantom-like dark energy. We focus on algebraic coupling, where the…

广义相对论与量子宇宙学 · 物理学 2024-01-23 Priyanka Saha , Dipanjan Dey , Kaushik Bhattacharya

The coupling of antimatter to gravity is of general interest because of conceivable cosmological consequences ("surprises") related to dark energy and the cosmological constant. Here, we revisit the derivation of the gravitationally coupled…

高能物理 - 唯象学 · 物理学 2015-01-04 U. D. Jentschura

In this article, we examine the dynamical system of the $f(R,\mathcal{G})$ gravity model. This $f(R,G)$ model framework is composed of interactions between dark matter and scalar field through the linear coupling term. The key objective of…

广义相对论与量子宇宙学 · 物理学 2025-04-03 Shivani Sharma , R. Chaubey