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We investigate the scalar sector of linear cosmological perturbations in quadratic gravity. Working in the Einstein frame, we derive the equations of motion in a gauge-independent manner and express them in terms of three sets of…

广义相对论与量子宇宙学 · 物理学 2026-05-26 Adrian Palomares , Ying-li Zhang , Jinsu Kim

We revisit a scenario in which the cosmological constant is cancelled by the potential energy of a slowly evolving scalar field, or "cosmon". The cosmon's evolution is tied to the cosmological constant by a feedback mechanism. This feedback…

高能物理 - 唯象学 · 物理学 2011-05-12 Stephen M. Barr , Siew-Phang Ng , Robert J. Scherrer

As a sequel to (Berman, 2008a), we show that the rotation of the Universe can be dealt by generalised Gaussian metrics, defined in this paper. Robertson-Walker's metric has been employed with proper-time, in its standard applications; the…

综合物理 · 物理学 2009-11-13 Marcelo Samuel Berman

Taking a hint from Dirac's large number hypothesis, we note the existence of cosmic combined conservation laws that work to cosmologically long time. We thus modify or generalize Einstein's theory of general relativity with fixed…

广义相对论与量子宇宙学 · 物理学 2014-11-17 H. W. Peng

In this paper, we discuss a gravitational theory based on the generalized gauge field. Our Lagrangian is invariant not only under local Lorentz transformation and the ordinary gauge transformation but also under a new gauge transformation.…

高能物理 - 理论 · 物理学 2012-07-03 Kouzou Nishida

We present $N$-body cosmlogical simulations in the framework of the Newtonian limit of scalar-tensor theories of gravity. The scalar field is described by a modified Helmholtz equation with a source that is coupled to the standard Poisson…

天体物理学 · 物理学 2009-06-23 M. A. Rodriguez-Meza

With the help of Nordtvedt's scalar tensor theory an exact analytical model of a non-minimally coupled scalar field cosmology in which the gravitational coupling $G$ and the Hubble factor $H$ oscillate during the radiation era is presented.…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Narayan Banerjee , Diego Pavon , Somasri Sen

We investigate sufficient conditions under which cubic gravity is healthy and viable at the perturbation level. We perform a detailed analysis of the scalar and tensor perturbations. We impose the requirement that the two scalar potentials,…

广义相对论与量子宇宙学 · 物理学 2024-02-19 Petros Asimakis , Spyros Basilakos , Emmanuel N. Saridakis

We propose a gravitational energy-momentum tensor of the general relativity obtained using Noethers theorem. It transforms as a tensor under general coordinate transformations. One of the two indices of the gravitational energy-momentum…

广义相对论与量子宇宙学 · 物理学 2017-01-05 Katsutaro Shimizu

We study a noncommutative deformation of general relativity where the gravitational field is described by a matrix-valued symmetric two-tensor field. The equations of motion are derived in the framework of this new theory by varying a…

广义相对论与量子宇宙学 · 物理学 2011-02-17 Guglielmo Fucci , Ivan G. Avramidi

We study the induced primordial gravitational waves (GW) coming from the effect of scalar perturbation on the tensor perturbation at the second order of cosmological perturbation theory. We use the evolution of the standard model degrees of…

高能物理 - 唯象学 · 物理学 2020-02-19 Fazlollah Hajkarim , Jürgen Schaffner-Bielich

Non-perturbative studies of quantum gravity have recently suggested the possibility that the strength of gravitational interactions might slowly increase with distance. Here a set of generally covariant effective field equations are…

高能物理 - 理论 · 物理学 2011-07-19 Herbert W. Hamber , Ruth M. Williams

The framework for considering the astronomical and cosmological observations in the context of scalar-tensor quintessence in which the quintessence field also accounts for a time dependence of the gravitational constant is developed. The…

天体物理学 · 物理学 2010-05-28 Alain Riazuelo , Jean-Philippe Uzan

We propose a time-varying parameter $\underline{\alpha}$ for G\"{o}del metric and an energy momentum tensor corresponding to this geometry is found. To satisfy covariance arguments time-varying gravitational and cosmological term are…

高能物理 - 理论 · 物理学 2007-05-23 Carlos Pinheiro , F. C. Khanna , Robert Riche

We consider the cosmological implications of a four-dimensional extension of the Gauss-Bonnet $f(G)$ gravity, where $G$ is the Gauss-Bonnet topological invariant, in which the Einstein-Hilbert action is replaced by an arbitrary function…

广义相对论与量子宇宙学 · 物理学 2025-06-23 Ratul Mandal , Himanshu Chaudhary , Tiberiu Harko , Ujjal Debnath , G. Mustafa

We consider f(R,T) modified theories of gravity, where the gravitational Lagrangian is given by an arbitrary function of the Ricci scalar R and of the trace of the stress-energy tensor T. We obtain the gravitational field equations in the…

广义相对论与量子宇宙学 · 物理学 2011-07-14 Tiberiu Harko , Francisco S. N. Lobo , Shin'ichi Nojiri , Sergei D. Odintsov

Motivated by the newly proposal for gravity as the effect of the torsion scalar $T$ and trace of the energy momentum tensor $\mathcal{T}$,we investigate the cosmological reconstruction of different models of the Universe. Our aim here is to…

广义相对论与量子宇宙学 · 物理学 2018-10-09 Davood Momeni , Ratbay Myrzakulov

A scalar-tensor theory of gravity can be made not only to account for the current cosmic acceleration, but also to satisfy solar-system and laboratory constraints, by introducing a non-linear derivative interaction for the scalar field.…

宇宙学与河外天体物理 · 物理学 2015-03-13 Tsutomu Kobayashi , Hiroyuki Tashiro , Daichi Suzuki

A certain vector-tensor (VT) theory is revisited. It was proposed and analyzed as a theory of electromagnetism without the standard gauge invariance. Our attention is first focused on a detailed variational formulation of the theory, which…

宇宙学与河外天体物理 · 物理学 2013-01-15 Roberto Dale , Diego Sáez

We develop the reconstruction program for the number of modified gravities: scalar-tensor theory, $f(R)$, $F(G)$ and string-inspired, scalar-Gauss-Bonnet gravity. The known (classical) universe expansion history is used for the explicit and…

高能物理 - 理论 · 物理学 2010-04-06 Shin'ichi Nojiri , Sergei D. Odintsov