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相关论文: Nonlinear Evolution of Quadratic Gravity in 3+1 Di…

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We consider the model of modified gravity with dynamical torsion. This model was previously found to have promising stability properties about various backgrounds. Here we study the stability of linear perturbations about the…

高能物理 - 理论 · 物理学 2017-11-06 V. Nikiforova

We consider a complex scalar field minimally coupled to gravity and to a U(1) gauge symmetry and we construct of a first order symmetric hyperbolic evolution system for the Einstein-Maxwell-Klein-Gordon system. Our analysis is based on a…

广义相对论与量子宇宙学 · 物理学 2013-04-04 Daniela Pugliese , Juan A. Valiente Kroon

We present the first proof-of-principle Cauchy evolutions of asymptotically global AdS spacetimes with no imposed symmetries, employing a numerical scheme based on the generalized harmonic form of the Einstein equations. In this scheme, the…

高能物理 - 理论 · 物理学 2021-04-23 Hans Bantilan , Pau Figueras , Lorenzo Rossi

We study the gravitational potential generated by static, spherically symmetric matter distributions in a quadratic $f(R)$ gravity model. In the weak-field regime, the linearized field equations lead to a fourth-order modified Poisson…

广义相对论与量子宇宙学 · 物理学 2026-02-10 Roger Anderson Hurtado

We consider predictions for structure formation from modifications to general relativity in which the Einstein-Hilbert action is replaced by a general function of the Ricci scalar. We work without fixing a gauge, as well as in explicit…

天体物理学 · 物理学 2010-04-06 Rachel Bean , David Bernat , Levon Pogosian , Alessandra Silvestri , Mark Trodden

The massive nonsymmetric gravitational theory is shown to posses a linearisation instability at purely GR field configurations, disallowing the use of the linear approximation in these situations. It is also shown that arbitrarily small…

广义相对论与量子宇宙学 · 物理学 2009-10-28 M. A. Clayton

Gravitational collapse and bubble evolution in the asymptotical Friedmann-Lemaitre-Robertson-Walker (FLRW) Universe is an intriguing and intricate problem. We systematically analyze dynamics for contact \sch-FLRW (McVittie) spacetimes,…

广义相对论与量子宇宙学 · 物理学 2026-05-26 Jining Tang , Yang Huang , Hongsheng Zhang

We consider a series of distorted black hole initial data sets, and develop techniques to evolve them using the linearized equations of motion for the gravitational wave perturbations on a Schwarzschild background. We apply this to 2D and…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Gabrielle Allen , Karen Camarda , Edward Seidel

Modifications to gravity that add additional functions of the Ricci curvature to the Einstein-Hilbert action -- collectively known as $f(R)$ theories -- have been studied in great detail. When considered as complete theories of gravity they…

天体物理学 · 物理学 2009-02-20 Simon DeDeo , Dimitrios Psaltis

We study modified theories of gravity of the f(R) type in Palatini formalism. We first consider the stability of atoms when the Palatini gravitational interaction is taken into account in the derivation of the non-relativistic Schrodinger…

广义相对论与量子宇宙学 · 物理学 2014-11-20 Gonzalo J. Olmo

We present a general approach to the analysis of gauge stability of 3+1 formulations of General Relativity (GR). Evolution of coordinate perturbations and the corresponding perturbations of lapse and shift can be described by a system of…

广义相对论与量子宇宙学 · 物理学 2009-11-07 A. M Khokhlov , I. D. Novikov

A new approach to gravitational gauge-invariant perturbation theory begins from the fourth-order Einstein-Ricci system, a hyperbolic formulation of gravity for arbitrary lapse and shift whose centerpiece is a wave equation for curvature. In…

广义相对论与量子宇宙学 · 物理学 2011-04-21 Arlen Anderson , Andrew M. Abrahams , Chris Lea

We analyze evolution of gravitational perturbations of D-dimensional Schwarzschild, Reissner-Nordstr\"om, and Reissner-Nordstrom-de Sitter black holes. It is known that the effective potential for the scalar type of gravitational…

高能物理 - 理论 · 物理学 2010-10-27 R. A. Konoplya , A. Zhidenko

To explain the accelerated expansion of late universe, the 1/R correction to Einstein gravity is usually considered, where R is the Ricci scalar. This correction term is generally believed to be negligible in the early universe. However, if…

宇宙学与河外天体物理 · 物理学 2014-11-20 Shi Pi , Tower Wang

A cosmological model describing the evolution of n Ricci-flat spaces (n>1) in the presence of 1-component perfect-fluid and minimally coupled scalar field is considered. When the pressures in all spaces are proportional to the density, the…

高能物理 - 理论 · 物理学 2009-09-25 V. D. Ivashchuk , V. N. Melnikov

Through averaging the Einstein equations over transverse gravitational perturbations it is obtained a closed system of two ordinary differential equations describing macroscopic cosmological evolution of the isotropic space-flat Universe…

广义相对论与量子宇宙学 · 物理学 2016-08-24 Yurii Ignat'ev

The evolution equations for tensor perturbations in a generic scalar tensor theory of gravity are presented. Exact solution are given for a specific class of theories and Friedmann-Lema\^{i}tre-Robertson-Walker backgrounds. In these cases…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Sante Carloni , Peter K. S. Dunsby

This paper establishes the global existence of solutions for a class of wave-Klein-Gordon coupled systems with specific nonlinearities in 3+1-dimensional Minkowski spacetime. The study demonstrates that imposing certain constraints on the…

偏微分方程分析 · 数学 2026-04-21 Yue Ma , Weidong Zhang

Gravitational waves with parallel rays are known to have remarkable properties: Their orbit space of null rays possesses the structure of a non-relativistic spacetime of codimension-one. Their geodesics are in one-to-one correspondence with…

高能物理 - 理论 · 物理学 2016-02-22 Xavier Bekaert , Kevin Morand

We analyze the global nonlinear stability of FRW (Friedmann-Robertson-Walker) spacetimes in presence of an irrotational perfect fluid. We assume that the fluid is governed by the so-called (generalized) Chaplygin equation of state relating…

广义相对论与量子宇宙学 · 物理学 2015-12-14 Philippe G. LeFloch , Changhua Wei
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