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相关论文: Bigravity and Lorentz-violating Massive Gravity

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We obtain static, spherically symmetric, and asymptotically flat numerical solutions of massive gravity with a source. Those solutions show, for the first time explicitly, a recovery of the Schwarzschild solution of General Relativity via…

广义相对论与量子宇宙学 · 物理学 2010-04-23 E. Babichev , C. Deffayet , R. Ziour

We present a survey of the known cosmological and black hole solutions in ghost-free bigravity and massive gravity theories. These can be divided into three classes. First, there are solutions with proportional metrics, which are the same…

高能物理 - 理论 · 物理学 2015-06-15 Mikhail S. Volkov

Lorentz and diffeomorphism violations are studied in linearized gravity using effective field theory. A classification of all gauge-invariant and gauge-violating terms is given. The exact covariant dispersion relation for gravitational…

广义相对论与量子宇宙学 · 物理学 2018-02-23 Alan Kostelecky , Matthew Mewes

A quantitative test for the validity of the semi-classical approximation in gravity is given. The criterion proposed is that solutions to the semi-classical Einstein equations should be stable to linearized perturbations, in the sense that…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Paul R. Anderson , Carmen Molina-Paris , Emil Mottola

It is believed that gravity will be explained in the framework of the existing quantum theory when one succeeds in eliminating divergencies at large momenta or small distances (although the phenomenon of gravity has been observed only at…

广义相对论与量子宇宙学 · 物理学 2008-07-28 Felix Lev

We study the cosmological perturbations of the recently proposed extension of non-linear massive gravity with a scalar field. The added scalar field ensures a new symmetry on the field space of the theory. The theory has the property of…

广义相对论与量子宇宙学 · 物理学 2013-07-12 Zahra Haghani , Hamid Reza Sepangi , Shahab Shahidi

We study static spherically symmetric solutions of Einstein gravity plus an action polynomial in the Ricci scalar, $R$, of arbitrary degree, $n$, in arbitrary dimension, $D$. The global properties of all such solutions are derived by…

高能物理 - 理论 · 物理学 2010-11-19 S. Mignemi , D. L. Wiltshire

A unified description of all interactions could be based on a higher-dimensional theory involving only spinor fields. The metric arises as a composite object and the gravitational field equations contain torsion-corrections as compared to…

高能物理 - 理论 · 物理学 2009-02-20 A. Hebecker , C. Wetterich

A number of recent observations have suggested that the Einstein's theory of general relativity may not be the ultimate theory of gravity. The f(R) gravity model with R being the scalar curvature turns out to be one of the best bet to…

广义相对论与量子宇宙学 · 物理学 2019-11-26 Surajit Kalita , Banibrata Mukhopadhyay

We investigate perturbations of a class of spherically symmetric solutions in massive gravity and bi-gravity. The background equations of motion for the particular class of solutions we are interested in reduce to a set of the Einstein…

广义相对论与量子宇宙学 · 物理学 2015-09-08 Tsutomu Kobayashi , Masaru Siino , Masahide Yamaguchi , Daisuke Yoshida

General Relativity is expected to break down in the high-curvature regime. Beyond an effective field theory treatment with higher-order operators, it is important to identify consistent theories with higher-curvature terms at the…

广义相对论与量子宇宙学 · 物理学 2025-10-22 Fabrizio Corelli , Paolo Pani , Andrea P. Sanna

Quasidilaton massive gravity is an extension of massive General Relativity to a theory with additional scale invariance and approximate internal Galilean symmetry. The theory has a novel self-accelerated solution with the metric…

高能物理 - 理论 · 物理学 2014-07-16 Gregory Gabadadze , Rampei Kimura , David Pirtskhalava

General relativity is a non-linear theory with the distinguishing feature that gravitational field energy also acts as gravitational charge density. In the well-known Schwarzschild solution describing field of an isolated massive body at…

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

The basic building block for Lorentz invariant and ghost free massive gravity is the square root of the combination $g^{-1}\eta\,$, where $g^{-1}$ is the inverse of the physical metric and $\eta$ is a reference metric. Since the square root…

高能物理 - 理论 · 物理学 2015-07-08 Denis Comelli , Marco Crisostomi , Kazuya Koyama , Luigi Pilo , Gianmassimo Tasinato

Cascading gravity is an explicit realization of the idea of degravitation, where gravity behaves as a high-pass filter. This could explain why a large cosmological constant does not backreact as much as anticipated from standard General…

高能物理 - 理论 · 物理学 2010-11-02 Claudia de Rham

We derive consistent equations for gravitational wave oscillations in bigravity. In this framework a second dynamical tensor field is introduced in addition to General Relativity and coupled such that one massless and one massive linear…

广义相对论与量子宇宙学 · 物理学 2017-09-25 Kevin Max , Moritz Platscher , Juri Smirnov

We present the exact exterior solution for a static and neutral cylindrically symmetric source in locally conformal invariant Weyl gravity. As a special case the general relativity analogue still can be attained, however only as a…

广义相对论与量子宇宙学 · 物理学 2012-06-05 Jackson Levi Said , Joseph Sultana , Kristian Zarb Adami

As previously observed the massless limit of massive gravity leads to a modification of general relativity. Here we study spherically symmetric solutions of the modified field equations which contain normal matter together with a dark…

广义相对论与量子宇宙学 · 物理学 2009-02-18 G. Scharf

We consider the analytic solutions of massive (bi)gravity which can be written in a simple form using advanced Eddington-Finkelstein coordinates. We analyse the stability of these solutions against radial perturbations. First we recover the…

广义相对论与量子宇宙学 · 物理学 2014-04-23 Eugeny Babichev , Alessandro Fabbri

A theory with the action combining the Einstein--Hilbert term and graviton mass terms violating Lorentz invariance is considered at linearized level about Minkowskian background. It is shown that with one of the masses set equal to zero,…

高能物理 - 理论 · 物理学 2007-05-23 V. Rubakov