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Some recently discovered nonperturbative strong-field effects in tensor-scalar theories of gravitation are interpreted as a scalar analog of ferromagnetism: "spontaneous scalarization". This phenomenon leads to very significant deviations…

广义相对论与量子宇宙学 · 物理学 2016-08-24 Thibault Damour , Gilles Esposito-Farese

We investigate cosmological perturbations of f(G) gravity in the presence of a scalar field. Using the 1 + 3 covariant formalism, we present the energy overdensity perturbation equations responsible for large scale structure formation.…

广义相对论与量子宇宙学 · 物理学 2023-12-27 Albert Munyeshyaka , Joseph Ntahompagaze , Tom Mutabazi , Manasse. R Mbonye

We present a formalism to compute Lagrangian displacement fields for a wide range of cosmologies in the context of perturbation theory up to third order. We emphasize the case of theories with scale dependent gravitational strengths, such…

宇宙学与河外天体物理 · 物理学 2018-01-16 Alejandro Aviles , Jorge L. Cervantes-Cota

We study new consistent scalar-tensor theories of gravity recently introduced by Langlois and Noui with potentially interesting cosmological applications. We derive the conditions for the existence of a primary constraint that prevents the…

高能物理 - 理论 · 物理学 2016-04-22 Marco Crisostomi , Kazuya Koyama , Gianmassimo Tasinato

In perturbative gravity, it is straight-forward to characterize the two local degrees of freedom of the gravitational field in terms of a mode expansion of the linearized perturbation. In the non-perturbative regime, we are in a more…

广义相对论与量子宇宙学 · 物理学 2023-05-04 Wolfgang Wieland

Within the scheme of modified gravity, an exponential Lagrangian density will be considered, and the corresponding scalar-tensor description will be addressed for both positive and negative values of the cosmological constant. For negative…

广义相对论与量子宇宙学 · 物理学 2008-11-26 O. M. Lecian , G. Montani

Gravitational double layers, unlike their classical electromagnetic counterparts, are thought to be forbidden in gravity theories. It has been recently shown, however, that they are feasible in, for instance, gravity theories with a…

广义相对论与量子宇宙学 · 物理学 2015-05-20 José M. M. Senovilla

Modified gravity theories on cosmic scales have three key deviations from general relativity. They can cause cosmic acceleration without a physical, highly negative pressure fluid, can cause a gravitational slip between the two metric…

宇宙学与河外天体物理 · 物理学 2014-11-04 Eric V. Linder

In a four-dimensional space I shall construct all of the conformally invariant, scalar-vector-tensor field theories that are consistent with conservation of charge, and flat space compatible. By the last assumption I mean that the…

广义相对论与量子宇宙学 · 物理学 2018-01-29 Gregory W. Horndeski

We investigate the nature of additional scalar degrees of freedom contained in extended hybrid metric-Palatini gravity, outlining the emergence of two coupled dynamical scalar modes. In particular, we discuss the weak field limit of the…

广义相对论与量子宇宙学 · 物理学 2019-12-17 Flavio Bombacigno , Fabio Moretti , Giovanni Montani

Lagrange scalar densities which are concomitants of two scalar fields, a pseudo-Riemannian metric tensor, and their derivatives of arbitrary differential order are investigated in a space of four-dimensions. I construct the most general…

广义相对论与量子宇宙学 · 物理学 2025-08-05 Gregory W. Horndeski

We investigate scalar-induced gravitational waves (SIGWs) in the framework of spatially covariant gravity (SCG), a broad class of Lorentz-violating modified gravity theories respecting only spatial diffeomorphism invariance. Extending…

广义相对论与量子宇宙学 · 物理学 2026-02-13 Jiehao Jiang , Jieming Lin , Xian Gao

We formulate a scalar realization of Sciama's Machian programme within the general Bergmann-Wagoner class of scalar--tensor gravity. Starting from a universally conformally coupled matter sector, we rewrite the field equations in terms of…

广义相对论与量子宇宙学 · 物理学 2026-01-14 Velásquez-Toribio , A. M

The Hamiltonian constraint formalism is used to obtain the first explicit complete analysis of non-trivial viable dynamic modes for the Poincar\'e gauge theory of gravity. Two modes with propagating spin-zero torsion are analyzed. The…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Hwei-jang Yo , James M. Nester

The cosmological scalar perturbations of standard matter are investigated in the context of extended teleparallel $f(T)$ gravity theories using the $1+3$ covariant formalism. After a review of the background, gravitational field equations…

广义相对论与量子宇宙学 · 物理学 2020-06-24 Shambel Sahlu , Joseph Ntahompagaze , Amare Abebe , Alvaro de la Cruz-Dombriz , David F. Mota

The evidence of the acceleration of universe at present time has lead to investigate modified theories of gravity and alternative theories of gravity, which are able to explain acceleration from a theoretical viewpoint without the need of…

高能物理 - 理论 · 物理学 2011-05-05 Gianluca Allemandi , Andrzej Borowiec , Mauro Francaviglia

We present new second derivative, generally covariant theories of gravity for spherically symmetric spacetimes (general covariance is in the $t-r$ plane) belonging to the class where the spherically symmetric Einstein-Hilbert theory is…

广义相对论与量子宇宙学 · 物理学 2015-05-20 Rakesh Tibrewala

We investigate generally covariant theories which admit a Fierz-Pauli mass term for metric perturbations around an arbitrary curved background. For this we restore the general covariance of the Fierz-Pauli mass term by introducing four…

高能物理 - 理论 · 物理学 2012-07-02 Lasma Alberte

Investigations of the dynamic modes of the Poincare gauge theory of gravity found only two good propagating torsion modes; they are effectively a scalar and a pseudoscalar. Cosmology affords a natural situation where one might see…

广义相对论与量子宇宙学 · 物理学 2008-12-18 Kun-Feng Shie , James M. Nester , Hwei-Jang Yo

We derive a condition on the Lagrangian density describing a generic, single, non-canonical scalar field, by demanding that the intrinsic, non-adiabatic pressure perturbation associated with the scalar field vanishes identically. Based on…

宇宙学与河外天体物理 · 物理学 2010-06-18 Sanil Unnikrishnan , L. Sriramkumar