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We study $f(R)$ gravity models in the language of scalar-tensor theories. The correspondence between $f(R)$ gravity and scalar-tensor theories is revisited since $f(R)$ gravity is a subclass of Brans-Dicke models, with a vanishing coupling…

广义相对论与量子宇宙学 · 物理学 2017-06-28 Joseph Ntahompagaze , Amare Abebe , Manasse Mbonye

In this work, we study a vector model of spontaneous spacetime-symmetry breaking coupled to gravity: the bumblebee model. The primary focus is on static spherically symmetric solutions. Complementing previous work on black hole solutions,…

广义相对论与量子宇宙学 · 物理学 2025-12-02 Quentin G. Bailey , Hailey S. Murray , Dario T. Walter-Cardona

We construct a family of measures for random fields based on the iterated subdivision of simple geometric shapes (triangles, squares, tetrahedrons) into a finite number of similar shapes. The intent is to construct continuum limits of scale…

高能物理 - 理论 · 物理学 2012-07-05 Arnab Kar , S. G. Rajeev

For specifically coupled values of the quadratic gravity parameters, we present a fully explicit static spherically symmetric solution. It contains the central singularity surrounded by the black-hole or the cosmological horizon for the…

广义相对论与量子宇宙学 · 物理学 2026-02-04 Simon Knoska , David Kofron , Robert Svarc

We study gravity coupled to a scalar field in spherical symmetry using loop quantum gravity techniques. Since this model has local degrees of freedom, one has to face ``the problem of dynamics'', that is, diffeomorphism and Hamiltonian…

广义相对论与量子宇宙学 · 物理学 2009-11-19 Rodolfo Gambini , Jorge Pullin , Saeed Rastgoo

The properties of static, spherically symmetric configurations are considered in the framework of two models of nonlocally corrected gravity, suggested in S. Deser and R. Woodard., Phys. Rev. Lett. 663, 111301 (2007), and S. Capozziello et…

高能物理 - 理论 · 物理学 2010-04-06 K. A. Bronnikov , E. Elizalde

Static, cylindrically symmetric solutions to nonlinear scalar-Einstein equations are considered. Regularity conditions on the symmetry axis and flat or string asymptotic conditions are formulated in order to select soliton-like solutions.…

广义相对论与量子宇宙学 · 物理学 2011-08-11 K. A. Bronnikov , G. N. Shikin

We set up an Einstein-Gauss-Bonnet theory in four dimensions, based on the recent formulation of pure gravity with extra dimensions of vanishing metrical length [1]. In absence of torsion, the effective field equations depend only on the…

广义相对论与量子宇宙学 · 物理学 2022-02-11 Sandipan Sengupta

Fundamental theories, like strings, supergravity, Kaluza-Klein, lead after dimensional reduction and a suitable choice of field configurations, to an effective action in four dimensions where gravity is coupled non-mininally to one scalar…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Julio C. Fabris

We investigate the existence of static, spherically symmetric compact objects within the framework of symmetric teleparallel scalar-tensor gravity. This theory extends the Brans-Dicke and scalar-tensor models within the symmetric…

广义相对论与量子宇宙学 · 物理学 2026-05-26 Grigorios Panotopoulos , Andrés Lueiza-Colipí , Nikolaos Dimakis , Andronikos Paliathanasis

Static spherically symmetric (SSS) solutions of f(R) gravity are studied in the Einstein frame. The solutions involve SSS configuration mass M and scalaron mass $\mu$ (in geometrized units); for typical astrophysical masses, the…

广义相对论与量子宇宙学 · 物理学 2025-07-28 V. I. Zhdanov

Quintessence models have been widely examined in the context of scalar-Gauss-Bonnet gravity, a subclass of Horndeski's theory, and were proposed as viable candidates for Dark Energy. However, the relatively recent observational constraints…

广义相对论与量子宇宙学 · 物理学 2024-02-27 José Jaime Terente Díaz , Konstantinos Dimopoulos , Mindaugas Karčiauskas , Antonio Racioppi

It is known that the cosmological constant can be dynamically tuned to an arbitrary small value in classes of scalar tensor theories. The trouble with such schemes is that effective gravity itself vanishes. We explore the possibility of…

天体物理学 · 物理学 2007-05-23 Nimmi Rooprai , Daksh Lohiya

We engineer compact SU(5) Grand Unified Theories in F-theory in which GUT-breaking is achieved by a discrete Wilson line. Because the internal gauge field is flat, these models avoid the high scale threshold corrections associated with…

高能物理 - 理论 · 物理学 2015-06-05 Herb Clemens , Joseph Marsano , Tony Pantev , Stuart Raby , Hsian-Hua Tseng

We construct a model unifying gravity with weak $SU(2)$ gauge and "Higgs" scalar fields. We assume the existence of a visible and an invisible (hidden) sector of the Universe. We used the extension of Plebanski's 4-dimensional gravitational…

高能物理 - 唯象学 · 物理学 2013-12-24 C. D. Froggatt , C. R. Das , L. V. Laperashvili , H. B. Nielsen , A. Tureanu

In scalar-tensor Horndeski theories, nonsingular cosmological models - bounce and genesis - are problematic because of potential ghost and/or gradient instabilities. One way to get around this obstacle is to send the effective Planck mass…

高能物理 - 理论 · 物理学 2021-10-04 Y. Ageeva , P. Petrov , V. Rubakov

Theories of modified gravity, in both the linear and fully non-linear regime, are often studied under the assumption that the evolution of the new (often scalar) degree of freedom present in the theory is quasi-static. This approximation…

广义相对论与量子宇宙学 · 物理学 2015-09-09 Hans A. Winther , Pedro G. Ferreira

Global properties of static, spherically symmetric configurations of scalar fields of sigma-model type with arbitrary potentials are studied in $D$ dimensions, including space-times containing multiple internal factor spaces. The latter are…

广义相对论与量子宇宙学 · 物理学 2015-06-25 K. A. Bronnikov , S. B. Fadeev , A. V. Michtchenko

We propose a gravitational model with a Brans-Dicke-type scalar field having, in the would-be action, a "wrong-sign" kinetic term and a quartic interaction term. In a cosmological context, we obtain, depending on the boundary conditions,…

广义相对论与量子宇宙学 · 物理学 2020-08-14 F. R. Klinkhamer

We discuss spherically symmetric static solutions of the Einstein-Klein-Gordon equations for a real scalar field with a mass and a quartic self-interaction term. As for the massless case the solutions have a naked singularity at the origin.…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Philippe Jetzer , David Scialom