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相关论文: The covariant approach to static spacetimes in Ein…

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A general covariant extension of Einstein's field equations is considered with a view to Numerical Relativity applications. The basic variables are taken to be the metric tensor and an additional four-vector. The extended field equations,…

广义相对论与量子宇宙学 · 物理学 2007-05-23 C. Bona , T. Ledvinka , C. Palenzuela , M. Zacek

We summarize recent results on $D$-dimensional Robinson-Trautman solutions of Einstein's gravity in the presence of a conformally invariant non-linear electromagnetic field and a cosmological constant. These spacetimes contain static dyonic…

广义相对论与量子宇宙学 · 物理学 2022-02-01 David Kokoška , Marcello Ortaggio

This research is an extension of the author's article \cite{zar}, in which conformally invariant generalization of string theory was suggested to higher-dimensional objects. Special cases of the proposed theory are Einstein's theory of…

广义相对论与量子宇宙学 · 物理学 2014-10-13 Farkhat Zaripov

The purpose of this paper is to analyze the existence of static stable Einstein universe using inhomogeneous linear perturbations in the context of $f(R,T)$ gravity ($R$ and $T$ denote the scalar curvature and trace of the stress-energy…

广义相对论与量子宇宙学 · 物理学 2020-02-19 M. Sharif , Arfa Waseem

It is shown that the Cotton tensor can describe the effects of gravity beyond general relativity. Any solution of the Einstein equations with or without the cosmological constant satisfies the field equations described by the Cotton tensor.…

广义相对论与量子宇宙学 · 物理学 2021-06-23 Junpei Harada

We study the behavior of static, spherically symmetric solutions to the field equations of scalar-tensor theories (STT) of gravity belonging to the Bergmann-Wagoner-Nordtvedt class, in the presence of an electric and/or magnetic charge.…

广义相对论与量子宇宙学 · 物理学 2024-10-18 Kirill A. Bronnikov , Sergei V. Bolokhov , Milena V. Skvortsova , Rustam Ibadov , Feruza Y. Shaymanova

We investigate the existence of inhomogeneous Szekeres spacetimes in Einstein-\ae ther theory. We show that inhomogeneous solutions which can be seen as extension of the Szekeres solutions existing in Einstein-\ae ther gravity only for a…

广义相对论与量子宇宙学 · 物理学 2020-06-17 Andronikos Paliathanasis

Space-time quantum contributions to the classical Einstein equations of General Relativity are determined. The theoretical background is provided by the non-perturbative theory of manifestly-covariant quantum gravity and the…

广义相对论与量子宇宙学 · 物理学 2018-07-18 Claudio Cremaschini , Massimo Tessarotto

We continue recent work and formulate the gravitational vacuum Einstein equations over a locally finite spacetime by using the basic axiomatics, techniques, ideas and working philosophy of Abstract Differential Geometry. The whole…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Anastasios Mallios , Ioannis Raptis

The subject of this thesis is the coupling of quantum fields to a classical gravitational background in a semiclassical fashion. It contains a thorough introduction into quantum field theory on curved spacetime with a focus on the…

数学物理 · 物理学 2015-03-09 Daniel Siemssen

Scalar curvature invariants are studied in type N solutions of vacuum Einstein's equations with in general non-vanishing cosmological constant Lambda. Zero-order invariants which include only the metric and Weyl (Riemann) tensor either…

广义相对论与量子宇宙学 · 物理学 2008-11-26 J. Bicak , V. Pravda

In this work a static solution of Einstein-Cartan (EC) equations in 2+1 dimensional space-time is given by considering classical spin-1/2 field as external source for torsion of the space-time. Here, the torsion tensor is obtained from…

广义相对论与量子宇宙学 · 物理学 2008-07-29 M. Hortacsu , H. T. Ozcelik , N. Ozdemir

We derive the full set of field equations based on Hossenfelder's recent covariant formulation of the emergent gravity model, along with perturbative and exact solutions. The exact solution describes a static, spherically-symmetric…

广义相对论与量子宇宙学 · 物理学 2018-12-26 Yen-Kheng Lim , Qing-hai Wang

The properties of some locally rotationally symmetric (LRS) perfect fluid space-times are examined in order to demonstrate the usage of the description of geometries in terms of the Riemann tensor and a finite number of its covariant…

广义相对论与量子宇宙学 · 物理学 2009-10-28 Mattias Marklund

Since all Einstein spacetimes are vacuum solutions to quadratic gravity in four dimensions, in this paper we study various aspects of non-Einstein vacuum solutions to this theory. Most such known solutions are of traceless Ricci and Petrov…

广义相对论与量子宇宙学 · 物理学 2017-04-25 Vojtech Pravda , Alena Pravdova , Jiri Podolsky , Robert Svarc

The covariant canonical transformation theory applied to the relativistic Hamiltonian theory of classical matter fields in dynamical space-time yields a novel (first order) gauge field theory of gravitation. The emerging field equations…

广义相对论与量子宇宙学 · 物理学 2023-11-29 David Vasak , Johannes Kirsch , Dirk Kehm , Juergen Struckmeier

The Einstein field equations are derived for a static cylindrically symmetric spacetime with elastic matter. The equations can be reduced to a system of two nonlinear ordinary differential equations and we present analytical and numerical…

广义相对论与量子宇宙学 · 物理学 2014-03-25 I. Brito , J. Carot , F. C. Mena , E. G. L. R. Vaz

The field equations of the recent nonlocal generalization of Einstein's theory of gravitation are presented in a form that is reminiscent of general relativity. The implications of the nonlocal field equations are studied in the case of…

广义相对论与量子宇宙学 · 物理学 2016-05-24 Donato Bini , Bahram Mashhoon

The covariant scheme is proposed to couple gravity and electrodynamics in pseudo-Riemannian four-spaces with electromagnetic connections. Novel dynamics of the extended charge and electromagnetic dilation-compression of its proper time can…

广义相对论与量子宇宙学 · 物理学 2007-05-23 I. E. Bulyzhenkov

We consider tensor-vector theories with varying the space-time-matter coupling constant (varying Einstein velocity) in a spatially flat FRW universe. We examine the dynamics of this model by dynamical system method assuming a \Lambda CDM…

综合物理 · 物理学 2015-06-11 Azam Izadi , Ali Shojai , Mojtaba Nouradini
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