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Related papers: Purely Magnetic Spacetimes

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Spacetimes in which the electric part of the Weyl tensor vanishes (relative to some timelike unit vector field) are said to be purely magnetic. Examples of purely magnetic spacetimes are known and are relatively easy to construct, if no…

General Relativity and Quantum Cosmology · Physics 2007-05-23 Alan Barnes

It is shown that there are no vacuum space-times (with or without cosmological constant) for which the Weyl-tensor is purely gravito-magnetic with respect to a normal and timelike congruence of observers.

General Relativity and Quantum Cosmology · Physics 2017-08-23 N. Van den Bergh

We study almost universal spacetimes - spacetimes for which the field equations of any generalized gravity with the Lagrangian constructed from the metric, the Riemann tensor and its covariant derivatives of arbitrary order reduce to one…

General Relativity and Quantum Cosmology · Physics 2019-02-05 Martin Kuchynka , Tomáš Málek , Vojtěch Pravda , Alena Pravdová

We consider time reversal transformations to obtain twofold orthogonal splittings of any tensor on a Lorentzian space of arbitrary dimension n. Applied to the Weyl tensor of a spacetime, this leads to a definition of its electric and…

General Relativity and Quantum Cosmology · Physics 2013-07-30 Sigbjørn Hervik , Marcello Ortaggio , Lode Wylleman

We introduce the new algebraic property of Weyl compatibility for symmetric tensors and vectors. It is strictly related to Riemann compatibility, which generalizes the Codazzi condition while preserving much of its geometric implications.…

Mathematical Physics · Physics 2016-03-10 Carlo A. Mantica , Luca G. Molinari

We introduce a general algebraic decomposition of Riemann-like and Weyl-like tensors with respect to a non-null vector $u$. We derive Gauss, Codazzi and Ricci-type identities for the Weyl tensor, that allow to relate the components of the…

General Relativity and Quantum Cosmology · Physics 2025-07-30 Marc Mars , Carlos Peón-Nieto

A four-index tensor is constructed with terms both quadratic in the Riemann tensor and linear in its second derivatives, which has zero divergence for space-times with vanishing scalar curvature. This tensor reduces in vacuum to the…

General Relativity and Quantum Cosmology · Physics 2009-10-31 M. A. G. Bonilla , C. F. Sopuerta

This brief paper investigates the consequences for the metric tensor of space-time when the Weyl tensor (in its conformally invariant form) and the energy-momentum tensor is specified. It is shown that, unless rather special conditions…

General Relativity and Quantum Cosmology · Physics 2010-11-11 G. S. Hall , M. Sharif

The paper considers the problem of finding the metric of space time around a rotating, weakly gravitating body. Both external and internal metric tensors are consistently found, together with an appropriate source tensor. All tensors are…

General Relativity and Quantum Cosmology · Physics 2007-05-23 A. Tartaglia

Recent results on purely electric (PE) or magnetic (PM) spacetimes in n dimensions are summarized. These include: Weyl types; diagonalizability; conditions under which direct (or warped) products are PE/PM.

General Relativity and Quantum Cosmology · Physics 2014-11-14 Sigbjørn Hervik , Marcello Ortaggio , Lode Wylleman

A comprehensive analysis of general relativistic spacetimes which admit a shear-free, irrotational and geodesic timelike congruence is presented. The equations governing the models for a general energy-momentum tensor are written down.…

General Relativity and Quantum Cosmology · Physics 2010-04-06 Alan A. Coley , Des J. Mc Manus

Universal spacetimes are spacetimes for which all conserved symmetric rank-2 tensors, constructed as contractions of polynomials from the metric, the Riemann tensor and its covariant derivatives of arbitrary order, are multiples of the…

General Relativity and Quantum Cosmology · Physics 2014-10-17 Sigbjørn Hervik , Vojtech Pravda , Alena Pravdova

We study umbilically synchronized space-times $M$ that have vanishing electric part of the Weyl tensor and show that (i) If $dim(M) = 4$, then $M$ is conformally flat, (ii) If $dim(M) > 4$, $M$ is conformally flat if and only if the spatial…

General Relativity and Quantum Cosmology · Physics 2022-11-15 Ramesh Sharma

Taking wedge products of the $p$ distinct principal null directions associated with the eigen-bivectors of the Weyl tensor associated with the Petrov classification, when linearly independent, one is able to express them in terms of the…

General Relativity and Quantum Cosmology · Physics 2023-07-26 D. Bini , A. Geralico , R. T. Jantzen

We prove theorems about the Ricci and the Weyl tensors on generalized Robertson-Walker space-times of dimension $n\ge 3$. In particular, we show that the concircular vector introduced by Chen decomposes the Ricci tensor as a perfect fluid…

Mathematical Physics · Physics 2016-10-24 Carlo Alberto Mantica , Luca Guido Molinari

We have solved the Einstein-Maxwell equations for a class of isotropic metrics with constant spatial curvature in the presence of magnetic fields. We consider a slight modification of the Tolman averaging relations so that the…

General Relativity and Quantum Cosmology · Physics 2014-09-11 Eduardo Bittencourt , José Salim , Grasiele B. dos Santos

It is shown that there are no vacuum space-times (with or without cosmological constant) for which the Weyl-tensor is purely gravito-magnetic with respect to a congruence of freely falling observers.

General Relativity and Quantum Cosmology · Physics 2009-11-10 Norbert Van den Bergh

We study the class of vacuum (Ricci flat) six-dimensional spacetimes admitting a non-degenerate multiple Weyl aligned null direction l, thus being of Weyl type II or more special. Subject to an additional assumption on the asymptotic…

General Relativity and Quantum Cosmology · Physics 2017-06-26 Marcello Ortaggio

A regular class of static, cylindrically symmetric pure magnetic field metrics is rederived in a different metric ansatz in all dimensions. Radial, time dependent perturbations show that for dimensions d>3 such spacetimes are stable at both…

General Relativity and Quantum Cosmology · Physics 2016-09-30 Tayebeh Tahamtan , Mustafa Halilsoy

We define space-times which are asymptotic to radiation dominant Friedman-Robertson-Walker space-times at timelike infinity and study the asymptotic structure. We discuss the local asymptotic symmetry and give a definition of the total…

General Relativity and Quantum Cosmology · Physics 2009-10-31 Tetsuya Shiromizu , Uchida Gen
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