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相关论文: On G\"odel-type Solution in Rastall's Gravity

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We present a generalization of Rastall's gravity in which the conservation law of the energy-momentum tensor is altered, and as a result, the trace of the energy-momentum tensor is taken into account together with the Ricci scalar in the…

广义相对论与量子宇宙学 · 物理学 2022-02-24 Clésio E. Mota , Luis C. N. Santos , Franciele M. da Silva , Guilherme Grams , Iarley P. Lobo , Débora P. Menezes

Rastall gravity is the same as General Relativity, with a simple algebraic redefinition of what is called the energy-momentum tensor. Despite it having been very clearly explained by M. Visser several years go, there are still many papers…

广义相对论与量子宇宙学 · 物理学 2024-07-11 Alexey Golovnev

The Rastall's theory is a modification of General Relativity touching one of the cornestone of gravity theory: the conservation laws. In Rastall's theory, the energy-momentum tensor is not conserved anymore, depending now on the gradient of…

广义相对论与量子宇宙学 · 物理学 2015-06-19 J. C. Fabris , O. F. Piattella , D. C. Rodrigues , M. H. Daouda

Rastall gravity, originally developed in 1972, is currently undergoing a significant surge in popularity. Rastall gravity purports to be a modified theory of gravity, with a non-conserved stress-energy tensor, and an unusual non-minimal…

广义相对论与量子宇宙学 · 物理学 2018-05-30 Matt Visser

Rastall's theory is a modification of Einstein's theory of gravity where the covariant divergence of the stress-energy tensor is no more vanishing, but proportional to the gradient of the Ricci scalar. The motivation of this theory is to…

广义相对论与量子宇宙学 · 物理学 2015-06-12 Gabriel F. Silva , Oliver F. Piattella , Julio C. Fabris , Luciano Casarini , Taislane O. Barbosa

Rastall generalized Einstein's field equations relaxing the Einstein's assumption that the covariant divergence of the energy-momentum tensor should vanish. His field equations contain a free parameter alpha and in an empty space, i.e. if…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Vladimir Majernik , Lukas Richterek

Rastall gravity is a modified gravity proposal that incorporates a non-conserved energy momentum tensor (EMT). We study the equivalence between Rastall gravity and general relativity, analyzing its consequences for an EMT of dark matter and…

广义相对论与量子宇宙学 · 物理学 2023-03-08 Javier Chagoya , López-Domínguez , C. Ortiz

Einstein's famous equivalence principle is certainly one of the most striking features of the gravitational interaction. In a strict reading, it states that the effects of gravity can be made to disappear $locally$ by a convenient choice of…

广义相对论与量子宇宙学 · 物理学 2023-08-02 Daniel A. T. Vanzella

In this short review, we discuss the approach of the commutator algebra of covariant derivative to analyse the gravitational theories, starting from the standard Einstein's general theory of relativity and focusing on the Rastall theory.…

广义相对论与量子宇宙学 · 物理学 2017-09-14 I. Licata , H. Moradpour , C. Corda

Rastall introduced a stress-energy tensor whose divergence is proportional to the gradient of the Ricci scalar. This proposal leads to a change in the form of the field equations of General Relativity, but it preserves the number of degrees…

广义相对论与量子宇宙学 · 物理学 2023-02-28 Júlio C. Fabris , Oliver F. Piattella , Davi C. Rodrigues

We calculate static and spherically symmetric solutions for the Rastall modification of gravity to describe Neutron Stars (NS). The key feature of the Rastall gravity is the non-conservation of the energy-momentum tensor proportionally to…

广义相对论与量子宇宙学 · 物理学 2016-10-24 A. M. Oliveira , H. E. S. Velten , J. C. Fabris , L. Casarini

One of the eminent generalizations of theory of general relativity is the Rastall gravity which was {constructed} based on the assumption of the non-conserved energy-momentum tensor of the matter field. Despite in the literature several…

广义相对论与量子宇宙学 · 物理学 2023-09-06 Bobir Toshmatov , Zdeněk Stuchlík , Bobomurat Ahmedov

Rastall gravity is a generalization of the Einstein gravity in which the matter is not conserved in the presence of a non-constant spacetime curvature. In this report, we analyze Rastall gravity using the linearized formalism. The…

广义相对论与量子宇宙学 · 物理学 2025-05-12 Yuwadee Tongkong

We profit by a recent paper of Visser claiming that Rastall gravity is equivalent to Einstein gravity to compare the two gravitational theories in a general way. Our conclusions are different from Visser's ones. We indeed argue that these…

广义相对论与量子宇宙学 · 物理学 2018-01-16 F. Darabi , H. Moradpour , I. Licata , Y. Heydarzade , C. Corda

The existence of conservation laws is one of the most important requirement of physical theories. Some of them, like energy conservation, knows no experimental exception. However, the generalization of these conservation laws to curved…

广义相对论与量子宇宙学 · 物理学 2012-08-24 J. C. Fabris

In the Rastall gravity a non-minimal coupling between geometry and matter fields is considered. Then the usual energy-momentum tensor conservation law is not valid. Here a Lagrangian formalism is proposed to the Rastall theory of gravity.…

广义相对论与量子宇宙学 · 物理学 2019-12-16 W. A. G. De Moraes , A. F. Santos

The Rastall gravity is a modification of Einstein's general relativity, in which the energy-momentum conservation is not satisfied and depends on the gradient of the Ricci curvature. It is in dispute whether the Rastall gravity is…

星系天体物理 · 物理学 2020-08-26 Meirong Tang , Zhaoyi Xu , Jiancheng Wang

The Einstein static (ES) state is a good candidate for describing the very early universe in terms of a regular cosmological model in which the Big Bang singularity is avoided. In the present study we propose an ES solution in the framework…

广义相对论与量子宇宙学 · 物理学 2022-08-18 Hamid Shabani , Amir Hadi Ziaie , Hooman Moradpour

The Rastall's theory is a modification of the General Relativity theory leading to a different expression for the conservation law in the matter sector compared with the usual one. It has been argued recently that such a theory may have…

宇宙学与河外天体物理 · 物理学 2010-04-29 C. E. M. Batista , J. C. Fabris , M. Hamani Daouda

Rastall's theory is a modification of General Relativity, based on the non-conservation of the stress-energy tensor. The latter is encoded in a parameter $\gamma$ such that $\gamma = 1$ restores the usual $\nabla_\nu T^{\mu\nu} = 0$ law. We…

宇宙学与河外天体物理 · 物理学 2014-07-18 C. E. M. Batista , J. C. Fabris , O. F. Piattella , A. M. Velasquez-Toribio
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