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It is shown that the relativistic invariance plays a key role in the study of integrable systems. Using the relativistically invariant sine-Gordon equation, the Tzitzeica equation, the Toda fields and the second heavenly equation as dual…

可精确求解与可积系统 · 物理学 2023-05-23 S. Y. Lou , X. B. Hu , Q. P. Liu

The post-Minkowskian limit and gravitational wave solutions for general fourth-order gravity theories are discussed. Specifically, we consider a Lagrangian with a generic function of curvature invariants $f(R,…

广义相对论与量子宇宙学 · 物理学 2015-04-28 A. Stabile , S. Capozziello

General relativity can be recast as a theory of connections by performing a canonical transformation on its phase space. In this form, its (kinematical) structure is closely related to that of Yang-Mills theory and topological field…

高能物理 - 理论 · 物理学 2008-02-03 Abhay Ashtekar

Recently there has been developed a reformulation of General Relativity - referred to as {\it the null surface version of GR} - where instead of the metric field as the basic variable of the theory, families of three-surfaces in a…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Simonetta Frittelli , Carlos N. Kozameh , Ezra T. Newman

The Lorentz transformations are represented on the ball of relativistically admissible velocities by Einstein velocity addition and rotations. This representation is by projective maps. The relativistic dynamic equation can be derived by…

经典物理 · 物理学 2010-08-23 Yaakov Friedman

In this paper we identify a new regularity in the systematics of galactic rotation curves, namely we find that at the last detected points in galaxies of widely varying luminosity, the centripetal acceleration is found to have the…

天体物理学 · 物理学 2009-10-28 Philip D. Mannheim

We explore the possibility that the entire departure of galactic rotational velocities from their luminous Newtonian expectation be cosmological in origin, and show that within the framework of conformal gravity (but not Einstein gravity…

天体物理学 · 物理学 2016-08-30 Philip D. Mannheim

Questioning the experimental basis of continuous descriptions of fundamental interactions we discuss classical gravity as an effective continuous first-order approximation of a discrete interaction. The sub-dominant contributions produce a…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Manoelito M de Souza

We covariantly modify the Einstein-Hilbert action such that the modified action perturbatively resolves the flat rotational velocity curve of the spiral galaxies and gives rise to the Tully-Fisher relation, and dynamically generates the…

广义相对论与量子宇宙学 · 物理学 2011-02-01 Qasem Exirifard

It has been claimed in I. Arraut, 2023 EPL 144 29003 [arXiv:2311.05652] that General Relativity can generate effects equivalent to dark matter, based on a "new modified symmetry that emerges at galactic scale". We show that (i) the…

广义相对论与量子宇宙学 · 物理学 2024-04-05 L. Filipe O. Costa , F. Frutos-Alfaro , José Natário , Michael Soffel

We consider a generalized Einstein-Cartan theory, in which we add the unique covariant dimension four operators to general relativity that couples fermionic spin current to the torsion tensor (with an arbitrary strength). Since torsion is…

广义相对论与量子宇宙学 · 物理学 2017-11-01 Stefano Lucat , Tomislav Prokopec

Cosmologies based on General Relativity encompassing an anti-symmetric connection (torsion) can display nice desirable features as the absence of the initial singularity and the possibility of inflation in the early stage of the universe.…

广义相对论与量子宇宙学 · 物理学 2018-12-12 Sergio Bravo Medina , Marek Nowakowski , Davide Batic

We investigate the possibility that the observed flatness of the rotation curves of spiral galaxies is not an evidence for the existence of dark matter haloes, but rather a signal of the breakdown of General Relativity. To this aim, we…

天体物理学 · 物理学 2008-11-26 S. Capozziello , V. F. Cardone , A. - Troisi

The different forms of the Hamiltonian formulations of linearized General Relativity/spin-two theories are discussed in order to show their similarities and differences. It is demonstrated that in the linear model, non-covariant…

广义相对论与量子宇宙学 · 物理学 2011-07-18 K. R. Green , N. Kiriushcheva , S. V. Kuzmin

We exploit the gravitational potential of massive cluster lenses to probe the emission line properties of six z=1 galaxies which appear as highly magnified luminous arcs. Using the GMOS integral field spectrograph together with detailed…

天体物理学 · 物理学 2009-11-11 M. Swinbank , R. Bower , G. P. Smith , Ian Smail , J. -P. Kneib , R. Ellis , D. Stark , A. Bunker

It has recently been suggested that observed galaxy rotation curves can be accounted for by general relativity without recourse to dark-matter halos. A number of objections have been raised, which have been addressed by the authors. Here,…

天体物理学 · 物理学 2007-05-23 Dylan Menzies , Grant J. Mathews

This thesis investigates in the time domain a particular class of second order perturbations of a perfect fluid non-rotating compact star: those arising from the coupling between first order radial and non-radial perturbations. This problem…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Andrea Passamonti

We present a modified Schwarzschild metric to introduce a weak breakdown of asymptotic flatness. The kinematics of the metric captures a wide range of galaxy rotation curves. We show baryonic Tully-Fisher relation on the basis of this…

广义相对论与量子宇宙学 · 物理学 2020-11-10 A. Bhattacharyay

A sample of 22 spiral galaxy rotation curves, measured in the 21 cm line of neutral hydrogen, is considered in the context of Milgrom's modified dynamics (MOND). Combined with the previous highly selected sample of Begeman et al. (1990),…

天体物理学 · 物理学 2009-10-28 R. H. Sanders

Using the Cartan formulation of General Relativity, we construct a well defined lattice-regularized theory capable to describe large non-perturbative quantum fluctuations of the frame field (or the metric) and of the spin connection. To…

高能物理 - 理论 · 物理学 2011-09-02 Dmitri Diakonov