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相关论文: Comment on the Relativistic Galactic Model by Coop…

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It has recently been suggested that observed galaxy rotation curves can be accounted for by general relativity without recourse to dark-matter halos. Good fits have been produced to observed galatic rotation curves using this model. We show…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Dylan Menzies , Grant J. Mathews

Cooperstock and Tieu have proposed a model to account for galactic rotation curves without invoking dark matter. I argue that no model of this type can work.

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

The general relativistic model of Cooperstock & Tieu, which attempts to fit rotation curves of spiral galaxies without invoking dark matter, is tested empirically using observations of the Milky Way. In particular, predictions for the mass…

天体物理学 · 物理学 2009-11-11 Burkhard Fuchs , Stefanie Phleps

We consider the possibility of an alternative gravity theory explaining the dynamics of galactic systems without dark matter. From very general assumptions about the structure of a relativistic gravity theory we derive a general expression…

广义相对论与量子宇宙学 · 物理学 2009-10-22 Vadim V. Zhytnikov , James M. Nester

The recently proposed Cooperstock-Tieu galaxy model claims to explain the flat rotation curves without dark matter. The purpose of this note is to show that this model is internally inconsistent and thus cannot be considered a valid…

天体物理学 · 物理学 2007-05-23 Daniel J. Cross

We consider the consequences of applying general relativity to the description of the dynamics of a galaxy, given the observed flattened rotation curves. The galaxy is modeled as a stationary axially symmetric pressure-free fluid. In spite…

天体物理学 · 物理学 2010-10-27 F. I. Cooperstock , S. Tieu

Many cosmological observations call for the existence of dark matter. The most direct evidence for dark matter is inferred from the measured flatness of galactic rotation curves. The latter is based on Newtonian gravity. Alternative…

广义相对论与量子宇宙学 · 物理学 2008-11-19 Aleksandar Rakic , Dominik J. Schwarz

There are some approaches, either based on General Relativity (GR) or modified gravity, that use galaxy rotation curves to derive the matter density of the corresponding galaxy, and this procedure would either indicate a partial or a…

星系天体物理 · 物理学 2016-08-29 Álefe O. F. de Almeida , Oliver F. Piattella , Davi C. Rodrigues

Recently a new model of galactic gravitational field, based on ordinary General Relativity, has been proposed by Cooperstock and Tieu in which no exotic dark matter is needed to fit the observed rotation curve to a reasonable ordinary…

天体物理学 · 物理学 2007-05-23 Mikolaj Korzynski

The missing of a Keplerian fall-off in the observed galaxy rotation curves represents classical evidence for the existence of dark matter on galactic scales. There has been some recent activity concerning the potential of modelling galactic…

广义相对论与量子宇宙学 · 物理学 2010-02-17 Aleksandar Rakic , Dominik J. Schwarz

It has been proposed that the flat rotation curves observed at large radii in disk galaxies can be interpreted as an effect of General Relativity (GR) instead of the presence of dark matter (DM) halos in Newtonian gravity. In Ciotti (2022)…

星系天体物理 · 物理学 2024-11-07 Luca Ciotti

A solution for the problem of understanding observed rotation curves in galaxies without the introduction of dark matter halos is presented. This solution has been obtained upon considering the distribution of masses in the expanding…

广义相对论与量子宇宙学 · 物理学 2009-09-25 J. L. Rosales

The observed flat rotation curves of galaxies require either the presence of dark matter in Newtonian gravitational potentials or a significant modification to the theory of gravity at galactic scales. Detecting relativistic Doppler shifts…

星系天体物理 · 物理学 2012-02-15 Alan Cooney , Dimitrios Psaltis , Dennis Zaritsky

We show that, contrary to some recent claims, relativistic effects cannot mimic dark matter in the galactic rotation curves and gravitational lensing.

广义相对论与量子宇宙学 · 物理学 2026-04-03 L. Filipe O. Costa , José Natário

A unified parametrization of the circular velocity, which accurately fits 850 galaxy rotation curves without needing in advance the knowledge of the luminous matter components, nor a fixed dark matter halo model, is proposed. A notable…

星系天体物理 · 物理学 2018-03-14 E. Lopez Fune

A galaxy is modeled as a stationary axially symmetric pressure-free fluid in general relativity. For the weak gravitational fields under consideration, the field equations and the equations of motion ultimately lead to one linear and one…

天体物理学 · 物理学 2007-05-23 F. I. Cooperstock , S. Tieu

Galactic rotation curve is a powerful indicator of the state of the gravitational field within a galaxy. The flatness of these curves indicates the presence of dark matter in galaxies and their clusters. In this paper, we focus on the…

广义相对论与量子宇宙学 · 物理学 2023-11-28 Gayatri Mohan , Umananda Dev Goswami

The existence of "dark matter", inferred from the observed rotation curves of galaxies, is a hypothesis which is widely regarded as problematic. This paper proposes an alternative hypothesis based on the space-time geometry near a rotating…

综合物理 · 物理学 2020-02-27 Colin Rourke

Recently, several interesting proposals were made modifying the law of gravity on large scales, within a sensible relativistic formulation. This allows a precise formulation of the idea that such a modification might account for galaxy…

高能物理 - 唯象学 · 物理学 2010-04-06 A. Aguirre , C. P. Burgess , A. Friedland , D. Nolte

We derive a formula for the velocity distribution of an axially symmetric galaxy where the mass density is corrected using the mass formula from special relativity. We take some reasonable test mass densities and numerically compute the…

广义相对论与量子宇宙学 · 物理学 2023-02-21 Jaroslaw S. Jaracz
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