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We consider solutions with conformal symmetry of the static, spherically symmetric gravitational field equations in the vacuum in the brane world scenario. By assuming that the vector field generating the symmetry is non-static, the general…

广义相对论与量子宇宙学 · 物理学 2010-11-19 M. K. Mak , T. Harko

The effect of the global rotation of the universe on the formation of galaxies is investigated. It is found that the global rotation provides a natural origin for the rotation of galaxies, and the morphology of the objects formed from…

天体物理学 · 物理学 2015-06-24 Li-Xin Li

Assuming a suitable rotation of the Universe as a whole, we can attribute the rotation of galaxies to it. Using Lagrangian Mechanics we then can find the equations governing the rotation of a galaxy. We find in this way the azimuthal…

综合物理 · 物理学 2012-05-30 Evangelos Chaliasos

We review some recent developments in the conformal gravity theory that has been advanced as a candidate alternative to standard Einstein gravity. As a quantum theory the conformal theory is both renormalizable and unitary, with unitarity…

高能物理 - 理论 · 物理学 2015-05-27 Philip D. Mannheim

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

Conformal gravity has been proposed as an alternative theory of gravity which can account for flat galactic rotation curves without recourse to copious quantities of dark matter. However it was shown that for the usual choice of the metric,…

天体物理学 · 物理学 2008-12-30 A. Edery , A. A. Méthot , M. B. Paranjape

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

We investigate recent claims that gravitomagnetic effects in linearised general relativity can explain flat and rising rotation curves, such as those observed in galaxies, without the need for dark matter. If one models a galaxy as an…

广义相对论与量子宇宙学 · 物理学 2023-04-13 A. N. Lasenby , M. P. Hobson , W. E. V. Barker

We propose a new formula to explain circular velocity profiles of spiral galaxies obtained from the Starobinsky model in Palatini formalism. It is based on the assumption that the gravity can be described by two conformally related metrics:…

广义相对论与量子宇宙学 · 物理学 2018-04-13 Ciprian A. Sporea , Andrzej Borowiec , Aneta Wojnar

Circular velocities of stars and gas in galaxies generally do not decline in accordance with widely expected Keplerian fall-off in velocities further from the galactic nucleus. Two main groups of theories were proposed to explain the…

星系天体物理 · 物理学 2014-06-11 Konstantin Pavlovich , Alex Pavlovich , Alan Sipols

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

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

We make a first application of the linear gravitational potentials of the conformal gravity theory to the distance scale associated with clusters of galaxies, with the theory being found to give a reasonable value for the mean velocity of…

天体物理学 · 物理学 2007-05-23 Philip D. Mannheim

The flattening of spiral-galaxy rotation curves is unnatural in view of the expectations from Kepler's third law and a central mass. It is interesting, however, that the radius-independence velocity is what one expects in one less…

星系天体物理 · 物理学 2021-09-22 Felipe J. Llanes-Estrada

Quantum gravity places entirely new challenges on the formulation of a consistent theory as well as on an extraction of potentially observable effects. Quantum corrections due to the gravitational field are commonly expected to be tiny…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Martin Bojowald

The dark matter hypothesis, which is not called into question here, explains why typical rotation curves of spiral galaxies do not follow a Keplerian profile. It is however not sufficient in itself to explain why the whole matter…

星系天体物理 · 物理学 2019-06-13 Vincent Deledicque

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

In this work, we submit the explanation of spectra of the rotary curves of galaxies on the basis of a vector theory of gravitation without regard to the dark matter hypothesis. We study the approximation of rotary curves in case of existing…

综合物理 · 物理学 2011-05-10 V. N. Borodikhin

It has been suggested that the observed flat rotation curves of disk galaxies can be a peculiar effect of General Relativity (GR) rather than evidence for the presence of dark matter (DM) halos in Newtonian gravity. In Ciotti (2022) the…

星系天体物理 · 物理学 2023-04-14 Luca Ciotti

We comment on the methods and the conclusion of Ref. [1], "Does gravitational confinement sustain flat galactic rotation curves without dark matter?" The article employs two methods to investigate whether non-perturbative corrections from…

广义相对论与量子宇宙学 · 物理学 2023-06-05 A. Deur