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If it is hypothesised that there is no dark matter then some alternative gravitational theory must take the place of general relativity (GR) on the largest scales. Dynamical measurements can be used to investigate the nature of such a…

天体物理学 · 物理学 2008-11-26 Daniel J. Mortlock , Edwin L. Turner

We consider f(R,T) modified theory of gravity, in which the gravitational Lagrangian is given by an arbitrary function of the Ricci scalar and the trace of the energy-momentum tensor of the matter, in order to investigate the dark-matter…

广义相对论与量子宇宙学 · 物理学 2016-11-02 Raziyeh Zaregonbadi , Mehrdad Farhoudi , Nematollah Riazi

The observation of the bending of light by mass, now known as gravitational lensing, was key in establishing general relativity as one of the pillars of modern physics. In the past couple of decades, there has been increasing interest in…

广义相对论与量子宇宙学 · 物理学 2022-07-20 Arthur B. Congdon , Savitri V. Iyer , Charles R. Keeton

We show that it is not possible in the absence of dark matter to construct a four-dimensional metric that explains galactic observations. In particular, by working with an effective potential it is shown that a metric which is constructed…

广义相对论与量子宇宙学 · 物理学 2009-10-31 A. Edery

We offer a concise and direct way to derive the bending angle of light (i.e. as generally called, gravitational lensing), while light grazes a star, through the approach suggested earlier by the first author, which is fundamentally based on…

综合物理 · 物理学 2014-01-15 Tolga Yarman , Alexander Kholmetskii , Metin Arik

We study gravitational lensing by clusters of galaxies in the context of the generic class of unconventional gravity theories of the scalar--tensor type. For positive energy scalar fields with any dynamics, the bending of light by a weakly…

天体物理学 · 物理学 2010-11-01 Jacob D. Bekenstein , Robert H. Sanders

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

Weyl's conformal gravity theory, which is considered as a compelling alternative to general relativity theory, has been claimed to describe the observed flat rotation curve feature of spiral galaxies without the need of invoking dark…

广义相对论与量子宇宙学 · 物理学 2023-07-12 Shubhrangshu Ghosh , Mahasweta Bhattacharya , Yanzi Sherpa , Arunava Bhadra

It is now, generally, believed that the presence of some form of dark matter is essential to explain the flat rotation curves of galaxies, and anomalous large velocities of galaxies in the clusters and superclusters. This dark matter turns…

天体物理学 · 物理学 2007-05-23 Mofazzal Azam

Various theories, such as MOND, MOG, Emergent Gravity and $f(R)$ theories avoid dark matter by assuming a change in General Relativity and/or in Newton's law. Galactic rotation curves are typically described well. Here the application to…

宇宙学与河外天体物理 · 物理学 2021-07-28 Theodorus Maria Nieuwenhuizen

Weyl gravity has been advanced in the recent past as an alternative to General Relativity (GR). The theory has had some success in fitting galactic rotation curves without the need for copious amounts of dark matter. To check the viability…

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

As we now know, there are indeed at least two major difficulties with General Relativity (GR). The first one is related with its incompatibility with quantum mechanics, in the absence of a widely accepted consistent theory that combines the…

综合物理 · 物理学 2015-06-05 Ram Gopal Vishwakarma

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

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

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

Light is the richest information retriever for most physical systems, particularly so for astronomy and cosmology, in which gravitation is of paramount importance, and also for solid state defects and metamaterials, in which some effects…

广义相对论与量子宇宙学 · 物理学 2017-04-03 Lucas T. Santana , Maurício O. Calvão , Ribamar R. R. Reis , Beatriz B. Siffert

Understanding the deflection of light by a massive deflector, as well as the associated gravitational lens phenomena, require the use of the theory of General Relativity. I consider here a classical approach, based on Newton's equation of…

物理教育 · 物理学 2008-03-05 T. Garel

Recently, it has been suggested that the phenomenology of flat rotation curves observed at large radii in the equatorial plane of disk galaxies can be explained as a manifestation of General Relativity instead of the effect of Dark Matter…

星系天体物理 · 物理学 2022-09-21 Luca Ciotti

We suggest a new explanation of flatness of galaxies rotation curves without invoking dark matter. For this purpose a new gravitational tensor field is introduced in addition to the metric tensor.

高能物理 - 唯象学 · 物理学 2023-12-25 S. A. Larin

There is evidence that Newton and Einstein's theories of gravity cannot explain the dynamics of a universe made up solely of baryons and radiation. To be able to understand the properties of galaxies, clusters of galaxies and the universe…

天体物理学 · 物理学 2014-02-18 T. G Zlosnik , P. G Ferreira , G. D Starkman
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