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相关论文: A common Milgromian acceleration scale in nature

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In a previous paper we have proposed a non--Newtonian, phenomenological description of the effective gravitational force acting between exotic dark matter and baryons, which was shown to fit well the kinematics in the inner regions of low…

天体物理学 · 物理学 2007-05-23 Christian Marinoni , Federico Piazza

One of the deepest and most long-standing mysteries in physics has been the huge discrepancy between the observed vacuum density and our expectations from theories of high energy physics, which has been dubbed the Old Cosmological Constant…

宇宙学与河外天体物理 · 物理学 2012-03-02 Siavash Aslanbeigi , Georg Robbers , Brendan Z. Foster , Kazunori Kohri , Niayesh Afshordi

We find a new family of galactic metrics corresponding to flat rotation curves at the outer radii. These are vacuum solutions to a gravity theory where the Newton's coupling varies mildly in space. The effective `mass', whose origin is…

广义相对论与量子宇宙学 · 物理学 2025-05-08 Rounak Chakraborty , Sandipan Sengupta

We investigate galactic rotation curves in $f(T)$ gravity, where $T$ represents a torsional quantity. Our study centers on the particular Lagrangian $f(T)=T+\alpha{T^n}$, where $|n|\neq 1$ and $\alpha$ is a small unknown constant. To do…

星系天体物理 · 物理学 2018-08-01 Andrew Finch , Jackson Levi Said

We submit the viewpoint that, perhaps, some of the controversies in gravitation occurred during this century are not due to insufficiencies of Einstein's field equations, but rather to insufficiencies in the mathematics used for their…

综合物理 · 物理学 2011-04-15 Ruggero Maria Santilli

Modified Gravity (MOG) has been used successfully to explain the rotation curves of galaxies, the motion of galaxy clusters, the Bullet Cluster, and cosmological observations without the use of dark matter or Einstein's cosmological…

宇宙学与河外天体物理 · 物理学 2015-03-17 J. W. Moffat

That preferred-frame theory accounts for special relativity and reduces to it if the gravitation field cancels. Starting from an interpretation of gravity as a pressure force, it is based on just one scalar field. This scalar gives the…

广义相对论与量子宇宙学 · 物理学 2017-08-23 Mayeul Arminjon

The amount of dark matter in the Milky Way and beyond is examined by taking into account the possible running of the gravitational constant $G$ as a function of distance scale. If the running of $G$, as suggested by the Asymptotically-Free…

天体物理学 · 物理学 2010-11-30 A. Bottino , C. W. Kim , J. Song

Dictated by Symmetry Principle, string theory predicts not General Relativity but its own gravity which assumes the entire closed string massless sector to be geometric and thus gravitational. In terms of $R/(MG)$, i.e. the dimensionless…

高能物理 - 理论 · 物理学 2018-01-12 Jeong-Hyuck Park

The discrepancy between the visible mass in galaxies or galaxy clusters, and that inferred from their dynamics is well known. The prevailing solution to this problem is dark matter. Here we show that a different approach, one that conforms…

星系天体物理 · 物理学 2020-06-24 Alexandre Deur , Corey Sargent , Balša Terzić

We discuss the problem of universe acceleration driven by global rotation. The redshift-magnitude relation is calculated and discussed in the context of SN Ia observation data. It is shown that the dynamics of considered problem is…

天体物理学 · 物理学 2008-07-22 Wlodzimierz Godlowski , Marek Szydlowski

Given the dimensions (including thickness) of a galaxy, and its rotation profile, a method is shown that finds the mass and density distributions in the defined envelope that will cause that rotation profile with near-exact speed matches.…

天体物理学 · 物理学 2007-05-23 Kenneth F. Nicholson

Galaxies are huge physical systems having dimensions of many tens of thousands of light years. Thus any change at the galactic center will be noticed at the rim only tens of thousands of years later. Those retardation effects seems to be…

综合物理 · 物理学 2025-05-27 Asher Yahalom

The accelerated expansion of the universe poses a significant challenge to General Relativity. Non-local modifications to gravity have emerged as a compelling class of theories to address this dark energy puzzle. Building upon earlier…

广义相对论与量子宇宙学 · 物理学 2025-11-19 Susobhan Mandal , S. Shankaranarayanan

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

In this work we study the properties of rigidly rotating neutral dust solutions in general relativity. This class of solutions gained relevance recently due to applications to the dynamics of spiral galaxies. We show that this class could…

广义相对论与量子宇宙学 · 物理学 2022-07-06 Davide Astesiano

The phenomenon of augmented gravity on the scale of galaxies, conventionally attributed to dark matter halos, is shown to possibly result from the incremental growth of galactic masses and radii over time. This approach elucidates the…

综合物理 · 物理学 2025-06-04 Artur Novais , André L. B. Ribeiro

We consider the classical theory of a gravitational field with spin 2 and non-vanishing (Pauli-Fierz) mass in flat spacetime, coupled to electromagnetism and point particles. We establish the law of light propagation and calculate the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Matteo Carrera , Domenico Giulini

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

The observed absence of gravitational aberration requires that ``Newtonian'' gravity propagate at a speed $c_g>2\times10^{10}c$. By evaluating the gravitational effect of an accelerating mass, I show that aberration in general relativity is…

广义相对论与量子宇宙学 · 物理学 2010-04-28 S. Carlip