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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

Galaxy velocities in clusters, rotation curves of galaxies, and "vertical" oscillations in the Milky Way currently show too high velocities with respect to the masses thought to be involved. While these velocity excesses are currently…

星系天体物理 · 物理学 2024-05-07 Andre Maeder

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

Dark matter, a conjectured substance not directly observable but which has tremendous mass, was proposed to explain why galaxies hold together and rotate faster at their edges than predicted by Newton's Inverse Square (1/r2) Law of Gravity.…

星系天体物理 · 物理学 2013-05-30 Martin Wen-Yu Lo

Recently a new -quantum motivated- theory of gravity has been proposed that modifies the standard Newtonian potential at large distances when spherical symmetry is considered. Accordingly, Newtonian gravity is altered by adding an extra…

星系天体物理 · 物理学 2013-03-14 Jorge Mastache , Jorge L. Cervantes-Cota , Axel de la Macorra

We propose a Lorentz-covariant theory of gravity, and explain its theoretical origins in the problem of time in Newtonian physics. In this retarded gravitation theory (RGT), the gravitational force depends upon both retarded position and…

综合物理 · 物理学 2015-05-27 C. K. Raju

We investigate the radial behavior of galactic rotation curves by a Fourth Order Gravity adding also the Dark Matter component. The Fourth Order Gravity is a Lagrangian containing the Ricci scalar, the Ricci and Riemann tensor, but the…

广义相对论与量子宇宙学 · 物理学 2015-05-28 A. Stabile , G. Scelza

The evidence of the acceleration of universe at present time has lead to investigate modified theories of gravity and alternative theories of gravity, which are able to explain acceleration from a theoretical viewpoint without the need of…

高能物理 - 理论 · 物理学 2011-05-05 Gianluca Allemandi , Andrzej Borowiec , Mauro Francaviglia

Non-baryonic Dark Matter (DM) appears in galaxies and other cosmic structures when and only when the acceleration of gravity, as computed considering only baryons, goes below a well defined value a0=1.2e-8 cm/s/s. This might indicate a…

天体物理学 · 物理学 2009-11-11 Riccardo Scarpa , Gianni Marconi , Roberto Gilmozzi

Verlinde suggested a new theory of gravity called ``emergent gravity,'' which resembles Modified Newtonian Dynamics, the alternative to dark matter theory. For his version of Milgrom's constant, he theoretically derived…

综合物理 · 物理学 2025-08-21 Youngsub Yoon , Ho Seong Hwang

The last decade has seen great advancements in the field of modified gravity, motivated by the dark energy problem, or by the search for a fundamental quantum gravity theory. With a phenomenologically-driven approach, we consider dRGT…

广义相对论与量子宇宙学 · 物理学 2020-01-17 Katarina Martinovic , Mairi Sakellariadou

We discuss the circumstances under which gravity might be repulsive rather than attractive. In particular we show why our standard solar system distance scale gravitational intuition need not be a reliable guide to the behavior of…

广义相对论与量子宇宙学 · 物理学 2022-10-12 Philip D. Mannheim

On the basis of a recent cosmological model, the puzzle of galactic rotational velocities at their edges is explained without invoking dark matter. A rationale for the existence of structures like galaxies and superclusters is also…

天体物理学 · 物理学 2007-05-23 B. G. Sidharth

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

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

The success of the Lambda-CDM model on large scales does not extend down to galaxy scales. We list a dozen problems of the dark matter hypothesis, some of which arise in specific models for the formation of structure in the universe, while…

天体物理学 · 物理学 2007-05-23 J. A. Sellwood , A. Kosowsky

Modified Newtonian dynamics by Milgrom is a paradigm for explaining the rotation curves of spiral galaxies and various other large scale structures. This paradigm includes several different theories. Here we present Milgrom's modified…

广义相对论与量子宇宙学 · 物理学 2021-11-12 Ahmad Shariati , Nosratollah Jafari

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

Dark matter has been a long-standing and important issue in physics, but direct evidence of its existence is lacking. This work aims to elucidate the mystery and show that the dark matter hypothesis is unnecessary. We can nicely reproduce…

星系天体物理 · 物理学 2023-03-07 Jau Tang , Qiang Tang

We present the results from the analysis of galaxy rotation curves with Verlinde's emergent gravity. We use the data in the SPARC (Spitzer Photometry and Accurate Rotation Curves) database, which contains a sample of 175 nearby disk…

广义相对论与量子宇宙学 · 物理学 2022-12-28 Youngsub Yoon , Jong-Chul Park , Ho Seong Hwang