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The behavior of the angular velocity of a test particle moving in a stable circular orbit in the vacuum on the brane is considered. In the brane world scenario, the four dimensional effective Einstein equation acquire extra terms, called…

广义相对论与量子宇宙学 · 物理学 2008-11-26 C. G. Boehmer , T. Harko

The dynamical mass of galaxies and the Newtonian acceleration generated from the baryons have been found to be strongly correlated. This correlation is known as 'Mass-Discrepancy Acceleration Relation' (MDAR). Further investigations have…

星系天体物理 · 物理学 2020-05-07 Tousif Islam , Koushik Dutta

We compare six models (including the baryonic model, two dark matter models, two modified Newtonian dynamics models and one modified gravity model) in accounting for the galaxy rotation curves. For the dark matter models, we assume NFW…

广义相对论与量子宇宙学 · 物理学 2017-05-10 Xin Li , Li Tang , Hai-Nan Lin

The phenomenology of MOND (flat rotation curves of galaxies, baryonic Tully-Fisher relation, etc.) is a basic set of phenomena relevant to galaxy dynamics and dark matter distribution at galaxy scales. Still unexplained today, it enjoys a…

宇宙学与河外天体物理 · 物理学 2015-06-19 Luc Blanchet , Laura Bernard

A theory is proposed which allows explaining the observed flat galaxy rotation curves, without needing to invoke dark matter. Whereas other theories have been proposed in the past which realize the same, the present theory rests on basic…

综合物理 · 物理学 2015-05-13 Rudi Van Nieuwenhove

We propose a phenomenological model where the gravitational interaction between dark matter and baryons is suppressed on small, subgalactic scales. We describe the gravitational force by adding a Yukawa contribution to the standard…

高能物理 - 唯象学 · 物理学 2009-11-10 Federico Piazza , Christian Marinoni

We show that a global relation between baryonic mass and virial velocity can be constructed from the scale of dwarf galaxies up to that of rich galaxy clusters. The slope of this relation is close to that expected if dark matter halos form…

天体物理学 · 物理学 2009-11-10 Lucio Mayer , Ben Moore

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

We present a new mechanism for baryogenesis, which links the baryon asymmetry of the universe to the dark matter density. The mechanism arises naturally in the Pentagon model of TeV scale physics. In that context, it forces a re-evaluation…

高能物理 - 唯象学 · 物理学 2009-11-11 T. Banks , S. Echols , J. L. Jones

We study gravitational waves (GWs) with frequencies in the $\mu$Hz range, which arise from phase transitions related to dark confinement in the context of dark versions of Quantum Chromodynamics. Based on several compelling motivations, we…

高能物理 - 唯象学 · 物理学 2024-05-28 Martin Rosenlyst

In the braneworld scenario the four dimensional effective Einstein equation has extra source terms, which arise from the embedding of the 3-brane in the bulk. These non-local effects, generated by the free gravitational field of the bulk,…

广义相对论与量子宇宙学 · 物理学 2011-10-14 L. Á. Gergely , T. Harko , M. Dwornik , G. Kupi , Z. Keresztes

We study geometries of galactic rotation curves from Dark Matter (DM) and Modified Newtonian Dynamics (MOND) models in $(g_{\rm bar},g_{\rm tot})$-space ($g2$-space) where $g_{\rm tot}$ is the total centripetal acceleration of matter in the…

星系天体物理 · 物理学 2018-05-29 Mads T. Frandsen , Jonas Petersen

Many studies point out that there exists some tight correlations between dark matter and baryonic matter at different radii in galaxies. However, similar tight correlations can only be found in galaxy clusters for large radii. Here we…

宇宙学与河外天体物理 · 物理学 2020-04-15 Man Ho Chan

In recent years, modified gravity theories have gained significant attention as potential replacements for the general theory of relativity. Neutron stars, which are dense compact objects, provide ideal astrophysical laboratories for…

广义相对论与量子宇宙学 · 物理学 2023-07-20 K. Nobleson , Sarmistha Banik , Tuhin Malik

We investigate the generation of the observed baryon asymmetry of the Universe within the framework of $f(T,T_{G})$ gravity, where $T$ is the torsion scalar and $T_{G}$ denotes its teleparallel Gauss--Bonnet counterpart. Two illustrative…

综合物理 · 物理学 2025-12-09 Amit Samaddar , S. Surendra Singh

General relativity (GR) is the most successful theory of gravity, with great observational support on local scales. However, to keep GR valid over cosmic scales, some phenomena (such as flat galaxy rotation curves and the cosmic expansion…

宇宙学与河外天体物理 · 物理学 2025-11-12 Robert Monjo , Indranil Banik

We study slowly-rotating neutron stars in ghost-free massive bigravity. This theory modifies General Relativity by introducing a second, auxiliary but dynamical tensor field that couples to matter through the physical metric tensor through…

广义相对论与量子宇宙学 · 物理学 2018-02-14 Andrew Sullivan , Nicolas Yunes

I review the connection between dynamics and the baryonic mass distribution in rotationally supported galaxies. The enclosed dynamical mass-to-light ratio increases with decreasing galaxy luminosity and surface brightness. The correlation…

星系天体物理 · 物理学 2015-03-27 Stacy S. McGaugh

We generalize tensor-scalar theories of gravitation by the introduction of an abnormally weighting type of energy. This theory of tensor-scalar anomalous gravity is based on a relaxation of the weak equivalence principle that is now…

天体物理学 · 物理学 2009-01-14 J. -M. Alimi , A. Füzfa

We have recently shown that the baryonic Tully-Fisher (BTF) and Faber-Jackson (BFJ) relations imply that the gravitational "constant" $G$ in the force law vary with acceleration $a$ as $1/a$. Here we derive the converse from first…

星系天体物理 · 物理学 2018-11-26 Dimitris M. Christodoulou , Demosthenes Kazanas