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相关论文: Dwarf Galaxies, MOND, and Relativistic Gravitation

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We propose a new framework unifying cold dark matter (CDM) and Modified Newtonian Dynamics (MOND) to solve their respective problems on galactic scales and large scale structure formation. In our framework the dark matter clusters on large…

宇宙学与河外天体物理 · 物理学 2012-07-04 Baojiu Li , Hongsheng Zhao

In our current cosmological model, the main constituents of the Universe are dark matter and dark energy, whose nature is unknown, and for which there is no place in the standard model of particle physics. How to include dark matter and…

宇宙学与河外天体物理 · 物理学 2009-10-31 Luc Blanchet , Francoise Combes

A general account of MOND theory is given. I start with the basic tenets of MOND, which posit departure from standard dynamics in the limit of low acceleration -- below an acceleration constant a0 -- where dynamics become scale invariant. I…

宇宙学与河外天体物理 · 物理学 2015-02-16 Mordehai Milgrom

Modified Gravity (MOG) and Non-Local Gravity (NLG) are two alternative theories to General Relativity. They are able to explain the rotation curves of spiral galaxies and clusters of galaxies without including dark matter (Moffat & Rahvar…

星系天体物理 · 物理学 2017-11-09 M. H. Zhoolideh Haghighi , S. Rahvar

The MOdified Newtonian Dynamics (MOND) is an alternative to the dark matter assumption that can explain the observed flat rotation curve of galaxies. Here hydrodynamic accretion is considered to critically check the consistency and to…

星系天体物理 · 物理学 2012-02-24 Nirupam Roy

I show that Modified Newtonian Dynamics (MOND) is equivalent to assuming an isothermal dark matter density profile, with its density related to the enclosed total baryonic mass. This density profile can be deduced by physical laws if a dark…

宇宙学与河外天体物理 · 物理学 2015-06-17 Man Ho Chan

Some dwarf galaxies are within the Mondian regime at all radii, i.e., the gravitational acceleration provided by the observed baryons is always below the threshold of $g_\dag\simeq 1.2\times 10^{-10}\,{\rm m\,s^{-2}}$. These dwarf galaxies…

星系天体物理 · 物理学 2022-11-30 J. Sanchez Almeida

The MOdified Newtonian Dynamics (MOND) is an attempt to modify the gravitation theory to solve the Dark Matter problem. This phenomenology is very successful at the galactic level. The main effect produced by MOND in the Solar System is…

广义相对论与量子宇宙学 · 物理学 2014-05-14 A. Hees , W. M. Folkner , R. A. Jacobson , R. S. Park

A new class of modified gravity theories, made possible by subtle features of the canonical formulation of general covariance, naturally allows MOND-like behavior (MOdified Newtonian Dynamics) in effective space-time solutions without…

广义相对论与量子宇宙学 · 物理学 2023-11-01 Martin Bojowald , Erick I. Duque

The discovery of dark matter particles would conclusively reject the MOND theory. MOND may violate Einstein's Strong Equivalence principle. However, as we show, there is already evidence that MOND is likely not required. MOND was invented…

天体物理学 · 物理学 2007-05-23 David B. Cline

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 detailed semi-analytical models for the formation of disk galaxies both in a Universe dominated by dark matter (DM), and in one for which the force law is given by modified Newtonian dynamics (MOND). We tune the models to fit the…

天体物理学 · 物理学 2009-10-31 Frank C. van den Bosch , Julianne J. Dalcanton

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

Regime of MOND, which is used in astronomy to describe the gravitating systems of island type without the need to postulate the existence of a hypothetical dark matter, is generalized to the case of homogeneous distribution of usual matter…

广义相对论与量子宇宙学 · 物理学 2019-11-28 V. V. Kiselev , S. A. Timofeev

The works in this portfolio test the hypothesis that it is not possible to extrapolate the Newtonian inverse square law of gravity from Solar System to galaxy scales. In particular, I look into various tests of Modified Newtonian Dynamics…

星系天体物理 · 物理学 2023-09-26 Indranil Banik

We derive the distribution of the phantom dark matter in the eight classical dwarf galaxies surrounding the Milky Way, under the assumption that modified Newtonian dynamics (MOND) is the correct theory of gravity. According to their…

星系天体物理 · 物理学 2020-10-02 Alistair O. Hodson , Antonaldo Diaferio , Luisa Ostorero

We discuss a comparison of models for the formation of disk galaxies both in a Universe dominated by cold dark matter (CDM) and one in which the force law is given by modified Newtonian dynamics (MOND). Our main aim is to address the claim…

天体物理学 · 物理学 2007-05-23 Frank C. van den Bosch , Julianne J. Dalcanton

I discuss open theoretical questions pertaining to the modified dynamics (MOND)--a proposed alternative to dark matter, which posits a breakdown of Newtonian dynamics in the limit of small accelerations. In particular, I point the reasons…

天体物理学 · 物理学 2009-11-07 Mordehai Milgrom

Modified Newtonian Dynamics (MOND) at low acceleration has been astonishingly powerful at explaining the flat rotation curve of galaxies and the relation between the baryonic content of the galaxies and their observed circular velocity,…

星系天体物理 · 物理学 2021-06-30 Mohammadtaher Safarzadeh , Abraham Loeb

I review briefly different aspects of the MOND paradigm, with emphasis on phenomenology, epitomized here by many MOND laws of galactic motion--analogous to Kepler's laws of planetary motion. I then comment on the possible roots of MOND in…

天体物理学 · 物理学 2008-03-10 Mordehai Milgrom