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We propose an alternative scalar-tensor theory based on the Khronon scalar field labeling a family of space-like three-dimensional hypersurfaces. This theory leads to modified Newtonian dynamics (MOND) at galactic scales for stationary…

广义相对论与量子宇宙学 · 物理学 2025-07-02 Luc Blanchet , Constantinos Skordis

The modified Newtonian dynamics (MOND) paradigm is discussed in the context of asymptotic safe gravity. We estimate quantum correction to the logarithmic potential which is well known to account for the constancy of the circular velocity…

广义相对论与量子宇宙学 · 物理学 2022-08-23 Bijan Bagchi , Sauvik Sen

The stability of galaxies is either explained by the existence of dark matter or caused by a modification of Newtonian acceleration (MOND). Here we show that the modification of the Newtonian dynamics can equally well be obtained by a…

星系天体物理 · 物理学 2024-04-24 Søren Toxvaerd

Many past attempts to kill MOND have only strengthened the theory. Better data on galaxy velocity curves clearly favor MOND (without fine-tuning) over cold dark matter. The usual critism on the incompleteness of classical MOND has spurred a…

天体物理学 · 物理学 2007-05-23 HongSheng Zhao

We propose that future experiments aiming at the detection of deviations from the inverse square gravitational law on submillimetric scales can be used to test the modified Newtonian dynamics theory (MOND). Current experiments are able to…

天体物理学 · 物理学 2009-11-06 Sandro O. Mendes , Reuven Opher

MOND-- modified Newtonian dynamics-- may be viewed as an algorithm for calculating the distribution of force in an astronomical object from the observed distribution of baryonic matter. The fact that it works for galaxies is quite…

天体物理学 · 物理学 2008-06-17 R. H. Sanders

The classical gravitational two-body problem is generalized in order to be applicable also to weak gravitational fields. The equation of motion holds both for terrestrial and large cosmic scales, the Newtonian gravitational law represents a…

星系天体物理 · 物理学 2020-05-18 Jozef Klačka

The Modified Newtonian Dynamics (MOND) paradigm generically predicts that the external gravitational field in which a system is embedded can produce effects on its internal dynamics. In this communication, we first show that this External…

星系天体物理 · 物理学 2015-11-10 A. Hees , B. Famaey , G. W. Angus , G. Gentile

Our main goal is here to make a comparative analysis between the well-known MOND theory and a more recent model called$\kappa$-model. An additional connection, between the $\kappa$-model and twoother novel MOND-type theories: Newtonian…

星系天体物理 · 物理学 2024-04-09 Gianni Pascoli

MOND is a paradigm that contends to account for the mass discrepancies in the Universe without invoking `dark' components, such as `dark matter' and `dark energy'. It does so by supplanting Newtonian dynamics and General Relativity,…

星系天体物理 · 物理学 2020-03-09 Mordehai Milgrom

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

We compare N-body simulations performed in MOND with analogs in Newtonian gravity with dark matter (DM). We have developed a code which solves the Poisson equation in both gravity models. It is a grid solver using adaptive mesh refinement…

天体物理学 · 物理学 2007-12-11 O. Tiret , F. Combes

Under natural assumptions on the thermodynamic properties of space and time with the holographic principle we reproduce a MOND-like behaviour of gravity on particular scales of mass and length, where Newtonian gravity requires a…

广义相对论与量子宇宙学 · 物理学 2015-10-16 D. A. Carranza , S. Mendoza

Stars with a different vertical motion relative to the galactic disk have a different average acceleration. According to Modified Newtonian Dynamics (MOND) theories they should therefore have a different average orbital velocity while…

星系天体物理 · 物理学 2016-01-27 Ben Margalit , Nir J. Shaviv

We consider a class of nonlocal, pure-metric modified gravity models which were developed to reproduce the Tully-Fisher relation without dark matter and without changing the amount of weak lensing predicted by general relativity. Previous…

宇宙学与河外天体物理 · 物理学 2015-06-19 Cedric Deffayet , Gilles Esposito-Farese , Richard P. Woodard

A relativistic MOND theory, promising in reproducing cosmology as well as the MOND phenomenology in the low acceleration regime, was recently proposed. We present the post-Newtonian (PN) approximation and relativistic perturbation equations…

广义相对论与量子宇宙学 · 物理学 2025-03-12 Jai-chan Hwang , Hyerim Noh

We show that treating gravitation as a thermodynamical theory leads to the modified Newton dynamics (MOND) equations if one takes into account the Hubble's expansion. Then the universal MOND acceleration a0 is exactly twice the product of…

宇宙学与河外天体物理 · 物理学 2015-03-17 Peter V. Pikhitsa

Galactic systems, and the Universe at large, exhibit large dynamical anomalies: The observed matter in them falls very short of providing enough gravity to account for their dynamics. The mainstream response to this conundrum is to invoke…

星系天体物理 · 物理学 2017-07-25 Mordehai Milgrom

We propose a relativistic model of dark matter reproducing at once the concordance cosmological model $\Lambda$-Cold-Dark-Matter ($\Lambda$-CDM) at cosmological scales, and the phenomenology of the modified Newtonian dynamics (MOND) at…

宇宙学与河外天体物理 · 物理学 2015-06-17 Laura Bernard , Luc Blanchet

For a point mass residing in an expanding universe, within General Relativity (GR), a new metric [1} is found to lead to a cosmological background dependent MOND-like acceleration in addition to the Newtonian acceleration. In [2], we study…

星系天体物理 · 物理学 2025-10-28 James C. C. Wong