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相关论文: MOND effects in the inner solar system

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It is surprising that we hardly know only 5% of the universe. Rest of the universe is made up of 70% of dark-energy and 25% of dark-matter. Dark-energy is responsible for acceleration of the expanding universe; whereas dark-matter is said…

综合物理 · 物理学 2011-04-06 R. C. Gupta , Anirudh Pradhan

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

A new interpretation is introduced for MOND based on the Sciama's interpretation of Mach principle and an Unruh like effect, in the context of a generalized equivalence principle. It is argued that in a locally accelerated frame with…

宇宙学与河外天体物理 · 物理学 2015-05-14 F. Darabi

I present a class of theories that generalize quasilinear MOND (QUMOND). Like QUMOND, these GQUMOND theories require solving only the linear Poisson equation (twice). Unlike QUMOND, their Lagrangian depends on higher derivatives of the…

星系天体物理 · 物理学 2023-10-05 Mordehai Milgrom

Building upon previous work that derived an alternative to (galactic) dark matter in the form of Modified Newtonian Dynamics (MOND), with a specific theoretical interpolating function, from the motion of a non-relativistic test particle in…

广义相对论与量子宇宙学 · 物理学 2025-11-20 M. E. Pietrzyk , V. A. Kholodnyi , I. V. Kanattšikov , J. Kozicki

The trajectories of test particles moving in the gravitational field of a non-spherically symmetric mass distribution become affected by the presence of multipole moments. In the case of hyperbolic trajectories, the quadrupole moment of an…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Hernando Quevedo

We look for observational signatures that could discriminate between Newtonian and modified Newtonian (MOND) dynamics in the Milky Way, in view of the advent of large astrometric and spectroscopic surveys. Indeed, a typical signature of…

星系天体物理 · 物理学 2015-05-13 O. Bienaymé , B. Famaey , X. Wu , H. S. Zhao , D. Aubert

We report an updated constraint on the Solar System quadrupole parameter $Q_2$, which encodes the external field effect predicted by modified gravity versions of the MOND paradigm. Using the dataset employed to compute the DE440 planetary…

广义相对论与量子宇宙学 · 物理学 2026-02-24 R. S. Park , A. Hees , B. Famaey , H. Desmond , A. Durakovic

We present a new test of modified Newtonian dynamics (MOND) on galactic scales, based on the escape speed in the solar neighbourhood. This test is independent from other empirical successes of MOND at reproducing the phenomenology of…

天体物理学 · 物理学 2009-10-08 Benoit Famaey , Jean-Philippe Bruneton , HongSheng Zhao

Milgromian dynamics (MD or MOND) is a promising physical description excelling especially in galaxies. When formulated as a modified gravity theory, it leads to the so called external field effect (EFE). In the case of the solar system this…

宇宙学与河外天体物理 · 物理学 2017-05-26 R. Paučo , J. Klačka

We reconsider the hypothesis of a vast cometary reservoir surrounding the Solar System - the Oort cloud of comets - within the framework of Milgromian Dynamics (MD or MOND). For this purpose we built a numerical model of the cloud assuming…

地球与行星天体物理 · 物理学 2017-05-25 R. Paučo , J. Klačka

The proximity of the MOND acceleration constant with cosmological accelerations -- for example, a0 cH0/2pi -- points to its possibly decreasing with cosmic time. I begin to consider the secular changes induced in galactic systems by such…

星系天体物理 · 物理学 2015-02-19 Mordehai Milgrom

Recent experimental results for the gravitational constant G from Cavendish-type experiments were analysed in the framework of Modified Newtonian Dynamics (MOND). MOND corrections were applied to the equation of motion of a pendulum, under…

广义相对论与量子宇宙学 · 物理学 2020-01-20 Norbert Klein

Modified Newtonian Dynamics (MOND) is a gravitational framework designed to explain the astronomical observations in the Universe without the inclusion of particle dark matter. Modified Newtonian Dynamics, in its current form, cannot…

宇宙学与河外天体物理 · 物理学 2017-02-15 Alistair Hodson , Hongsheng Zhao

Astrophysical observations (usually explained by dark matter) suggest that classical mechanics could break down when the acceleration becomes extremely small (the approach known as modified Newtonian dynamics, or MOND). I present the first…

广义相对论与量子宇宙学 · 物理学 2008-11-26 A. Yu. Ignatiev

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

Based on Newtonian dynamics, observations show that the luminous masses of astrophysical objects that are the size of a galaxy or larger are not enough to generate the measured motions which they supposedly determine. This is typically…

广义相对论与量子宇宙学 · 物理学 2016-04-22 Chung-Ming Ko

This paper introduces a possible alternative model of gravity based on the theory of fractional-dimension spaces and its applications to Newtonian gravity. In particular, Gauss's law for gravity as well as other fundamental classical laws…

广义相对论与量子宇宙学 · 物理学 2021-02-09 Gabriele U. Varieschi

Modified Newtonian dynamics (MOND) is a possible way to explain the flat galaxy rotation curves without invoking the existence of dark matter. It is however quite difficult to predict such a phenomenology in a consistent field theory, free…

广义相对论与量子宇宙学 · 物理学 2014-11-18 Jean-Philippe Bruneton , Gilles Esposito-Farese

Explaining the effects of dark matter using modified gravitational dynamics (MOND) has for decades been both an intriguing and controversial possibility. By insisting that the gravitational interaction that accounts for the Newtonian force…

天体物理学 · 物理学 2009-11-10 Arthur Lue , Glenn D. Starkman