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相关论文: On the MOND External Field Effect in the Solar Sys…

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Milgromian dynamics (MD or MOND) uniquely predicts motion in a galaxy from the distribution of its stars and gas in a remarkable agreement with observations so far. In the solar system, MD predicts the existence of some possibly…

地球与行星天体物理 · 物理学 2017-07-05 R. Paučo

In recent work (Milgrom 2009, Blanchet & Novak 2011), the authors showed that MOdified Newton Dynamics (MOND) have a non-negligible secular perturbation effect on planets with large semi-major axes (gaseous planets) in the Solar System.…

地球与行星天体物理 · 物理学 2015-04-16 Lucie Maquet , Frédéric Pierret

The tight radial acceleration relation (RAR) obeyed by rotationally supported disk galaxies is one of the most successful a priori predictions of the modified Newtonian dynamics (MOND) paradigm on galaxy scales. Another important…

星系天体物理 · 物理学 2022-02-02 J. Freundlich , B. Famaey , P. -A. Oria , M. Bílek , O. Müller , R. Ibata

MOdified Newtonian Dynamics (MOND) is an interesting alternative to dark matter in extragalactic systems. We here examine the possibility that mild or even strong MOND behavior may become evident well inside the solar system, in particular…

天体物理学 · 物理学 2009-11-11 Jacob Bekenstein , Joao Magueijo

We examine the claimed observations of a gravitational external field effect (EFE) reported in Chae et al. We show that observations suggestive of the EFE can be interpreted without violating Einstein's equivalence principle, namely from…

广义相对论与量子宇宙学 · 物理学 2025-11-11 Corey Sargent , William Clark , Antonia Seifert , Alicia Mand , Emerson Rogers , Adam Lane , Alexandre Deur , Balša Terzić

I discuss a novel MOND effect that entails a correction to the dynamics of isolated mass systems even when they are deep in the Newtonian regime: systems whose extent R<<Rm, where Rm=sqrt(GM/a0) is the MOND radius, and M the total mass.…

宇宙学与河外天体物理 · 物理学 2012-09-24 Mordehai Milgrom

The possibility that ultra-diffuse galaxies lacking dark matter has recently stimulated interest to check the validity of Modified Newton Dynamics (MOND) predictions on the scale of such galaxies. It has been shown that the External Field…

星系天体物理 · 物理学 2019-03-06 Oliver Müller , Benoit Famaey , Hongsheng Zhao

In this letter we investigate the deep Newtonian regime of the MOND paradigm from a purely phenomenological point of view by exploiting the least-square estimated corrections to the secular rates of the perihelia of the inner and of some of…

广义相对论与量子宇宙学 · 物理学 2008-02-22 Lorenzo Iorio

Theories of modified gravity generically violate the strong equivalence principle, so that the internal dynamics of a self-gravitating system in free fall depends on the strength of the external gravitational field (the external field…

星系天体物理 · 物理学 2021-11-17 Kyu-Hyun Chae , Harry Desmond , Federico Lelli , Stacy S. McGaugh , James M. Schombert

Any viable theory of modified Newtonian dynamcs (MOND) as modified gravity is likely to require fields in addition to the usual tensor field of General Relativity. For such theories the MOND phenomenology emerges from an effective fifth…

天体物理学 · 物理学 2009-11-11 R. H. Sanders

We examine the implications of Modified Newtonian Dynamics (MOND) on the large scale structure in a Friedmann-Robertson-Walker universe. We employ a ``Jeans swindle'' to write a MOND-type relationship between the fluctuations in the density…

天体物理学 · 物理学 2009-11-07 Adi Nusser

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

In this paper, we investigate the external field effect in the context of the MOdified Newtonian Dynamics (MOND) on the surface brightness and velocity dispersion profiles of globular clusters (GCs). Using N-MODY, which is an N-body…

星系天体物理 · 物理学 2014-04-09 Kamran Derakhshani

Modified Newtonian dynamics (MOND), which postulates a breakdown of Newton's laws of gravity/dynamics below some critical acceleration threshold, can explain many otherwise puzzling observational phenomena on galactic scales. MOND competes…

宇宙学与河外天体物理 · 物理学 2024-03-15 David Vokrouhlický , David Nesvorný , Scott Tremaine

The gravitational dipole theory of Hadjukovic (2010) is based on the hypothesis that antimatter has a negative gravitational mass and thus falls upwards on Earth. Astrophysically, the model is similar to but more fundamental than Modified…

地球与行星天体物理 · 物理学 2020-06-12 Indranil Banik , Pavel Kroupa

It is well-known that the application of Newtonian dynamics to an expanding spherical region leads to the correct relativistic expression (the Friedmann equation) for the evolution of the cosmic scale factor. Here, the cosmological…

天体物理学 · 物理学 2009-10-30 R. H. Sanders

In general relativity (GR), the internal dynamics of a self-gravitating system under free-fall in an external gravitational field should not depend on the external field strength. Recent work has claimed a statistical detection of an…

宇宙学与河外天体物理 · 物理学 2022-10-05 Aseem Paranjape , Ravi K. Sheth

It was recently proposed that the effects usually attributed to particle dark matter on galaxy scales are due to the displacement of dark energy by baryonic matter, a paradigm known as emergent gravity. This formalism leads to predictions…

星系天体物理 · 物理学 2017-03-22 Aurelien Hees , Benoit Famaey , Gianfranco Bertone

Analytical expressions for the orbital precessions affecting the relative motion of the components of a local binary system induced by Lorentz-violating Preferred Frame Effects (PFE) are explicitly computed in terms of the PPN parameters…

广义相对论与量子宇宙学 · 物理学 2014-01-06 Lorenzo Iorio

The Strong Equivalence Principle (SEP) demands, besides the validity of the Einstein Equivalence Principle, that all self-gravitating bodies feel the same acceleration in an external gravitational field. It has been found that metric…

广义相对论与量子宇宙学 · 物理学 2008-02-03 Norbert Wex