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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

We looked at the orbital motions of test particles according to the External Field Effect (EFE) predicted by the MOdified Newtonian Dynamics (MOND) in the Oort cloud which falls in the deep MONDian regime (r\approx 50-150 kAU). Concerning…

广义相对论与量子宇宙学 · 物理学 2014-11-20 Lorenzo Iorio

In the framework of the MOdified Newtonian Dynamics (MOND), the internal dynamics of a gravitating system s embedded in a larger one S is affected by the external background field E of S even if it is constant and uniform, thus implying a…

广义相对论与量子宇宙学 · 物理学 2009-09-17 Lorenzo Iorio

We numerically investigate the features of typical orbits occurring in the Oort cloud (r\approx 50-150 kAU) in the low-acceleration regime of the MOdified Newtonian Dynamics (MOND). We take into account the so-called External Field Effect…

广义相对论与量子宇宙学 · 物理学 2011-04-07 Lorenzo Iorio

The Modified Newtonian Dynamics (MOND) has been formulated as a modification of the Poisson equation for the Newtonian gravitational field. This theory generically predicts a violation of the strong version of the equivalence principle, and…

宇宙学与河外天体物理 · 物理学 2011-04-26 Luc Blanchet , Jerome Novak

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

Trans-Neptunian objects (TNOs) are remnants of a collisionally and dynamically evolved planetesimal disk in the outer solar system. This complex structure, known as the trans-Neptunian belt (or Edgeworth-Kuiper belt), can reveal important…

天体物理学 · 物理学 2010-11-11 Patryk Sofia Lykawka , Tadashi Mukai

A new class of Kuiper belt objects that lie beyond Neptune with semimajor axes greater than 250 astronomical units show orbital anomalies that have been interpreted as evidence for an undiscovered ninth planet. We show that a modified…

广义相对论与量子宇宙学 · 物理学 2023-08-25 Katherine Jones-Smith , Harsh Mathur

Trans-Neptunian objects (TNOs) are icy/rocky bodies that move beyond the orbit of Neptune in a region known as the trans-Neptunian belt (or Edgeworth-Kuiper belt). In contrast to the predictions of accretion models that feature…

地球与行星天体物理 · 物理学 2013-06-17 Patryk Sofia Lykawka

Unlike Newtonian dynamics which is linear and obeys the strong equivalence principle, in any nonlinear gravitation such as Milgromian dynamics (MOND), the strong version of the equivalence principle is violated and the gravitational…

星系天体物理 · 物理学 2016-03-23 Hosein Haghi , Amir E. Bazkiaei , Akram Hasani Zonoozi , Pavel Kroupa

Models of "modified-inertia" formulation of MOND are described and applied to nonrelativistic many-body systems. They involve time-nonlocal equations of motion. Momentum, angular momentum, and energy are (nonlocally) defined, whose total…

星系天体物理 · 物理学 2022-10-03 Mordehai Milgrom

The Modified Newtonian Dynamics (MOND) generically predicts a violation of the strong version of the equivalence principle. As a result the gravitational dynamics of a system depends on the external gravitational field in which the system…

宇宙学与河外天体物理 · 物理学 2011-06-01 Luc Blanchet , Jerome Novak

In MOND (modified Newtonian dynamics)-based theories the strong equivalence principle is generically broken in an idiosyncratic manner, manifested in the action of an "external field effect (EFE)". The internal dynamics in a…

星系天体物理 · 物理学 2022-03-30 Kyu-Hyun Chae , 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

It is still an open question how the Solar system is structured beyond 100 au from the Sun. Our understanding of this vast region remains very limited and only recently we have become aware of the existence there of a group of enigmatic…

地球与行星天体物理 · 物理学 2021-07-12 C. de la Fuente Marcos , R. de la Fuente Marcos

Galaxies within galaxy clusters are known to be subject to a wide variety of environmental effects, both gravitational and hydrodynamical. In this study, we examine the purely gravitational interaction of idealised galaxy models falling…

星系天体物理 · 物理学 2018-08-29 G. N. Candlish , R. Smith , Y. Jaffé , A. Cortesi

Context. The paths followed by the known extreme trans-Neptunian objects (ETNOs) effectively avoid direct gravitational perturbations from the four giant planets, yet their orbital eccentricities are in the range between 0.69-0.97. Solar…

地球与行星天体物理 · 物理学 2021-02-19 C. de la Fuente Marcos , R. de la Fuente Marcos

The MOND modified gravity paradigm, best known for its agreement with galactic rotation curve data, is difficult to devise laboratory tests for. MOND's predictions differ substantially from Newtonian gravity only in the case of very small…

星系天体物理 · 物理学 2024-10-03 Benjamin Monreal , Xavier Moskala , Sofia Splawska

The trans-Neptunian region of the solar system exhibits an intricate dynamical structure, much of which can be explained by an instability-driven orbital history of the giant planets. However, the origins of a highly inclined, and in…

地球与行星天体物理 · 物理学 2016-12-14 Konstantin Batygin , Michael E. Brown
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