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Modified Newtonian dynamics ( MOND) is a theory that proposes a modification of Newton's second law to account for observed properties of galaxies. Its primary motivation is to explain galaxy rotation curves without invoking dark matter, and is one of the most well-known theories of this class.
The Modified Newtonian Dynamics (MOND) paradigm was first proposed by Milgrom to reconcile discrepancies between general relativity and galaxy scale dynamics [66]. As presented in its first version, MOND by itself violates conservation of momentum and energy.
Jul 1, 2024 · MOND is an alternative paradigm of dynamics, seeking to replace Newtonian dynamics and general relativity. It aims to account for the ubiquitous mass discrepancies in the Universe, without invoking the dark matter that is required if one adheres to standard dynamics.
tional tests -- is the Modified Newtonian Dynamics. MOND posits a breakdown of Newton's law of gravity (or inertia) below a0, aft.
The Modified Newtonian Dynamics (MOND) s a scientific theory proposed by Moti Milgrom as a solution to the missing mass problem in extragalactic astronomy. Rather than invoking some invisible form of dark matter, it hypothesizes a subtle change to the effective force law at extremely low accelerations (< 10 -10 m/s/s).
Aug 12, 2023 · A study on the orbital motions of wide binaries has uncovered evidence that standard gravity breaks down at low accelerations. This discovery aligns with a modified theory called MOND and challenges current concepts of dark matter.
Dec 5, 2023 · Enter MOND—"modified Newtonian dynamics"—which proposes an adjustment to Newton's second law (nicely encapsulated in the formula that force equals mass multiplied by acceleration) to explain...
1 day ago · Dynamical friction works very differently for Newtonian gravity with dark matter and in modified Newtonian dynamics (MOND). While the absence of dark matter considerably reduces the friction in major galaxy mergers, analytic calculations indicate the opposite for very small perturbations, such as globular clusters (GCs) sinking in dwarf galaxies. Here, we study the decay of GCs in isolated gas-rich dwarf galaxies using simulations with the Phantom of Ramses code, which enables both the ...
