MOdified Newtonian Dynamics (MOND) tavânik-e niyutoni-ye vâtarzidé Fr.: dynamique newtonienne modifiée A modification of the Newton’s law of gravitation below a critical acceleration of
about 1.2 x 10-8 cm s-2, where the gravitational force scales
as 1/r instead of 1/r2. Originally put forward to
describe the rotation curves of
galaxies with no need to assume any dark matter, Etymology (EN): → modify; → Newtonian dynamics. |