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A modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis

The Astrophysical Journal · 1983 · Vol. 270 · pp. 365–365

Abstract

view Abstract Citations (2400) References (10) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS A modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis. Milgrom, M. Abstract The author considers the possibility that there is not, in fact, much hidden mass in galaxies and galaxy systems. If a certain modified version of the Newtonian dynamics is used to describe the motion of bodies in a gravitational field (of a galaxy, say), the observational results are reproduced with no need to assume hidden mass in appreciable quantities. Various characteristics of galaxies result with no further assumptions. The basis of the modification is the assumption that in the limit of small acceleration a very low a0, the acceleration of a particle at distance r from a mass M satisfies approximately a2/a0 ≈ MGr-2, where a0 is a constant of the dimensions of an acceleration. Publication: The Astrophysical Journal Pub Date: July 1983 DOI: 10.1086/161130 Bibcode: 1983ApJ...270..365M Keywords: Cosmology; Galactic Structure; Nonrelativistic Mechanics; Stellar Motions; Particle Acceleration; Solar System; Astrophysics full text sources ADS |

Experimental and Theoretical Physics StudiesSolar and Space Plasma DynamicsRelativity and Gravitational TheoryPhysicsModified Newtonian dynamicsNewtonian dynamicsDynamics (music)AstrophysicsStatistical physicsTheoretical physicsAstronomyGalaxy formation and evolutionGalaxy
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