Cited by 3,316Cosmology and Gravitation TheoriesGalaxies: Formation, Evolution, PhenomenaStellar, planetary, and galactic studies

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

Milgrom, M.·1983·The Astrophysical Journal

DOI 10.1086/161130

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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 |

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Kroupa, P. (2012) · Publications of the Astronomical Society of Australia · doi:10.1071/as12005 · Cited by 230
“In both cases, effective gravity would be non-Newtonian and is described by Mordehai Milgrom’s formulation (Milgrom 1983a).”
Influential
Clusters of galaxies with modified Newtonian dynamics
Sanders, R. H. (2003) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2003.06596.x · Cited by 244
New Relativistic Theory for Modified Newtonian Dynamics
Skordis, C., & Zlosnik, T. G. (2021) · Physical Review Letters · doi:10.1103/physrevlett.127.161302 · Cited by 219
Local-Group tests of dark-matter concordance cosmology
Kroupa, P., Famaey, B., de Boer, K. S., Dabringhausen, J., Pawlowski, M. S., Boily, C. M., Jerjen, H., Forbes, D. A., Hensler, G., & Metz, M. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201014892 · Cited by 257
NGC 3741: the dark halo profile from the most extended rotation curve
Gentile, G., Salucci, P., Klein, U., & Granato, G. L. (2006) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2006.11283.x · Cited by 218
H I KINEMATICS AND DYNAMICS OF MESSIER 31
Chemin, L., Claude Carignan, A., & Foster, T. (2009) · The Astrophysical Journal · doi:10.1088/0004-637x/705/2/1395 · Cited by 221
Cosmic distance-duality as a probe of exotic physics and acceleration
Bassett, B. A., & Kunz, M. (2004) · Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields · doi:10.1103/physrevd.69.101305 · Cited by 215
The MOG weak field approximation and observational test of galaxy rotation curves
Moffat, J. W., & Rahvar, S. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stt1670 · Cited by 208
“There are various approaches to modifying gravity, such as MOdified Newtonian Dynamics (MOND) or its relativistic version the so-called Tensor–Vector–Scalar (TeVeS) theory (Milgrom 1983; Bekenstein 2004).”
Method
Dark matter, dark energy, and alternate models: A review
Arun, K., Gudennavar, S. B., & Sivaram, C. (2017) · Advances in Space Research · doi:10.1016/j.asr.2017.03.043 · Cited by 209
“Perhaps critical acceleration is given as 00 cHa ª and it is related to cosmological constant by Lª 2 0 ca (Sivaram, 1994a, Milgrom, 1983a).”
BackgroundMethod

Authors: Milgrom, M.
Corresponding author: Milgrom, M.
Venue: The Astrophysical Journal
Publisher: American Astronomical Society
Published: 1983-07
Volume: 270
Pages: 365
ISSN: 0004-637X (ISSN-L)
1538-4357
DOI: 10.1086/161130
OpenAlex: W1990148897
Cited by: 3,316
References: 0
Citations by year: 2026: 147 · 2025: 181 · 2024: 191 · 2023: 187 · 2022: 155 · 2021: 200 · 2020: 191 · 2019: 165 · 2018: 189 · 2017: 149 · 2016: 146 · 2015: 138 · 2014: 135 · 2013: 122 · 2012: 122
FWCI: 6.70
Type: journal article
Language: en
Open access: closed
Locations: The Astrophysical Journal (publishedVersion)
Topics: Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
Keywords: MOND, dark matter, galaxy rotation curves, hidden mass, galaxy dynamics, modified gravity

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

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