The DOI matches its Crossref record; 5 of the 5 references it cites were found in a registry or an index.
Modified Newtonian Dynamics as an Alternative to Dark Matter
Open accessAbstract
▪ Abstract Modified Newtonian dynamics (MOND) is an empirically motivated modification of Newtonian gravity or inertia suggested by Milgrom as an alternative to cosmic dark matter. The basic idea is that at accelerations below a o≈ 10−8 cm/s 2≈ cH o/6 the effective gravitational attraction approaches [Formula: see text], where g n is the usual Newtonian acceleration. This simple algorithm yields flat rotation curves for spiral galaxies and a mass-rotation velocity relation of the form M ∝ V 4 that forms the basis for the observed luminosity–rotation velocity relation—the Tully-Fisher law. We review the phenomenological success of MOND on scales ranging from dwarf spheroidal galaxies to superclusters and demonstrate that the evidence for dark matter can be equally well interpreted as evidence for MOND. We discuss the possible physical basis for an acceleration-based modification of Newtonian dynamics as well as the extention of MOND to cosmology and structure formation.
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Cites
Measurements of Ω and Λ from 42 High‐Redshift Supernovae
Perlmutter, S., Aldering, G., Goldhaber, G., Knop, R. A., Nugent, P., Castro, P. G., Deustua, S., Fabbro, S., Goobar, A., Groom, D. E., et al. (1999) · The Astrophysical Journal · doi:10.1086/307221 · Cited by 18,062
The Structure of Cold Dark Matter Halos
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1996) · The Astrophysical Journal · doi:10.1086/177173 · Cited by 8,544 · cited 1×
“…high precision and resolution, this hypothesis has gained predictive power on the scale of galaxies– a power that considerably restricts the freedom to arrange dark matter as one would wish in order to explain the form and magnitude of the discrepancy in any particular system (Navarro et al. 1996).”
BackgroundMach's Principle and a Relativistic Theory of Gravitation
Brans, C., & Dicke, R. H. (1961) · Physical Review · doi:10.1103/physrev.124.925 · Cited by 5,621
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 · Cited by 3,316
A Modification of the Newtonian Dynamics - Implications for Galaxy Systems
Milgrom, M. (1983) · The Astrophysical Journal · doi:10.1086/161132 · Cited by 527
Cited by
Relativistic gravitation theory for the modified Newtonian dynamics paradigm
Bekenstein, J. D. (2004) · Physical Review D · doi:10.1103/physrevd.70.083509 · Cited by 1,487
Beyond the cosmological standard model
Joyce, A., Jain, B., Khoury, J., & Trodden, M. (2015) · Physics Reports · doi:10.1016/j.physrep.2014.12.002 · Cited by 1,231
Cosmology and Fundamental Physics with the Euclid Satellite
The Euclid Theory Working Group, Amendola, L., Appleby, S., Bacon, D., Baker, T., Baldi, M., Bartolo, N., Blanchard, A., Bonvin, C., Borgani, S., et al. (2013) · Living Reviews in Relativity · doi:10.12942/lrr-2013-6 · Cited by 899
Clowe, D., Gonzalez, A., & Markevitch, M. (2004) · The Astrophysical Journal · doi:10.1086/381970 · Cited by 638
Galactic‐Field Initial Mass Functions of Massive Stars
Kroupa, P., & Weidner, C. (2003) · The Astrophysical Journal · doi:10.1086/379105 · Cited by 522
Metadata
- Authors
- Sanders, R. H., & McGaugh, S. S.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 2002-09
- Volume
- 40
- Issue
- 1
- Pages
- 263-317
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2115399036
- Cited by
- 723
- References
- 5
- FWCI
- 1.90
- Type
- journal article
- Language
- en
- Open access
- green
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