Mordehai "Moti" Milgrom is an Israeli physicist and professor in the department of Particle Physics and Astrophysics at the Weizmann Institute in Rehovot, Israel.
Mordehai Milgrom | |
|---|---|
 | |
| Born | 1946 |
| Nationality | Israeli |
| Alma mater | Hebrew University Weizmann Institute |
| Known for | Modified Newtonian dynamics |
| Scientific career | |
| Fields | Astrophysics |
| Institutions | Weizmann Institute |
Biography
editHe received his B.Sc. degree from the Hebrew University of Jerusalem in 1966. Later he studied at the Weizmann Institute of Science and completed his doctorate in 1972. Before 1980 he worked primarily on high-energy astrophysics and became well-known for his kinematical model of the star system SS 433.[1][2] In the academic years 1980–1981 and 1985–1986 he was at the Institute for Advanced Study in Princeton.[3] In 1983, he proposed modified Newtonian dynamics (MOND) as an alternative to the dark matter and galaxy rotation curve problems,[4][5][6] although preliminary work and discussions on this subject started as early as 1981.[7]
Milgrom and modified Newtonian dynamics
editMilgrom is a prominent proponent of the hypothesis that Newton's law of universal gravitation should be modified for very small accelerations, typically of the order of 10−11g and less.
Personal life
editMilgrom is married and has three daughters.
See also
edit- Cosmic rays
- Gamma-ray burst
- Gamma ray and x-ray sources.
References
edit- ^ Sanders, R. H. (2014). "A historical perspective on modified Newtonian dynamics". Canadian Journal of Physics. 93 (2): 126–138. arXiv:1404.0531. Bibcode:2015CaJPh..93..126S. doi:10.1139/cjp-2014-0206. S2CID 119240769. page 5 of arXiv.org preprint
- ^ Milgrom, Mordehai (October 1979). "Thomson scattered lines in the spectrum of SS 433 - A powerful tool for studying the system". Astronomy and Astrophysics. 78 (3): L17–L20. Bibcode:1979A&A....78L..17M.
- ^ Mordehai, Milgrom, Community of Scholars Profile, IAS Archived 2016-03-07 at the Wayback Machine
- ^ Milgrom, Mordehai (July 1983). "A modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis". Astrophysical Journal. 270: 365–370. Bibcode:1983ApJ...270..365M. doi:10.1086/161130.
- ^ Milgrom, Mordehai (July 1983). "A modification of the Newtonian dynamics - Implications for galaxies". Astrophysical Journal. 270: 371–383. Bibcode:1983ApJ...270..371M. doi:10.1086/161131.
- ^ Milgrom, Mordehai (July 1983). "A modification of the newtonian dynamics : implications for galaxy systems". Astrophysical Journal. 270: 384–389. Bibcode:1983ApJ...270..384M. doi:10.1086/161132.
- ^ Sanders, RH (February 2015). "A modification of the newtonian dynamics : implications for galaxy systems". Canadian Journal of Physics. 93 (3): 126–138. arXiv:1404.0531. Bibcode:2015CaJPh..93..126S. doi:10.1139/cjp-2014-0206.
Further reading
edit- Milgrom, Mordehai (Aug 2002), "Does Dark Matter Really Exist?" (PDF), Scientific American, pp. 42–50, 52, archived from the original (PDF) on 2004-09-19
- Schilling, Govert (April 2007), "Battlefield Galactica: Dark Matter vs. MOND" (PDF), Sky & Telescope, pp. 30–36
- Zhiping Li, Ran Li. (30 April 2014). "The relativistic astrodynamics of spiral tracks, localized equivalence principle and the dark matter problem of our Milky Way galaxy". Sciencepaper Online.
External links
edit
- MOND - A Pedagogical Review - M. Milgrom, 2001
- M. Milgrom @ Astrophysics Data System
- "MOND: Scale invariance at low accelerations - an alternative to the dark Universe". YouTube. Weizmann Institute of Science. May 11, 2020. Archived from the original on 2021-12-21.
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