MOdified Newtonian Dynamics

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large discrepancy (O(1) or more) • Oort (1932): acceleration of stars perpendicular to Galactic disk • Zwicky (1933): radial velocity of galaxies in Coma cluster • Babcock (1939), Mayall (1951): rotation curve of M31 • Kahn & Woltjer (1959): M31 approaches Milky Way against expansion of universe
large discrepancy (O(1) or more) • Rogstad & Shostak (1972): rotation curve beyond optical disk of spirals from 21 cm • Rubin et al. (1980): rotation curve of optical disk of spirals •… • proper motion of stars near galactic centre (Eckart & Genzel 1997, Ghez et al. 1998) •…
Page 1 and 2: MOdified Newtonian Dynamics applica
Page 3 and 4: mass • dynamical mass - observe m
Page 5: minute discrepancy • existence of
Page 9 and 10: many more rotation curves
Page 11 and 12: acceleration scale • it seems tha
Page 13 and 14: MOND • view as modified gravity i
Page 15 and 16: deep MOND regime Newtonian regime c
Page 17 and 18: gravitational lensing • TeVeS or
Page 19 and 20: angle of deflection of a point mass
Page 21 and 22: mass of lens mass consistent with p
Page 23 and 24: • time delay systems (Danuta & Je
Page 25 and 26: galactic dynamics • Jeans equatio
Page 27 and 28: velocity dispersion • cumulative
Page 29 and 30: • SLACS (Auger et al. 2009) - gal
Page 31 and 32: SDSSJ1204+0358 SDSSJ0946+1006 SDSSJ
Page 33 and 34: acceleration scale from ellipticals
Page 35 and 36: • MOND is in trouble - method is
Page 37: • if it turns out that MOND is on
Page 40 and 41: elative redshift • 3D relative gr
Page 43 and 44: • existence of Neptune - Neptune
Page 45 and 46: tally (2012.05.12) Jean Schneider e

MOdified Newtonian Dynamics

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