Abstract
A possible connection between MOND (Modification of Newtonian Dynamics) proposed as an alternative hypothesis to dark matter in galaxies and clusters and a residual cosmological constant term dominating cosmological dynamics in a Ω = 1 universe is explored.
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Milgrom, M.: 1983,Astrophys. J. 270, 365.
Milgrom, M. and Sanders, R.: 1993,Nature 362, 25.
Sivaram, C.: 1979,Phys. Reports 51, 111.
Sivaram, C.: 1982,Amer. J. Phys. 50, 279.
Sivaram, C.: 1982,Astrophys. Space Sci. 82, 507.
Sivaram, C.: 1983,Amer. J. Phys. 51, 277.
Sivaram, C.: 1986a,Astrophys. Space Sci. 125, 189.
Sivaram, C.: 1986b,Intern. J. Theor. Phys. 26, 825.
Sivaram, C.: 1986c,Astrophys. Space Sci. 127, 133.
Sivaram, C.: 1987,Nature 327, 108.
Sivaram, C.: 1990,Astrophys. Space Sci. 167, 335.
Sivaram, C.: 1993a,Astron. Astrophys. 275, 37.
Sivaram, C.: 1993b,Astrophys. Space Sci., (in press).
Sivaram, C.: 1993c, in: T. Ho (ed.),Cosmology and Elementary Particles, NATO ASI, Kluwer Acad. Publ., (in press).
Sivaram, C.: 1994,Found. Phys. Lett., (in press).
Yoshii, Y.: 1993a,b,Astrophys. J. 403, 522;Astrophys. J. 418, L1.
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Sivaram, C. Mond, dark matter and the cosmological constant. Astrophys Space Sci 219, 135–141 (1994). https://doi.org/10.1007/BF00657864
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DOI: https://doi.org/10.1007/BF00657864