Abstract
We next discuss some elements self-gravitating many body systems.
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Notes
- 1.
We shall assume gravitation according to Newton’s law. For astronomical systems, however, this may entail weak gravitational accelerations on the scale of or less than the cosmic scale \(cH_0\) of the velocity of light c times the Hubble parameter \(H_0\). In this regime, Newton’s law has not yet been established by first principle laboratory experiments.
- 2.
“If one cannot see gravity acting here, he has no soul.” R.P. Feynman, 1995, Six Easy Pieces , (Perseus Books), Chap. 5.
- 3.
- 4.
The tidal sphere has the effect of lowering the potential barrier for stars to escape in the direction \(L_1\) and \(L_2\) [8].
- 5.
For a recent discussion, see, e.g., [14].
- 6.
Possibly, there is further a soft magnetic moment-magnetic moment repulling force between them, induced by Saturn’s 1 Gauss magnetic field, nearly perfectly aligned with its spin axis and orthogonal to Saturn’s disk, that tends to contribute to stability.
References
Zia, R.K., Redish, E.F., & McKay, S.R., 2009, arXiv:0806.1147v2.
Chernoff, D.F., & Djorgovski, S., 1989. ApJ 339, 904.
Chaboyer, B., 2007, Proc. IAU Symp. 248, Eds. Jin, W.J., Platais, I., Perryman, M.A.C.
Richer, H.B. et al., 2004. AJ 127, 2771.
Lynden-Bell, D., Wood, R., 1968, MNRAS, 138, 495; Lynden-Bell, D., Eggleton, P.P., 1980, MNRAS, 191, 483; Lynden-Bell, D., 1988, arXiv/cond-mat/9812172; Antonov, V.A., 1962, Vest. Leningrad Univ. 7, 135 (IAU Symp. 113, 525 (1995).
Chernoff, D., & Djorgovski, S., 1989, ApJ, 339, 904.
van Putten, M.H.P.M., 2012, New A, 17, 411.
Hayli, A., 1967. Bull. Astron. 2, 67.
Aarseth, S.J., 2003, Gravitational \(N\) -Body Simulations (Cambridge: Cambridge University Press).
Ambartsumian, V., 1938, Uch. Zap. LGU, 22, 19; in Dynamics of Star Clusters, Princeton, 1984, eds. J. Goodman & P. Hut (IAU Symposium, No. 113), 1985, p. 521.
van Putten, M.H.P.M., 2012, NewA, 17, 411.
Heggie, D.C., 2001. In: Deiters, S., Fuchs, B., Spurzem, R. Just, A., Wielen R. (Eds.), Dynamics of Star Clusters and the Milky Way, ASP Conference Series, p. 228.
Odenkirchen, M. et al., 1997. New A 2, 477.
Gajda, G., & Lokas, E.L., 2016, ApJ, 819, 20.
Harris, W.E., 2010, Catalogue of parameters for Milky Way Globular Clusters, http://physwww.mcmaster.ca/harris/mwgc.dat.
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van Putten, M.H. (2017). Thermodynamics of N-body Systems. In: Introduction to Methods of Approximation in Physics and Astronomy. Undergraduate Lecture Notes in Physics. Springer, Singapore. https://doi.org/10.1007/978-981-10-2932-5_10
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