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Part of the book series: Undergraduate Lecture Notes in Physics ((ULNP))

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Abstract

We next discuss some elements self-gravitating many body systems.

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Notes

  1. 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. 2.

    “If one cannot see gravity acting here, he has no soul.” R.P. Feynman, 1995, Six Easy Pieces , (Perseus Books), Chap. 5.

  3. 3.

    E.g., Table 10.1 in [7].

  4. 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. 5.

    For a recent discussion, see, e.g., [14].

  6. 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.

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Correspondence to Maurice H.P.M. van Putten .

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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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