Abstract
The theory of collisional relaxation in stellar systems is discussed in terms of an expansion in powers of 1/N, the inverse of the total number of stars. The results are expressed in terms of the concept of gravitational polarization.
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© 1972 D. Reidel Publishing Company, Dordrecht, Holland
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Gilbert, I.H. (1972). Collisional Processes in Stellar Systems. In: Lecar, M. (eds) Gravitational N-Body Problem. Astrophysics and Space Science Library, vol 31. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-2870-7_1
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DOI: https://doi.org/10.1007/978-94-010-2870-7_1
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-2872-1
Online ISBN: 978-94-010-2870-7
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