Hostname: page-component-78c5997874-v9fdk Total loading time: 0 Render date: 2024-11-20T03:39:08.442Z Has data issue: false hasContentIssue false

Do Stellar Systems Agree with the Singular Evolution of N-Body Systems?

Published online by Cambridge University Press:  14 August 2015

D. Lynden-Bell*
Affiliation:
Institute of Astronomy, The Observatories, Cambridge, U.K.

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

One of the important jobs of scientists is to formulate new laws and principles, and I have attempted to summarise those we have learnt in this most enjoyable and fruitful symposium in the laws stated below. However, recognising that laws derived from stellar dynamics may lead to important discoveries in other fields, I have translated these laws into the language of sociology. The key concept of hard and soft binaries has been introduced into stellar dynamics by Heggie. If at some point in a stellar system is defined to be then Heggie defines a soft binary to be one whose internal energy has β|ε| < 1 and a hard binary to be one with β|ε| > 1. Heggie's laws cover the interaction of these binaries with the field stars and his first basic discovery is that on interacting with this society hard binaries become harder while soft binaries become softer and may even cease to be binaries at all. The same may be true of criminals in their interaction with society.

Type
Part V/General Conclusion and Final Discussion
Copyright
Copyright © Reidel 1975