Abstract
We introduce a set of order parameters to classify the possible equilibrium states of rotating self-gravitating systems. As an example, the formation and thermodynamics of asymmetric binaries is discussed.
Click here to close this panel.
A. De Martino1, E. V. Votyakov1 and D. H. E. Gross1
2003 EDP Sciences
,
,
Citation A. De Martino et al 2003 EPL 62 14
DOI 10.1209/epl/i2003-00330-9
70 Total downloads
We introduce a set of order parameters to classify the possible equilibrium states of rotating self-gravitating systems. As an example, the formation and thermodynamics of asymmetric binaries is discussed.