Asymmetric binaries and hierarchy of states in self-gravitating systems

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dc.creatorDe Martino, A.
dc.creatorVotyakov, E. V.
dc.creatorGross, D. H. E.
dc.date2002-10-31
dc.date.accessioned2026-07-07T02:48:00Z
dc.date.available2026-07-07T02:48:00Z
dc.descriptionWe complete the analysis of the equilibrium shapes of rotating self-gravitating gases initiated in Phys. Rev. Lett. 89 031101 (2002) (cond-mat/0202140) by studying the formation and thermodynamics of asymmetric binaries and by introducing a family of order parameters to classify the possible equilibrium states.
dc.description4 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/cond-mat/0210707
dc.identifierhttp://arxiv.org/abs/cond-mat/0210707
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/20232
dc.subjectStatistical Mechanics
dc.subjectAstrophysics
dc.titleAsymmetric binaries and hierarchy of states in self-gravitating systems
dc.typetext

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