Gravitational Thermodynamics

dc.creatorHut, Piet
dc.date1997-04-29
dc.date.accessioned2026-07-07T02:23:18Z
dc.date.available2026-07-07T02:23:18Z
dc.descriptionThe gravitational N-body problem, for $N>2$, is the oldest unsolved problem in mathematical physics. Some of the most ideal examples that can be found in nature are globular star clusters, with $N \sim 10^6$. In this overview, I discuss six types of fundamental sources of unpredictability, each of which poses a different challenge to attempts to determine the long-term behavior of these systems, governed by a peculiar type of thermodynamics.
dc.description19 pages, 5 included figures, Tex, uses psfig.tex. To appear in `Complexity', as part of the Proceedings of the Workshop on Fundamental Sources of Unpredictability, held at the Santa Fe Institute, March 28-30, 1996, eds. James Hartle, Piet Hut, and Joseph Traub
dc.identifierhttps://arxiv.org/abs/astro-ph/9704286
dc.identifierhttp://arxiv.org/abs/astro-ph/9704286
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/11197
dc.subjectAstrophysics
dc.titleGravitational Thermodynamics
dc.typetext

Files

Collections