Thermo-Statistical description of the Hamiltonian non extensive systems: The selfsimilarity scaling laws

dc.creatorVelazquez, L.
dc.creatorGuzman, F.
dc.date2006-04-11
dc.date2006-04-21
dc.date.accessioned2026-07-07T07:05:26Z
dc.date.available2026-07-07T07:05:26Z
dc.descriptionThe foundations for a thermo-statistical description of the called non extensive Hamiltonian systems are reconsidered. The relevance of the parametric resonance as a fundamental mechanism of the Hamiltonian chaoticity in those systems with bound motions in the configurational space is discussed. The universality of this mechanism suggests us the possibility of performing a thermo-statistical description with microcanonical basis in the context of the long-range interacting Hamiltonian systems. The concept of selfsimilarity is proposed as an appropriate generalization of the well-known extensive conditions exhibited by the traditional systems, which is used to justify a given generalized thermodynamic formalism starting from the consideration of the microcanonical ensemble, i.e. the nonextensive Statistics of Tsallis. These ideas are illustrated by considering a recent proposed astrophysical model based on the quasi-ergodic character of the microscopic dynamics of these paradigmatic examples of real long-range interacting systems.
dc.descriptionReview of PhD thesis with 10 pages and 3 eps figures (Revised version)
dc.identifierhttps://arxiv.org/abs/cond-mat/0604290
dc.identifierhttp://arxiv.org/abs/cond-mat/0604290
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/109668
dc.subjectStatistical Mechanics
dc.titleThermo-Statistical description of the Hamiltonian non extensive systems: The selfsimilarity scaling laws
dc.typetext

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