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Nonextensive Statistical Mechanics

Nonextensive Statistical Mechanics

Nonextensive Statistical Mechanics

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2.4 Boltzmann–Gibbs <strong>Statistical</strong> <strong>Mechanics</strong> and Thermodynamics 35concepts and statistical mechanics provide the correct connection between microscopicand macroscopic laws for a vast class of physical systems. But – we insist –the mathematically precise qualification of this class remains an open question.2.4.1 Isolated System – Microcanonical EnsembleIn this and subsequent subsections, we briefly review BG statistical mechanics (see,for instance, [35]). We consider a quantum Hamiltonian system constituted by N interactingparticles under specific boundary conditions, and denote by {E i } its energyeigenvalues.The microcanonical ensemble corresponds to an isolated N-particle systemwhose total energy U is known within some precision δU (tobeinfacttakenatits zero limit at the appropriate mathematical stage). The number of states i withU ≤ E i ≤ U + δU is denoted by W . Assuming that the system is such that itsdynamics leads to ergodicity at its stationary state (thermal equilibrium), we assumethat all such states are equally probable, i.e., p i = 1/W , and the entropy is given byEq. (1.3). The temperature T is introduced through1T ≡ S BGU= k ln WU . (2.62)2.4.2 In the Presence of a Thermostat – Canonical EnsembleThe canonical ensemble corresponds to an N-particle system defined in a Hilbertspace whose dimension is noted W , and which is in longstanding thermal contactwith a (infinitely large) thermostat at temperature T . Its exact energy is unknown,but its mean energy U is known since it is determined by the thermostat. We mustoptimize the entropy given by Eq. (1.1) with the norm constraint (1.2), and with theenergy constraintW∑p i E i = U . (2.63)i=1Following along the lines of Section 2.3, we obtain the celebrated BG weightwith the partition function given byp i = e−β E iZ BG, (2.64)Z BG ≡W∑e −β E i, (2.65)i=1the Lagrange parameter β being related with the temperature through β ≡ 1/(kT).

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