Quantum thermodynamics describes dynamic processes by means of the operators of entropy production P and time t . P and t do not commute. It exists the non-vanishing t – P commutator [ t , P ]= ik . Here the Boltzmann constant k has the physical meaning of a quantum of entropy. The t – P commutator immediately leads us to the t – P uncertainty relation Δ t Δ P ≥ k /2. Hence the observables t and P are not sharply defined simultaneously. Similar uncertainty relations can also be expected for other pairs of conjugate variables with products of the physical meaning of an entropy. The free energy F and the reciprocal temperature (1/ T ) are the respective conjugate variables of an isolated system of many particles, which leads us to the F –(1/ T ) uncertainty relation ǀΔ F ǁΔ(1/ T )ǀ≥ k /2. It can be traced back to the t – P uncertainty relation mentioned above. In this way the Helmholtz free energy F and the temperatur T are introduced into quantum thermodynamics. The uncertainties ǀΔ F ǀ→0 and ǀΔ T ǀ→0 are negligible at low temperatures T →0, and quantum thermodynamics turns into the time-independent classical thermodynamics. Against this the uncertainties ǀΔ F ǀ→∞ and ǀΔ T ǀ→∞ grow unlimited at high temperatures T →∞, and classical thermodynamics loses its sense. In the limit of one particle the uncertainties cannot be neglected even at low temperatures. However a detailed discussion shows that the free energy f of a single particle vanishes within the whole range of temperatures T . This defines the particle entropy σ =ε/ T = ak . The dimensionless entropy number a connects the particle energy ε= akT with the temperature T . The entropy number a of a single (s) independent particle can be calculated with the extended, temperature-dependent Schrödinger equation A s φ=aφ . Here A s =−( Λ 2 /4 π )∇ 2 means the dimensionless entropy operator describing the entropy number a and thus the particle entropy σ = ak . Λ is the thermal de Broglie wave length. Finally we calculate by means of quantized particle entropies σ the internal energy E , the Helmholtz free energy F , the entropy S , the chemical potential μ , and the equation of state of an ideal gas of N monatomic free particles in full agreement with classical thermodynamics. We also calculate the partition function q = V / Λ 3 of a single free particle within the volume V . Here Λ 3 is a small volume element taking into account the wave–particle dualism of a single free particle of mass m at temperature T . Extension to a system of N free particles leads us to a simple geometrical model and to the conclusion that an ideal gas of independent particles becomes instable below a critical temperature T C . T C corresponds to the critical temperature T BE of Bose–Einstein condensation.
Contents
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