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Modern Engineering Thermodynamics

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18.9 Three Classical Quantum Statistical Models 749<br />

where λ = c/v is the wavelength of the photon. De Broglie then extended the argument to mass particles (like<br />

electrons) by postulating that, for them,<br />

p = mV = ħ λ<br />

where λ is the particle’s wavelength. This postulation was experimentally verified in 1927, when it was demonstrated<br />

that electrons could be diffracted in a wavelike manner from a ruled diffraction surface. Thus, electrons<br />

appeared to have both particlelike and wavelike behavior, and the duality principle of matter was established.<br />

Once the wavelike character of matter was recognized, it became clear that the kinetic behavior of atomic particles<br />

ought to be governed by the same equations that govern the propagation of waves in a continuum. In<br />

1926, Erwin Schrödinger developed an unsteady wave equation appropriate to matter waves of the form<br />

∇ 2 ψ = 2mðε − ε <br />

pÞ ∂ 2 ψ<br />

ε 2 ∂t 2<br />

(18.39)<br />

where ψ is the wave function (the wave amplitude), ε is the total energy of the particle, ε p is the potential energy<br />

of the particle, m is the particle’s mass, and ∇ 2 is the differential operator defined by<br />

∇ 2 ðÞ= ∂2<br />

∂x<br />

∂y<br />

∂z 2 ðÞ<br />

∂2 ∂2<br />

ðÞ+ ðÞ+<br />

2 2<br />

Remarkably, the solutions to (18.39) are inherently quantitized (i.e., solutions exist for only discrete values of ε);<br />

thus, it has become a fundamental equation in quantum mechanics.<br />

18.9 THREE CLASSICAL QUANTUM STATISTICAL MODELS<br />

Consider a system composed of N = ∑N i particles that are distributed in some manner among ε i energy levels.<br />

Then, the total internal energy of the system is U = ∑N i ε i . The most probable distribution (N i ) mp of the N particles<br />

is the one that corresponds to the macrostate with the maximum probability P, and the total internal energy<br />

of that macrostate is U mp = ∑(N i ) mp ε i . Once an equation for W is found, the distribution N i that maximizes it<br />

can easily be found by setting d(W) = 0 subject to the constraint that the total energy and total number of particles<br />

in the system are constant (i.e., dN = dU = 0), and solving for N i = (N i ) mp .<br />

A particle N i has a total energy ε i , which, in general, is made up of a number of energy modes. For example, we<br />

could partition the total energy of the particle into kinetic energy, rotational energy, vibrational energy, and so<br />

forth; and the particle’s total energy can be divided among these modes in many ways. The total number of<br />

arrangements of a particle’s different energy modes that add up to a given energy level ε i is called the degeneracy<br />

of that energy level and is given the symbol g i .<br />

The following three classical statistical models have been developed to describe the basic particle-wave nature of<br />

certain material particles, and their corresponding W and (N i ) mp equations can be found in Table 18.7.<br />

1. The Maxwell-Boltzmann model. 6 Here, all the N i particles are assumed to be indistinguishable from each<br />

other and distributed among various degenerate energy levels. This model accurately represents the behavior<br />

of most simple gases at low pressures.<br />

2. The Fermi-Dirac model. Here, the particles are assumed to be indistinguishable and are distributed among<br />

various degenerate energy levels with only one particle per degeneracy (g i ) value. This model accurately<br />

represents the behavior of electron and proton gases.<br />

3. The Bose-Einstein model. Here, the particles are assumed to be indistinguishable and are distributed among<br />

various degenerate energy levels with no limit on the number of particles per degeneracy. This model<br />

accurately represents the behavior of photon and phonon gases.<br />

The second law of thermodynamics states that S p or _S p ≥ 0, which implies that, at equilibrium, the entropy of a<br />

closed system is a maximum. Also, since thermodynamic equilibrium corresponds to the system’s beinginits<br />

most probable macrostate, it is logical to assume that a functional relation exists between the entropy S of the<br />

system and the statistical probability of the most probable macrostate, W mp . We postulate that this relation has<br />

the form:<br />

S = f ðW mp Þ<br />

6 This is called the “corrected” Maxwell-Boltzmann model in most statistical thermodynamics texts.

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