Multiplicity (statistical mechanics)
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In statistical mechanics, multiplicity (also called statistical weight) refers to the number of microstates corresponding to a particular macrostate of a
thermodynamic system A thermodynamic system is a body of matter and/or radiation, confined in space by walls, with defined permeabilities, which separate it from its surroundings. The surroundings may include other thermodynamic systems, or physical systems that are ...
. Commonly denoted \Omega, it is related to the configuration entropy of an isolated system via
Boltzmann's entropy formula In statistical mechanics, Boltzmann's equation (also known as the Boltzmann–Planck equation) is a probability equation relating the entropy S, also written as S_\mathrm, of an ideal gas to the multiplicity (commonly denoted as \Omega or W), the ...
S = k_\text \log \Omega, where S is the
entropy Entropy is a scientific concept, as well as a measurable physical property, that is most commonly associated with a state of disorder, randomness, or uncertainty. The term and the concept are used in diverse fields, from classical thermodynam ...
and k_\text = 1.38\cdot 10^ \, \mathrm is
Boltzmann's constant The Boltzmann constant ( or ) is the proportionality factor that relates the average relative kinetic energy of particles in a gas with the thermodynamic temperature of the gas. It occurs in the definitions of the kelvin and the gas constant ...
.


Example: the two-state paramagnet

A simplified model of the two-state paramagnet provides an example of the process of calculating the multiplicity of particular macrostate. This model consists of a system of N microscopic dipoles \mu which may either be aligned or anti-aligned with an externally applied magnetic field B. Let N_\uparrow represent the number of dipoles that are aligned with the external field and N_\downarrow represent the number of anti-aligned dipoles. The energy of a single aligned dipole is U_\uparrow = -\mu B, while the energy of an anti-aligned dipole is U_\downarrow = \mu B; thus the overall energy of the system is U = (N_\downarrow-N_\uparrow)\mu B. The goal is to determine the multiplicity as a function of U; from there, the entropy and other thermodynamic properties of the system can be determined. However, it is useful as an intermediate step to calculate multiplicity as a function of N_\uparrow and N_\downarrow. This approach shows that the number of available macrostates is N+1. For example, in a very small system with N=2 dipoles, there are three macrostates, corresponding to N_\uparrow=0, 1 \, \mathrm \, 2. Since the N_\uparrow = 0 and N_\uparrow = 2 macrostates require both dipoles to be either anti-aligned or aligned, respectively, the multiplicity of either of these states is 1. However, in the N_\uparrow = 1, either dipole can be chosen for the aligned dipole, so the multiplicity is 2. In the general case, the multiplicity of a state, or the number of microstates, with N_\uparrow aligned dipoles follows from combinatorics, resulting in \Omega = \frac = \frac, where the second step follows from the fact that N_\uparrow+N_\downarrow = N. Since N_\uparrow - N_\downarrow = -U/\mu B, the energy U can be related to N_\uparrow and N_\downarrow as follows: \begin N_\uparrow &= \frac - \frac\\ N_\downarrow &= \frac + \frac. \end Thus the final expression for multiplicity as a function of internal energy is \Omega = \frac. This can be used to calculate entropy in accordance with Boltzmann's entropy formula; from there one can calculate other useful properties such as temperature and heat capacity.


References

Statistical mechanics {{Thermodynamics-stub