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9.2: Thermal Equilibrium

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    107266
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    For a statistical mixture at thermal equilibrium, individual molecules can occupy a distribution of energy states. An equilibrium system at temperature \(T\) has the canonical probability distribution

    \[\rho _ {e q} = \frac {e^{- \beta H}} {Z} \label{8.10}\]

    \(Z\) is the partition function and \(\beta = \left( k _ {B} T \right)^{- 1}\). Classically, we can calculate the equilibrium ensemble average value of a variable \(A\) as

    \[\langle A \rangle = \int d \mathbf {p} \, \int d \mathbf {q} A ( \mathbf {p} , \mathbf {q} ; t ) \rho _ {e q} ( \mathbf {p} , \mathbf {q} ) \label{8.11}\]

    In the quantum mechanical case, we can obtain an equilibrium expectation value of \(A\) by averaging \(\langle A \rangle\) over the thermal occupation of quantum states:

    \[\langle A \rangle = \operatorname {Tr} \left( \rho _ {e q} A \right) \label{8.12}\]

    where \(\rho_{eq}\) is the density matrix at thermal equilibrium and is a diagonal matrix characterized by Boltzmann weighted populations in the quantum states:

    \[\rho _ {m n} = p _ {n} = \frac {e^{- \beta E _ {s}}} {Z} \label{8.13}\]

    In fact, the equilibrium density matrix is defined by Equation \ref{8.10}, as we can see by calculating its matrix elements using

    \[\left( \rho _ {e q} \right) _ {\operatorname {mm}} = \frac {1} {Z} \left\langle n \left| e^{- \beta \hat {H}} \right| m \right\rangle = \frac {e^{- \beta E _ {n}}} {Z} \delta _ {m m} = p _ {n} \delta _ {m m} \label{8.15}\]

    Note also that

    \[Z = \operatorname {Tr} \left( e^{- \beta \hat {H}} \right) \label{8.16}\]

    Equation \ref{8.12} can also be written as

    \[\langle A \rangle = \sum _ {n} p _ {n} \langle n | A | n \rangle \label{8.14}\]

    It may not be obvious how this expression relates to our previous expression for mixed states

    \[\langle A \rangle = \sum _ {n , m} \left\langle c _ {n}^{*} c _ {m} \right\rangle A _ {m n} = \operatorname {Tr} ( \rho \hat {A} ). \]

    Remember that for an equilibrium system we are dealing with a statistical mixture in which no coherences (no phase relationships) are present in the sample. The lack of coherence is the important property that allows the equilibrium ensemble average of \(\left\langle c _ {m} c _ {n}^{*} \right\rangle\) to be equated with the thermal population \(p_n\). To evaluate this average we recognize that these are complex numbers, and that the equilibrium ensemble average of the expansion coefficients is equivalent to phase averaging over the expansion coefficients. Since at equilibrium all phases are equally probable

    \[\left\langle c _ {n}^{*} c _ {m} \right\rangle = \frac {1} {2 \pi} \int _ {0}^{2 \pi} c _ {n}^{*} c _ {m} d \phi = \frac {1} {2 \pi} | c _ {n} \| c _ {m} | \int _ {0}^{2 \pi} e^{- i \phi _ {m n}} d \phi _ {n m} \label{8.17}\]

    where

    \[c _ {n} = \left| c _ {n} \right| e^{i \phi _ {n}}\]

    and

    \[\phi _ {n m} = \phi _ {n} - \phi _ {m}.\]

    The integral in Equation \ref{8.17} is quite clearly zero unless \(\phi _ {n} = \phi _ {m}\) giving

    \[\left\langle c _ {n}^{*} c _ {m} \right\rangle = p _ {n} = \frac {e^{- \beta E _ {s}}} {Z} \label{8.18}\]


    9.2: Thermal Equilibrium is shared under a CC BY-NC-SA 4.0 license and was authored, remixed, and/or curated by Andrei Tokmakoff via source content that was edited to conform to the style and standards of the LibreTexts platform; a detailed edit history is available upon request.

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