Boltzmann distribution

The Boltzmann distribution, formulated in 1868 by Ludwig Boltzmann, describes the probability distribution of objects (particles or oscillation modes) in a system over various energy states, .

It is mathematically expressed as:

where

is the Boltzmann constant.
is the number of objects in the energy state .
is the total number of objects in the system.

The derivation of the Boltzmann distribution equation involves the following steps:

    1. Derivation of the total differential of .
    2. Application of the Lagrange method of undetermined multipliers on the total differential of .
    3. Simplification of solution using Stirling’s approximation.
    4. Evaluation of .

 

Step 1

Consider a system with  molecules randomly occupying different energy states, . The configuration of the system can be represented by with molecules in energy state , molecules in energy state , and so on. The total number of molecules is therefore:

where is the number of molecules in the energy state .

Let’s further define our system as a closed system with total energy, , given by:

The number of ways, , to achieve a configuration of is given by the multinomial permutation:

or in the natural logarithmic form:

 

Question

Eq3 implies that the molecules are distinguishable when they are being assigned to different energy states, and that once these assignments are made, the order of molecules within each state does not matter. Why?

Answer

Boltzmann statistics is rooted in classical physics, where particles of the same type are considered distinguishable because they can be differentiated by their physical states, such as position and velocity. In contrast, particles of the same type in quantum mechanics are considered indistinguishable, which leads to different statistical distributions like Fermi-Dirac statistics for fermions and Bose-Einstein statistics for bosons.

Once the molecules are assigned to energy states, the order of the molecules within each state does not matter, because the configuration is defined only by the number of molecules in each state, not by which specific molecules occupy them.

 

However, the possible configurations that the system may adopt are restricted by eq1 and eq2. For example, the configurations of  and cannot coexist as they have different total energies. Within the allowed set of configurations, the most probable configuration is the one with the largest number of ways of achieving it, i.e. the one whose (or ) is maximal.

We can therefore express the LHS of eq4 in its total differential form of
, or for simplicity:

 

Step 2

The most probable configuration is found by evaluating the maximum point for the function in eq4, i.e.

To solve eq 6, we employ the Lagrange method of undetermined multipliers. We begin by rearranging eq1 to , where is dependent on the rest of the variables, which are all independent. Eq1 can also be written in the form of a new function, :

Likewise, by rearranging eq2 to
we have another dependent variable,  and another function:

This results in eq6 having two dependent variables. The total differential of and are

and

respectively.

Since , we can multiply eq9 and eq10 by the factors and respectively and add them to eq6 to give:

The factors, and , are called Lagrange multipliers. Two of the variables, e.g. and , are dependent variables, while the rest are independent variables. If there is some value of and some value of that render the -th and -th terms of eq11 zero, we have

Consequently, we are left with all independent variables terms. in eq11 can now vary arbitrarily, which implies that all the remaining coefficients equal to zero. Substituting eq9 and eq10 in eq11,

Noting that  and are constants, eq7 and eq8 become and respectively. Substituting and in eq14,

Since all coefficients are now equal to zero,

 

Step 3

To simplify eq16, we rearrange eq4 to give . Since ,

For large , we have . Integrating by parts, . Hence, , which is known as Stirling’s approximation. Eq17 becomes . Since, ,

Substituting eq18 in eq16,

where we have changed the summation index from to in eq19 to discriminate the summation variable from the differentiation variable.

Since , we have . By implicit differentiation, and . Furthermore, . Therefore, eq19 becomes,

Substituting eq20 into eq1 yields , which when substituted into eq20 gives

 

Step 4

An easy way to determine the value of  is to use the equation for the distribution of molecules of an ideal gas in a cylinder:

where

is number of molecules at a height , which implies that is number of molecules in energy state .
is the number of molecules at a height , where . It follows that is number of molecules in energy state .
is the mass of a molecule.
is the acceleration due to gravity.
is the difference in height between and .
is the Avogadro constant
is the universal gas constant

Since represents the difference in energy between states and , we can rewrite eq22 as:

From eq21, the fractions of molecules in energy states and are and respectively. Dividing by ,

Comparing eq23 and 24, , and introducing the constant (the Boltzmann constant), we have

Therefore, eq21 becomes

which is the Boltzmann distribution.

The Boltzmann distribution is used to derive mathematical expressions of many scientific concepts, including the statistical entropy, the Maxwell-Boltzmann distribution, and the Planck radiation law.

 

Question

If the Boltzmann distribution is derived based on distinguishable particles, does it mean that the ideal gas particles described in the barometric formula of eq22 are distinguishable?

Answer

No, the ideal gas particles are indistinguishable. However, whether the particles are distinguishable or not only affects the total statistical weight (also known as the molecular partition function) in eq25. Relative probabilities, such as those expressed by the barometric formula, do not depend on the distinguishability of the particles because the partition function cancels out in the ratio.

 

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