First of all, I'm not majoring this part and just finding some answer about Arrhenius rate equation: $$v \propto \exp\left(-\frac{E_a}{kT}\right) .$$

To derive this relation, I started with Maxwell-Boltzmann distribution. When there are $N=\sum_j n_j$ particles with energy distribution $$E_{tot} = \sum_j \epsilon_j n_j$$, the disorder number becomes $$\Omega = \frac{N!}{n_1 ! n_2 ! n_3 ! \ldots}.$$ To find when to get the maximum $\Omega$, I used Lagrange multiplyer. Therefore, not considering degeneracy, I got this:$$\textrm{d}(\ln\Omega)=\sum_j\left(\ln \frac{1}{n_j} +\alpha -\beta\epsilon_j\right)\textrm{d}n_j$$ To make $\textrm{d}(\ln\Omega)$ be zero, I obtained $$n(\epsilon)=e^\alpha e^{-\beta\epsilon}.$$

But, the question is how we know that $\beta = \frac{1}{k_B T}$? Somewhere i found that by using $\beta = \frac{\textrm{d}\ln\Omega}{\textrm{d}E}$ and the equation of entropy it is possible. However, I assumed that total energy $E$ is constant so I think $\textrm{d}E$ should be 0. What's the problem in my way?

• You have assumed a constant $E$ and got $\Omega$, moreover, if you assume an another value of $E$, then you get an another $\Omega$ by repeating what you have done. Hence, $\Omega$ is a function of $E$, it is not strange and we can calculate $\frac{d ln \Omega}{d E}$. – qfzklm Sep 9 '15 at 11:40
• In this problem, I cannot understand exactly what another $E$ and another $\Omega$ mean. Could you explain little bit more? Thanks @qfzklm. – Jungmin Kim Sep 9 '15 at 11:46
• For a simple case, let's assmue that $\epsilon=1$ and $E$ is nothing but $N$. Then, assuming $E=1000000$ we can get $\Omega$, and also another $E=1000001$ and another $\Omega$. We can roughly consider $dE$ equal to $1000001-1000000=1$ and obtain $d ln \Omega$. Noted here a large enough particle number is necessary in statistics. – qfzklm Sep 9 '15 at 12:06
• The problem is that statistical mechanics does not describe dynamics. Arrhenius's law is an experimental observation. – Tom-Tom Sep 10 '15 at 20:22

In the derivation of the Boltzmann distribution, one finds the maximum of the function \begin{equation}\ \ln \Omega(\{n_{i}\}) = \ln\!\Big[\Big(\sum_{i} n_{i}\Big)!\Big]-\sum_{i}\ln n_{i}! \end{equation} under the constraints \begin{equation} \sum_{i} n_{i} = N,\quad \sum_{i} n_{i}\epsilon_{i} = E, \end{equation} where the corresponding Lagrange multipliers are respectively called $\alpha$ and $\beta$. The constrained maximum of $\ln \Omega$ occurring at $n_{i} = \exp(-\alpha-\beta\epsilon_{i})$ (i.e., the Boltzmann distribution) is a function of $N$ and $E$. Let's denote it as $\ln \tilde{\Omega}(N,E)$. A theorem on constrained stationary point (which I will state and prove below) guarantees that \begin{equation} \beta = \frac{\partial \ln\tilde{\Omega}}{\partial E}. \end{equation}
Theorem. Suppose that a stationary point of a function $f(\{x_{i}\})$ under a set of constraints $\big\{g_{\alpha}(\{x_{i}\}) = c_{\alpha}\big\}$ occurs at $\big\{\tilde{x}_{i}(\{c_{\alpha}\})\big\}$. Define $\tilde{f}(\{c_{\alpha}\})\equiv f\Big(\Big\{\tilde{x}_{i}\big(\{c_{\alpha}\}\big)\Big\}\Big)$. Then, \begin{equation} \frac{\partial\tilde{f}}{\partial c_{\alpha}} = \lambda_{\alpha}, \end{equation} where $\lambda_{\alpha}$ is the Lagrange multiplier for the $\alpha$-th constraint, i.e., \begin{equation} \left[\frac{\partial f}{\partial x_{i}} - \sum_{\alpha} \lambda_{\alpha}\frac{\partial g_{\alpha}}{\partial x_{i}}\right]_{x_{i}=\tilde{x}_{i}} = 0. \end{equation}