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-rw-r--r--source/know/concept/bose-einstein-distribution/index.md36
1 files changed, 18 insertions, 18 deletions
diff --git a/source/know/concept/bose-einstein-distribution/index.md b/source/know/concept/bose-einstein-distribution/index.md
index 5640e69..ea5ca68 100644
--- a/source/know/concept/bose-einstein-distribution/index.md
+++ b/source/know/concept/bose-einstein-distribution/index.md
@@ -14,19 +14,19 @@ which do not obey the [Pauli exclusion principle](/know/concept/pauli-exclusion-
distribute themselves across the available states
in a system at equilibrium.
-Consider a single-particle state $$s$$,
+Consider a single-particle state $$\ket{i}$$,
which can contain any number of bosons.
-Since the occupation number $$N$$ is variable,
+Since the occupation number $$n_i$$ is variable,
we use the [grand canonical ensemble](/know/concept/grand-canonical-ensemble/),
whose grand partition function $$\mathcal{Z}$$ is as shown below,
-where $$\varepsilon$$ is the energy per particle,
+where $$\varepsilon_i$$ is the energy per particle,
and $$\mu$$ is the chemical potential.
We evaluate the sum in $$\mathcal{Z}$$ as a geometric series:
$$\begin{aligned}
\mathcal{Z}
- = \sum_{N = 0}^\infty \Big( e^{-\beta (\varepsilon - \mu)} \Big)^{N}
- = \frac{1}{1 - e^{-\beta (\varepsilon - \mu)}}
+ = \sum_{m = 0}^\infty \Big( e^{-\beta (\varepsilon_i - \mu)} \Big)^{m}
+ = \frac{1}{1 - e^{-\beta (\varepsilon_i - \mu)}}
\end{aligned}$$
The corresponding [thermodynamic potential](/know/concept/thermodynamic-potential/)
@@ -35,42 +35,42 @@ is the Landau potential $$\Omega$$, given by:
$$\begin{aligned}
\Omega
= - k T \ln{\mathcal{Z}}
- = k T \ln\!\big( 1 - e^{-\beta (\varepsilon - \mu)} \big)
+ = k T \ln\!\big( 1 - e^{-\beta (\varepsilon_i - \mu)} \big)
\end{aligned}$$
-The average number of particles $$\expval{N}$$ in $$s$$
+The average number of particles $$\expval{n_i}$$ in $$\ket{i}$$
is then found by taking a derivative of $$\Omega$$:
$$\begin{aligned}
- \expval{N}
+ \expval{n_i}
= - \pdv{\Omega}{\mu}
= k T \pdv{\ln{\mathcal{Z}}}{\mu}
- = \frac{e^{-\beta (\varepsilon - \mu)}}{1 - e^{-\beta (\varepsilon - \mu)}}
+ = \frac{e^{-\beta (\varepsilon_i - \mu)}}{1 - e^{-\beta (\varepsilon_i - \mu)}}
\end{aligned}$$
-By multiplying both the numerator and the denominator by $$e^{\beta(\varepsilon \!-\! \mu)}$$,
+By multiplying both the numerator and the denominator by $$e^{\beta(\varepsilon_i - \mu)}$$,
we arrive at the standard form of the **Bose-Einstein distribution** $$f_B$$:
$$\begin{aligned}
\boxed{
- \expval{N}
- = f_B(\varepsilon)
- = \frac{1}{e^{\beta (\varepsilon - \mu)} - 1}
+ \expval{n_i}
+ = f_B(\varepsilon_i)
+ = \frac{1}{e^{\beta (\varepsilon_i - \mu)} - 1}
}
\end{aligned}$$
-This gives the expected occupation number $$\expval{N}$$
-of state $$s$$ with energy $$\varepsilon$$,
+This gives the expected occupation number $$\expval{n_i}$$
+of state $$\ket{i}$$ with energy $$\varepsilon_i$$,
given a temperature $$T$$ and chemical potential $$\mu$$.
{% comment %}
-The corresponding variance $$\sigma^2 \equiv \expval{N^2} - \expval{N}^2$$ is found to be:
+The corresponding variance $$\sigma^2 \equiv \expval{n_i^2} - \expval{n_i}^2$$ is found to be:
$$\begin{aligned}
\boxed{
\sigma^2
- = k T \pdv{\expval{N}}{\mu}
- = \expval{N} \big(1 + \expval{N}\!\big)
+ = k T \pdv{\expval{n_i}}{\mu}
+ = \expval{n_i} \big(1 + \expval{n_i}\!\big)
}
\end{aligned}$$
{% endcomment %}