Math Extension¶

LATEX is the gold standard for math notation. TeXSmith relies on the same syntax that MathJax/Arithmatex understand.

Inline Math¶

Inline math uses the usual delimiters $ ... $ or $ ... $ :

The quadratic formula is given by \(x = \frac{-b \pm \sqrt{b^2 - 4ac}}{2a}\)
or $x = \frac{-b \pm \sqrt{b^2 - 4ac}}{2a}$.

Rendered as:

The quadratic formula is given by $x = \frac{-b \pm \sqrt{b^2 - 4ac}}{2a}$ or $x = \frac{-b \pm \sqrt{b^2 - 4ac}}{2a}$.

Note

Skip the spaces right after $ or \(—they confuse the parser.

Block Math¶

Simple equations¶

Example: Schrödinger’s equation in the non-relativistic case:

$$
\imath \hbar \frac{\partial}{\partial t} \Psi(\mathbf{r},t) =
\left[ -\frac{\hbar^2}{2m} \nabla^2 + V(\mathbf{r},t) \right] \Psi(\mathbf{r},t)
$$

\[ \imath \hbar \frac{\partial}{\partial t} \Psi(\mathbf{r},t) = \left[ -\frac{\hbar^2}{2m} \nabla^2 + V(\mathbf{r},t) \right] \Psi(\mathbf{r},t) \]

Multiple equations¶

$$
\begin{align*}
\nabla \cdot \vec{E} &= \frac{\rho}{\varepsilon_0} \quad &&\text{Gauss Law}\\[4pt]
\nabla \cdot \vec{B} &= 0 \quad &&\text{Gauss's law for electricity}\\[4pt]
\nabla \times \vec{E} &= -\,\frac{\partial \vec{B}}{\partial t}
    \quad &&\text{Faraday's law}\\[4pt]
\nabla \times \vec{B} &= \mu_0 \vec{J} + \mu_0 \varepsilon_0
    \frac{\partial \vec{E}}{\partial t}
\quad &&\text{Ampère-Maxwell law}
\end{align*}
$$

\[ \begin{align*} \nabla \cdot \vec{E} &= \frac{\rho}{\varepsilon_0} \quad &&\text{Gauss Law}\\[4pt] \nabla \cdot \vec{B} &= 0 \quad &&\text{Gauss's law for electricity}\\[4pt] \nabla \times \vec{E} &= -\,\frac{\partial \vec{B}}{\partial t} \quad &&\text{Faraday's law}\\[4pt] \nabla \times \vec{B} &= \mu_0 \vec{J} + \mu_0 \varepsilon_0 \frac{\partial \vec{E}}{\partial t} \quad &&\text{Ampère-Maxwell law} \end{align*} \]

Numbered equation¶

Wrap an equation inside \begin{equation}...\end{equation} (or equation*) to control numbering. Example: the relativistic gravitational field equation:

The equation $\eqref{eq:gravity}$ describes the fundamental interaction of
gravitation as a result of spacetime being curved by matter and energy.

$$
\begin{equation} \label{eq:gravity}
R_{\mu \nu} - \frac{1}{2} R g_{\mu \nu} + \Lambda g_{\mu \nu} =
    \frac{8 \pi G}{c^4} T_{\mu \nu}
\end{equation}
$$

The equation $\eqref{eq:gravity}$ describes the fundamental interaction of gravitation as a result of spacetime being curved by matter and energy.

\[ \begin{equation} \label{eq:gravity} R_{\mu \nu} - \frac{1}{2} R g_{\mu \nu} + \Lambda g_{\mu \nu} = \frac{8 \pi G}{c^4} T_{\mu \nu} \end{equation} \]

Reference numbered equations via \label{} and drop $\eqref{...}$ in Markdown.

In an aligned environment, you can number individual lines using the \label{} command:

As we see in $\eqref{eq:max2}$, the magnetic flux through any closed surface is zero;
this implies that there are no magnetic monopoles.

$$
\begin{align}
\oint_{\partial V} \vec{E} \cdot d\vec{S} &= \frac{Q_{\text{int}}}{\varepsilon_0}
    \label{eq:max1} \\[6pt]
\oint_{\partial V} \vec{B} \cdot d\vec{S} &= 0 \label{eq:max2} \\[6pt]
\oint_{\partial S} \vec{E} \cdot d\vec{\ell} &= -\,\frac{d}{dt} \int_{S} \vec{B}
    \cdot d\vec{S} \label{eq:max3} \\[6pt]
\oint_{\partial S} \vec{B} \cdot d\vec{\ell} &= \mu_0 I_{\text{int}}
+ \mu_0 \varepsilon_0 \frac{d}{dt} \int_{S} \vec{E} \cdot d\vec{S} \label{eq:max4}
\end{align}
$$

As we see in $\eqref{eq:max2}$, the magnetic flux through a closed surface is zero, implying the lack of magnetic monopoles.

\[ \begin{align} \oint_{\partial V} \vec{E} \cdot d\vec{S} &= \frac{Q_{\text{int}}}{\varepsilon_0} \label{eq:max1} \\[6pt] \oint_{\partial V} \vec{B} \cdot d\vec{S} &= 0 \label{eq:max2} \\[6pt] \oint_{\partial S} \vec{E} \cdot d\vec{\ell} &= -\,\frac{d}{dt} \int_{S} \vec{B} \cdot d\vec{S} \label{eq:max3} \\[6pt] \oint_{\partial S} \vec{B} \cdot d\vec{\ell} &= \mu_0 I_{\text{int}} + \mu_0 \varepsilon_0 \frac{d}{dt} \int_{S} \vec{E} \cdot d\vec{S} \label{eq:max4} \end{align} \]

MkDocs Configuration¶

Running under MkDocs? Enable Arithmatex/MathJax and let it handle numbering:

markdown_extensions:
  - pymdownx.arithmatex:
      generic: true
extra_javascript:
  - js/mathjax.js
  - https://unpkg.com/mathjax@3/es5/tex-mml-chtml.js

In the js/mathjax.js file, include the following MathJax configuration:

window.MathJax = {
  tex: {
    inlineMath: [['\\(', '\\)']],
    displayMath: [['$$', '$$'], ['\\[', '\\]']],
    tags: 'ams',
    packages: {'[+]': ['ams']}
  },
  options: {
    ignoreHtmlClass: '.*',
    processHtmlClass: 'arithmatex'
  }
};

With LATEX output¶

Here’s what the above snippets look like once rendered through TeXSmith:

With the source:

The Schrödinger equation in a non-relativistic case is written as:

$$
\imath \hbar \frac{\partial}{\partial t} \Psi(\mathbf{r},t) =
\left[ -\frac{\hbar^2}{2m} \nabla^2 + V(\mathbf{r},t) \right] \Psi(\mathbf{r},t)
$$

And the set of Maxwell's equations in differential form. The magnetic flux $\eqref{eq:max2}$ through any closed surface is zero, which implies that there are no magnetic monopoles.

$$
\begin{align}
\nabla \cdot \vec{E} &= \frac{\rho}{\varepsilon_0} \quad &&\text{Gauss Law}\\[4pt]
\nabla \cdot \vec{B} &= 0 \quad &&\text{Gauss's law for electricity} \label{eq:max2}\\[4pt]
\nabla \times \vec{E} &= -\,\frac{\partial \vec{B}}{\partial t}
    \quad &&\text{Faraday's law}\\[4pt]
\nabla \times \vec{B} &= \mu_0 \vec{J} + \mu_0 \varepsilon_0
    \frac{\partial \vec{E}}{\partial t}
\quad &&\text{Ampère-Maxwell law}
\end{align}
$$