feat: add doks as a node module

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Henk Verlinde 2021-03-18 15:50:09 +01:00
commit cfed05efaf
55 changed files with 26751 additions and 0 deletions

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---
title: "Examples"
description: "Examples"
lead: ""
date: 2021-03-16T08:43:03+01:00
lastmod: 2021-03-16T08:43:03+01:00
draft: false
images: []
---

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---
title: "Code"
description: "Code highlighting examples."
lead: "Code highlighting examples."
date: 2021-03-16T08:43:34+01:00
lastmod: 2021-03-16T08:43:34+01:00
draft: false
images: []
menu:
docs:
parent: "examples"
weight: 200
toc: true
---
## JavaScript
```js
function $initHighlight(block, cls) {
try {
if (cls.search(/\bno\-highlight\b/) != -1)
return process(block, true, 0x0F) +
` class="${cls}"`;
} catch (e) {
/* handle exception */
}
for (var i = 0 / 2; i < classes.length; i++) {
if (checkCondition(classes[i]) === undefined)
console.log('undefined');
}
return (
<div>
<web-component>{block}</web-component>
</div>
)
}
export $initHighlight;
```
## JSON
```json
[
{
"title": "apples",
"count": [12000, 20000],
"description": {"text": "...", "sensitive": false}
},
{
"title": "oranges",
"count": [17500, null],
"description": {"text": "...", "sensitive": false}
}
]
```
## Bash
```bash
#!/bin/bash
###### CONFIG
ACCEPTED_HOSTS="/root/.hag_accepted.conf"
BE_VERBOSE=false
if [ "$UID" -ne 0 ]
then
echo "Superuser rights required"
exit 2
fi
genApacheConf(){
echo -e "# Host ${HOME_DIR}$1/$2 :"
}
echo '"quoted"' | tr -d \" > text.txt
```

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---
title: "Math"
description: "Math typesetting examples."
lead: "Math typesetting examples."
date: 2021-03-16T10:46:05+01:00
lastmod: 2021-03-16T10:46:05+01:00
draft: false
images: []
menu:
docs:
parent: "examples"
weight: 210
toc: true
---
[KaTeX](https://katex.org/) is switched off by default. Enable it by setting `kaTex = true` in the `[options]` section of `./config/_default/params.toml`.
## Example 1
_Excerpt taken from [Supernova Neutrinos](https://neutrino.leima.is/book/introduction/supernova-neutrinos/)_
### Markdown
```md
The average energy of the neutrinos $\langle E \rangle$ emitted during a supernova explosion is of the order of 10MeV, and the neutrino luminosity at the early epoch of the explosion is approximately $10^{52}\mathrm{ergs\cdot s^{-1}}$.
Therefore, the number density of the neutrinos at the radius $R$ is
$$
\begin{equation*}
n \sim 10^{18} \mathrm{cm^{-3}} \left(\frac{100\mathrm{km}}{R}\right)^2 \left(\frac{10\mathrm{MeV}}{\langle E \rangle}\right).
\end{equation*}
$$
```
### HTML
The average energy of the neutrinos $\langle E \rangle$ emitted during a supernova explosion is of the order of 10MeV, and the neutrino luminosity at the early epoch of the explosion is approximately $10^{52}\mathrm{ergs\cdot s^{-1}}$.
Therefore, the number density of the neutrinos at the radius $R$ is
$$
\begin{equation*}
n \sim 10^{18} \mathrm{cm^{-3}} \left(\frac{100\mathrm{km}}{R}\right)^2 \left(\frac{10\mathrm{MeV}}{\langle E \rangle}\right).
\end{equation*}
$$
It turns out that the ambient dense neutrino medium has a significant impact on neutrino oscillations, which has been intensely investigated in the last decade.