1.6 KiB
1.6 KiB
title | description | lead | date | lastmod | draft | images | menu | weight | toc | ||||
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Math | Math typesetting examples. | Math typesetting examples. | 2021-03-16T10:46:05+01:00 | 2021-03-16T10:46:05+01:00 | false |
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KaTeX 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
Markdown
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.