Difference between revisions of "Outreach"

From Wolverhampton Light and Matter
Jump to: navigation, search
Line 1: Line 1:
Look at this cool equation:
+
Look at this cool equation: \begin{equation}x^2\end{equation}
 +
 
 
\begin{equation*}
 
\begin{equation*}
 +
\centering
 
\label{eq:1}
 
\label{eq:1}
 
g_{{n_1},\cdots,{n_N},\Gamma}^{(N)}(\lbrace \tilde\omega_\mu \rbrace) \equiv \frac{\langle :\Pi_{\mu=1}^{N}{\xi_\mu^\dagger}^{n_\mu} (\tilde\omega_\mu) \xi_\mu^{n_\mu}(\tilde\omega_\mu): \rangle }{\Pi_{\mu=1}^{N} \langle {\xi_\mu^\dagger}^{n_\mu}(\tilde\omega_\mu) \xi_\mu^{n_\mu}(\tilde\omega_\mu) \rangle}\,,
 
g_{{n_1},\cdots,{n_N},\Gamma}^{(N)}(\lbrace \tilde\omega_\mu \rbrace) \equiv \frac{\langle :\Pi_{\mu=1}^{N}{\xi_\mu^\dagger}^{n_\mu} (\tilde\omega_\mu) \xi_\mu^{n_\mu}(\tilde\omega_\mu): \rangle }{\Pi_{\mu=1}^{N} \langle {\xi_\mu^\dagger}^{n_\mu}(\tilde\omega_\mu) \xi_\mu^{n_\mu}(\tilde\omega_\mu) \rangle}\,,
 
\end{equation*}
 
\end{equation*}

Revision as of 14:52, 29 March 2017

Look at this cool equation: \begin{equation}x^2\end{equation}

\begin{equation*} \centering \label{eq:1} g_{{n_1},\cdots,{n_N},\Gamma}^{(N)}(\lbrace \tilde\omega_\mu \rbrace) \equiv \frac{\langle :\Pi_{\mu=1}^{N}{\xi_\mu^\dagger}^{n_\mu} (\tilde\omega_\mu) \xi_\mu^{n_\mu}(\tilde\omega_\mu): \rangle }{\Pi_{\mu=1}^{N} \langle {\xi_\mu^\dagger}^{n_\mu}(\tilde\omega_\mu) \xi_\mu^{n_\mu}(\tilde\omega_\mu) \rangle}\,, \end{equation*}