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prescientmoon 2025-03-21 13:56:43 +01:00
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@ -121,7 +121,7 @@ code-for-last-col = \color{blue}
\begin{frame}[fragile]{Homogenous Spherical Spaces --- Results}
\begin{itemize}
\pause
\item For the majority of groups $\Gamma$, the anisotropies $\frac{\delta T}{T}$ do not coincide with observations.
\item For the majority of groups $\Gamma$, the anisotropies $\textcolor{purple}{\frac{\delta T}{T}}$ do not coincide with observations.
\pause
\item The only groups for which they do are $\Gamma = O^*$ and $\Gamma = I^*$ — the \textcolor{red}{binary octahedral} and \textcolor{red}{binary icosahedral} groups of order 48 and 120 respectively.
\pause
@ -236,7 +236,7 @@ code-for-last-col = \color{blue}
\begin{frame}{Conclusion}
\pause
\begin{enumerate}
\item We can infer the shape of the universe from its spectrum.
\item We can infer the \textcolor{blue}{shape} of the universe from its \textcolor{blue}{spectrum}.
\pause
\item There are two homogeneous spherical manifolds obtained as $\S^3/\Gamma$ which produce CMB similar to observations.
@ -245,7 +245,7 @@ code-for-last-col = \color{blue}
\item Inhomogeneous spherical spaces exhibit varied behavior of CMB anisotropies.
\pause
\item Statistical test results suggest possibilities of finite multi-connected topology.
\item Statistical test results suggest possibilities of \textcolor{red}{finite multi-connected} topology.
\end{enumerate}
\end{frame}