Merge branch 'master' of https://git.overleaf.com/67dbe68df0414d63b309f98a
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main.tex
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main.tex
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\begin{frame}[fragile]{Homogenous Spherical Spaces --- Results}
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\begin{itemize}
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\pause
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\item For the majority of groups $\Gamma$, the anisotropies $\frac{\delta T}{T}$ do not coincide with observations.
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\item For the majority of groups $\Gamma$, the anisotropies $\textcolor{purple}{\frac{\delta T}{T}}$ do not coincide with observations.
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\pause
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\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.
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\pause
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\begin{frame}{Conclusion}
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\pause
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\begin{enumerate}
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\item We can infer the shape of the universe from its spectrum.
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\item We can infer the \textcolor{blue}{shape} of the universe from its \textcolor{blue}{spectrum}.
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\pause
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\item There are two homogeneous spherical manifolds obtained as $\S^3/\Gamma$ which produce CMB similar to observations.
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\item Inhomogeneous spherical spaces exhibit varied behavior of CMB anisotropies.
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\pause
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\item Statistical test results suggest possibilities of finite multi-connected topology.
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\item Statistical test results suggest possibilities of \textcolor{red}{finite multi-connected} topology.
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\end{enumerate}
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\end{frame}
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