6.7.3 UV finiteness
\subsection{String compactifications} [1]<ol><li>Grana:2005jc</li><li>Anderson:2018pui</li><li>Font:2005td</li><li>McAllister:2023vgy</li><li>Alexandrov:2011va</li><li>VanRiet:2023pnx</li><li>Douglas:2006es</li><li>Denef:2008wq</li></ol>. See [2]<ol><li>Banks:2012hx</li></ol> for a critique of the string landscape.
\subsubsection{Scale separation} [3]<ol><li>Coudarchet:2023mfs</li></ol>
\subsection{Nongeometric compactifications} [4]<ol><li>Plauschinn:2018wbo</li><li>Wecht:2007wu</li><li>Kimura:2023knt</li></ol>
\subsection{String cosmology} [5]<ol><li>Cicoli:2023opf</li><li>Nastase:2019mhe</li><li>Leontaris:2023obe</li><li>Baumann:2014nda</li><li>Polchinski:2006gy</li><li>Bousso:2007gp</li><li>Silverstein:2016ggb</li><li>Baumann:2009ds</li><li>Brandenberger:2023ver</li><li>Berglund:2022qsb</li><li>Erdmenger:2009zz</li></ol>
\subsubsection{de-Sitter vacua} [6]<ol><li>Schachner:2025vol</li><li>Leontaris:2023obe</li><li>Berglund:2022qsb</li></ol> \subsubsection{String inflation} [7]<ol><li>Baumann:2014nda</li><li>Baumann:2009ds</li></ol> \subsubsection{Brane cosmology}
\subsection{Particle phenomenology} [8]<ol><li>Marchesano:2024gul</li><li>Cvetic:2022fnv</li><li>Marchesano:2022qbx</li></ol>
The previous section was on the phenomenology of cosmology. Unlike other quantum gravity theories, string theory, being a ToE, must also answer questions of particle phenomenology. \subsubsection{Axiverse} [9]<ol><li>Arvanitaki:2009fg</li><li>Reece:2023czb</li></ol> \etocsettocdepth.toc{subsection} \subsection{Swampland} [10]<ol><li>Brennan:2017rbf</li><li>Palti:2019pca</li><li>vanBeest:2021lhn</li><li>Agmon:2022thq</li><li>Grana:2021zvf</li></ol>
\subsubsection{No global symmetry conjecture}
\subsubsection{Completeness of spectrum}
\subsubsection{Weak gravity conjecture} [11]<ol><li>Harlow:2022ich</li><li>Rudelius_2024</li></ol>
\subsubsection{Distance conjectures}
\subsubsection{de Sitter conjectures}
\subsubsection{Finiteness and string lamppost}
\etocsettocdepth.toc{paragraph}
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