9.3.1 Celestial holography

^[1]<ol><li>Hori:2003ic</li><li>Aspinwall:2009isa</li><li>Auroux</li><li>Alim:2012gq</li><li>Hori:2002fa</li><li>Hosono:1994av</li><li>Ballard:2008sy</li><li>Quigley:2014rya</li><li>Haghighat:2017bep</li><li>Imparato:2021tca</li><li>Imparato:2023jja</li><li>Webster:2023kjd</li><li>Kapustin:2003kt</li><li>Clader:2014kfa</li><li>Cox:2000vi</li></ol>

\subsubsection{Gauged Linear Sigma Model} Chapter 13 of ^[2]<ol><li>Hori:2003ic</li></ol>. ^[3]<ol><li>Sharpe:2024dcd</li><li>Krivorol:2025ynl</li><li>Sharpe:2013anr</li><li>Pantev:2005zs</li></ol> and ^[4]<ol><li>Tachikawa:2018sae</li><li>Agmon:2022thq</li></ol>

\subsubsection{Motivic integration} ^[5]<ol><li>Veys</li><li>Blickle</li><li>Mallory</li><li>gordon2008</li><li>Hales</li><li>Craw</li><li>MilesReid</li></ol>

\subsubsection{3D mirror symmetry} ^[6]<ol><li>Webster:2023kjd</li></ol>

---

← Previous: 9.3 Flat space holography bottom-up approaches

Next: 9.3.2 Carrollian holography →