Chern-Simons-Ghost Theories and de Sitter Space
Dionysios Anninos, Raghu Mahajan, Djordje Radicevic, Edgar Shaghoulian
TL;DR
The paper investigates CS theories coupled to ghost-like fundamental matter in the large-$N$ limit, identifying an exact $N\to -N$ mapping to ordinary CS-matter on $\mathbb{R}^3$ that enforces a bosonization duality in this setting and supports a dS/CFT interpretation with a higher-spin bulk. It then shows that at high temperature on $S^1\times S^2$, the mapping and bosonization fail due to competing large-$N$ saddles and holonomy dynamics, yielding a rich phase structure with topological transitions and partial dualities. The analysis employs perturbative two-loop RG calculations in Landau gauge, nonperturbative light-cone gauge methods, and a detailed saddle-point treatment of thermal holonomies to connect boundary CS-ghost theories to bulk de Sitter gravity wavefunction data. Overall, the work clarifies when ghost CS theories reproduce dual bosonic/fermionic descriptions and highlights the distinct finite-temperature behavior that challenges straightforward holographic intuitions in the dS context. These results advance our understanding of non-unitary holography and the role of high-spin de Sitter duals in quantum gravity.
Abstract
We explore Chern-Simons theories coupled to fundamental ghost-like matter in the large $N$ limit at 't Hooft coupling $λ$. These theories have been conjectured to be holographically dual to parity-violating, asymptotically dS$_4$ universes with a tower of light higher-spin fields. On $\mathbb{R}^3$, to all orders in large-$N$ perturbation theory, we show that Chern-Simons-ghost theories are related to ordinary Chern-Simons-matter theories by mapping $N \rightarrow - N$ and keeping $λ$ fixed. Consequently, the bosonization duality of ordinary Chern-Simons-matter theories extends to a bosonization duality of Chern-Simons-ghost theories on $\mathbb R^3$. On $S^1 \times S^2$, in the small-$S^1$ limit, neither $N \rightarrow -N$ nor bosonization hold, as we show by extensively studying large-$N$ saddles of the theories with both ghost and ordinary matter. The partition functions we compute along the way can be viewed as pieces of the late-time Hartle-Hawking wavefunction for the bulk dS$_4$ gravity theories.
