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Chiral Higher Spin Gravity From Strong Homotopy Algebra

Richard van Dongen

TL;DR

This thesis develops a Covariant, unfolding-based formulation of Chiral Higher Spin Gravity (HiSGRA) by encoding its dynamics in an underlying $L_infty$-algebra, built from an $A_infty$-algebra of pre-Calabi–Yau type. The self-dual subtheories SDYM and SDGR are analyzed as minimal models, and their FDA/jet-space data are extended to higher spins using Homological Perturbation Theory to generate all higher-order vertices. A Stokes-theorem framework is established to prove the $A_infty$-relations and connect the construction to deformation quantization and Kontsevich formality, with integration spaces linked to convex polygons and swallowtails (positive Grassmannians). The results show that a covariant formulation of chiral HiSGRA is compatible with AdS/CFT expectations, implying a closed chiral subsector of $O(N)$ vector models, and suggest a generalized formality theorem beyond Kontsevich in a non-commutative setting. Altogether, the work provides a complete algebraic and geometric program for all-order interactions in Chiral HiSGRA and lays groundwork for covariant analysis of higher-spin holography and non-commutative deformation quantization.

Abstract

In this thesis, we derive the equations of motion of Chiral Higher Spin Gravity (HiSGRA) in terms of its underlying $L_\infty$-algebra. Chiral HiSGRA contains self-dual Yang-Mills and self-dual gravity as closed subsectors, which themselves form closed subsectors of Yang-Mills and general relativity. We begin by constructing a covariant formulation for self-dual Yang-Mills and self-dual gravity, and subsequently extend this construction to the full Chiral Higher Spin Gravity. Remarkably, the $L_\infty$-algebra is constructed from an $A_\infty$-algebra of pre-Calabi-Yau type, suggesting a deep connection to non-commutative deformation quantization. The structure maps of the resulting $L_\infty$-algebra are expressed as integrals of a simple exponential over convex polygons in $\mathbb{R}^2$. The existence of this covariant and coordinate independent formulation of chiral HiSGRA demonstrates, via the AdS/CFT correspondence, that $O(N)$ vector models possess a closed chiral subsector. Finally, we prove that the $A_\infty$-algebra follows from Stokes' theorem -- a crucial feature of the known formality theorems. To this end, we construct integration spaces that generalize convex polygons to $\mathbb{R}^3$, and are intimately connected to positive Grassmanians. This Stokes-based derivation points towards a novel generalization of Kontsevich' formality theorem to the non-commutative setting.

Chiral Higher Spin Gravity From Strong Homotopy Algebra

TL;DR

This thesis develops a Covariant, unfolding-based formulation of Chiral Higher Spin Gravity (HiSGRA) by encoding its dynamics in an underlying -algebra, built from an -algebra of pre-Calabi–Yau type. The self-dual subtheories SDYM and SDGR are analyzed as minimal models, and their FDA/jet-space data are extended to higher spins using Homological Perturbation Theory to generate all higher-order vertices. A Stokes-theorem framework is established to prove the -relations and connect the construction to deformation quantization and Kontsevich formality, with integration spaces linked to convex polygons and swallowtails (positive Grassmannians). The results show that a covariant formulation of chiral HiSGRA is compatible with AdS/CFT expectations, implying a closed chiral subsector of vector models, and suggest a generalized formality theorem beyond Kontsevich in a non-commutative setting. Altogether, the work provides a complete algebraic and geometric program for all-order interactions in Chiral HiSGRA and lays groundwork for covariant analysis of higher-spin holography and non-commutative deformation quantization.

Abstract

In this thesis, we derive the equations of motion of Chiral Higher Spin Gravity (HiSGRA) in terms of its underlying -algebra. Chiral HiSGRA contains self-dual Yang-Mills and self-dual gravity as closed subsectors, which themselves form closed subsectors of Yang-Mills and general relativity. We begin by constructing a covariant formulation for self-dual Yang-Mills and self-dual gravity, and subsequently extend this construction to the full Chiral Higher Spin Gravity. Remarkably, the -algebra is constructed from an -algebra of pre-Calabi-Yau type, suggesting a deep connection to non-commutative deformation quantization. The structure maps of the resulting -algebra are expressed as integrals of a simple exponential over convex polygons in . The existence of this covariant and coordinate independent formulation of chiral HiSGRA demonstrates, via the AdS/CFT correspondence, that vector models possess a closed chiral subsector. Finally, we prove that the -algebra follows from Stokes' theorem -- a crucial feature of the known formality theorems. To this end, we construct integration spaces that generalize convex polygons to , and are intimately connected to positive Grassmanians. This Stokes-based derivation points towards a novel generalization of Kontsevich' formality theorem to the non-commutative setting.
Paper Structure (179 sections, 2 theorems, 737 equations, 58 figures)

This paper contains 179 sections, 2 theorems, 737 equations, 58 figures.

Key Result

Lemma 4.A.2

For any SDR data (SDR) and a small perturbation $\delta$ of $d_V$ such that $(d_V+\delta)^2=0$ and $1-\delta h$ is invertible, there is a new SDR where the maps are given by

Figures (58)

  • Figure 1: The standard model and general relativity are described by fields up to spin $2$. In addition to this lower-spin sector, HiSGRA also incorporates higher spins. Figure adopted from Bekaert:2022poo
  • Figure 2: (Anti-)Chiral HiSGRA is a closed subsector of a full, parity-invariant HiSGRA. It should be dual to a closed subsector of Chern-Simons vector models.
  • Figure 3: Field content of HiSGRA. Along the axes we have the number of unprimed/primed indices on a spin-tensor. The black square shows a cocycle that links the one-form sector to zero-forms (at the free level it relates two fields for each spin's subsystem). The two fields in the rounded rectangle enter the free action. The rest of the fields encode derivatives thereof in a coordinate invariant and background independent way. The solid lines link pairwise the fields that 'talk' to each other in the free equations.
  • Figure 4: A generic tree $T$ in the left panel with elements of $\mathbb{A}_0$ attached left and right arbitrarily and the 'base' tree $T_0$ in the right panel with only elements of $\mathbb{A}_0$ attached to the right on the right branch. $T$ can be obtained form $T_0$ through flipping $\alpha_i$'s to the left of the right branch and/or shifting them to the left branch.
  • Figure 5: In the left panel a swallowtail constructed from the vectors $(\vec{q}_1,\vec{q}_2,\vec{q}_3,\vec{q}_4,\vec{q}_a,\vec{q}_b)$ and in the right panel a self-intersecting polygon constructed from $(\vec{q}_1,\vec{q}_2,\vec{q}_a,\vec{q}_3,\vec{q}_4,\vec{q}_b)$. They are associated to the quintic structure maps, respectively.
  • ...and 53 more figures

Theorems & Definitions (22)

  • Definition 1.3.1
  • Definition 1.3.2
  • Definition 1.3.3
  • Definition 1.3.4
  • Definition 1.3.5
  • Definition 1.3.6
  • Definition 1.3.7
  • Definition 1.3.8: algebraic definition
  • Definition 1.3.9
  • Definition 1.3.10: algebraic definition
  • ...and 12 more