Self-dual pp-wave solutions in chiral higher-spin gravity
Tung Tran
TL;DR
This work constructs a class of exact self-dual pp-wave solutions in chiral higher-spin gravity at zero cosmological constant ($\Lambda=0$) by employing a light-cone/Kerr– Schild-inspired ansatz. Central to the method is a harmonic-profile framework for the spin-2 sector, extended to all spins via a linearized and then non-linear free differential algebra (FDA) structure, with higher-order vertices shown to vanish on these backgrounds. The analysis demonstrates that the resulting configurations satisfy both linear and non-linear equations of motion, effectively yielding free-field dynamics on a self-dual background sourced by a positive-helicity spin-2 field, and it derives the corresponding effective action that reduces to kinetic terms on the SD pp-wave geometry. The results suggest a robust integrability structure for chiral HSGRA in flat space and point to potential extensions to nearby theories and to quantum-consistent constructions, including twistor-space approaches and Green–Schwarz-type mechanisms for anomaly cancellation.
Abstract
We show that chiral higher-spin gravity with a vanishing cosmological constant admits a class of exact self-dual pp-wave solutions derived from harmonic scalar functions and two principal spinors. These solutions satisfy both the linear and non-linear equations of motion, as they annihilate all higher-order vertices, leading to the equations of motion for free fields on a self-dual background sourced by a positive-helicity spin-2 field. Our method employs a simple light-cone ansatz for positive-helicity chiral higher-spin fields, along with a modified Kerr-Schild ansatz adapted for the self-dual gravity framework.
