Higher-order chiral scalar from boundary reduction of 3d higher-spin gravity
Calvin Chen (Theoretical Physics, Blackett Laboratory, Imperial College, London, SW7 2AZ, UK, Center for Theoretical Physics, National Taiwan University, Taipei, 10617, Taiwan, Leung Center for Cosmology and Particle Astrophysics, Taipei, 10617, Taiwan)
; Euihun Joung (Department of Physics, College of Science, Kyung Hee University, Seoul, 02447, South Korea)
; Karapet Mkrtchyan (Theoretical Physics, Blackett Laboratory, Imperial College, London, SW7 2AZ, UK)
; Junggi Yoon (School of Physics, Korea Institute for Advanced Study, 85 Hoegiro Dongdaemun-gu, Seoul, 02455, South Korea, Department of Physics, College of Science, Kyung Hee University, Seoul, 02447, South Korea, Asia Pacific Center for Theoretical Physics, POSTECH, 77 Cheongam-ro, Nam-gu, Pohang-si, Gyeongsangbuk-do, 37673, South Korea)
We use a recently proposed covariant procedure to reduce the Chern-Simons action of three-dimensional higher-spin gravity to the boundary, resulting in a Lorentz covariant action for higher-order chiral scalars. After gauge-fixing, we obtain a higher-derivative action generalizing the $\textit{s}$ = 1 Floreanini-Jackiw and $\textit{s}$ = 2 Alekseev-Shatashvili actions to arbitrary spin s. For simplicity, we treat the case of general spin at the linearized level, while the full non-linear asymptotic boundary conditions are presented in component form for the SL(3, ℝ) case. Finally, we extend the spin-3 linearized analysis to a background with non-trivial higher-spin charge and show that it has a richer structure of zero modes.