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Neiman,Higher-spin self-dual General Relativity: 6d and 4d pictures, covariant vs

4 Pith papers cite this work. Polarity classification is still indexing.

4 Pith papers citing it

fields

hep-th 4

years

2026 4

verdicts

UNVERDICTED 4

representative citing papers

Worldline Higher Spin Gravity

hep-th · 2026-05-27 · unverdicted · novelty 8.0

A worldline path integral model for higher-spin gravity in AdS4 is constructed using twistor actions and double-line vertices, reproducing boundary correlators of free boson and fermion vector models.

Self-dual gravity from higher-spin theory

hep-th · 2026-03-23 · unverdicted · novelty 6.0

Self-dual gravity with cosmological constant emerges uniquely as the rigid lower-spin sector of four-dimensional higher-spin interactions when only self-dual vertices are kept.

citing papers explorer

Showing 4 of 4 citing papers.

  • Worldline Higher Spin Gravity hep-th · 2026-05-27 · unverdicted · none · ref 105

    A worldline path integral model for higher-spin gravity in AdS4 is constructed using twistor actions and double-line vertices, reproducing boundary correlators of free boson and fermion vector models.

  • Self-dual holography: four-point AdS/CFT correlators in higher-spin gravity hep-th · 2026-05-28 · unverdicted · none · ref 77

    Develops holographic dictionary for self-dual higher-spin theories and computes four-point AdS/CFT correlators in a higher-spin extension of self-dual Yang-Mills.

  • Self-dual gravity from higher-spin theory hep-th · 2026-03-23 · unverdicted · none · ref 57

    Self-dual gravity with cosmological constant emerges uniquely as the rigid lower-spin sector of four-dimensional higher-spin interactions when only self-dual vertices are kept.

  • Dirichlet, Neumann, Mixed and self-dual holography: (self-dual) Yang--Mills theory II hep-th · 2026-06-24 · unverdicted · none · ref 44

    Derives bulk and boundary propagators and computes 3- and 4-point correlators for YM, CS and SDYM in AdS/CFT with multiple boundary conditions to relate their observables.