pith. sign in

arxiv: 1612.02479 · v2 · pith:THWBKF6Tnew · submitted 2016-12-07 · ✦ hep-th · math-ph· math.MP· math.SP

Harmony of Spinning Conformal Blocks

classification ✦ hep-th math-phmath.MPmath.SP
keywords blocksconformalspinningapproachanalysisbootstrapbundlescalogero-sutherland
0
0 comments X
read the original abstract

Conformal blocks for correlation functions of tensor operators play an increasingly important role for the conformal bootstrap programme. We develop a universal approach to such spinning blocks through the harmonic analysis of certain bundles over a coset of the conformal group. The resulting Casimir equations are given by a matrix version of the Calogero-Sutherland Hamiltonian that describes the scattering of interacting spinning particles in a 1-dimensional external potential. The approach is illustrated in several examples including fermionic seed blocks in 3D CFT where they take a very simple form.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Crosscap Defects

    hep-th 2026-04 unverdicted novelty 7.0

    Crosscap defects from Z2 spacetime quotients in CFTs yield new crossing equations and O(N) model examples without displacement or tilt operators, forming defect conformal manifolds lacking exactly marginal operators.

  2. Crosscap Defects

    hep-th 2026-04 unverdicted novelty 7.0

    Crosscap defects are introduced in CFTs via Z2 quotients, with crossing equations derived and CFT data computed in the O(N) model at Gaussian and Wilson-Fisher points showing absent displacement and tilt operators for...

  3. Superconformal Weight Shifting Operators

    hep-th 2025-06 unverdicted novelty 7.0

    Introduces SU(m,m|2n)-covariant weight-shifting operators in the super-Grassmannian formalism to derive all superconformal blocks from half-BPS ones.