Abstract

We use the formulation of conformal higher spin (CHS) theories in twistor space to study their tree-level scattering amplitudes, finding expressions for all three-point overline{mathrm{MHV}} amplitudes and all MHV amplitudes involving positive helicity conformal gravity particles and two negative helicity higher spins. This provides the on-shell analogue for the covariant coupling of CHS fields to a conformal gravity background. We discuss the restriction of the theory to a ghost-free unitary subsector, analogous to restricting conformal gravity to general relativity with a cosmological constant. We study the flat-space limit and show that the restricted amplitudes vanish, supporting the conjecture that in the unitary sector the S-matrix of CHS theories is trivial. However, by appropriately rescaling the amplitudes we find non-vanishing results which we compare with chiral flat-space higher spin theories.

Highlights

  • We use the formulation of conformal higher spin (CHS) theories in twistor space to study their tree-level scattering amplitudes, finding expressions for all three-point MHV amplitudes and all MHV amplitudes involving positive helicity conformal gravity particles and two negative helicity higher spins

  • We describe a unitary subsector of CHS theory, and discuss the various ways that external states of arbitrary spin are represented in twistor space

  • For the CHS theory we might hope to find analogous behaviour, which is to say that upon truncation to the unitary sector we find a massless higher spin theory on an AdS background where the dimensionful couplings are related to the dimensionless CHS

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Summary

Conformal higher spins on twistor space

Conformal higher spin (CHS) theories were first formulated at the linearized level in terms of rank s symmetric fields φμ1···μs with free action [3]. The action (2.1) is invariant under both the local (differential) and algebraic (Weyl) gauge symmetries δφμ1···μs (x) = ∂(μ1 ǫμ2···μs)(x) − δ(μ1μ2 αμ3···μs)(x) for totally symmetric ǫμ(s−1)(x) and αμ(s−2)(x). These free theories were extended to cubic interactions some time ago [4, 16], and can be completed to an interacting CHS theory involving single copies of conformal fields at all spins for integer s ≥ 0 [5, 7, 8]. We review the formulation of CHS theory in twistor space [14], making use of a perturbative expansion around a self-dual (SD) sector. We describe a unitary subsector of CHS theory, and discuss the various ways that external states of arbitrary spin are represented in twistor space

Perturbative expansion around a self-dual sector
Twistor actions for CHS theory
A unitary subsector
CHS scattering amplitudes from the twistor action
All MHV amplitudes
MHV amplitudes on a conformal gravity background
Restricting to the unitary subsector
Discussion
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