9-10 April 2024
US/Eastern timezone

Administrative Contact: Kimberly Potter

Prahar Mitra (Amsterdam) -- Celestial Conformal Primaries in Effective Field Theories

9 Apr 2024, 16:00
30m

Description

Scattering amplitudes in $d+2$ dimensions can be recast as correlators of conformal primary operators in a putative holographic CFT$_d$ by working in a basis of boost eigenstates instead of momentum eigenstates. In this talk, we show that completeness, normalizability, and consistency with CPT implies that we must restrict the boost eigenvalues of the operators to either $\Delta \in \frac{d}{2} + i {\mathbb R}$ or $\Delta \in {\mathbb R}$. Unlike those with $\Delta \in \frac{d}{2} + i {\mathbb R}$, operators with $\Delta \in {\mathbb R}$ can be constructed without knowledge of the UV and can therefore be defined in effective field theories. With additional analyticity assumptions, we can restrict $\Delta \in 2 - {\mathbb Z}_{\geq0}$ or $\Delta \in \frac{1}{2}-{\mathbb Z}_{\geq0}$ for bosonic or fermionic operators, respectively.

Presentation Materials

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