TT¯ Deformations and Form Factor Program

In this proceeding contribution, we review a recently proposed method to compute the minimal form factors (MFFs) of diagonal integrable field theories perturbed by irrelevant fields of the TT¯ family. Our construction generalizes standard form factor techniques to deal with the deformed two-body scattering amplitudes, which are typical in this setting. The results are minimal form factors which are the product of the undeformed solution and a new function. This function can be fixed by requiring constant asymptotics for large rapidities, smoothness in the limit when the perturbation parameters go to zero, and agreement with standard MFF formulae for particular choices of the perturbation couplings. We observe that, for a certain range of parameters, the new MFF develops a pole at θ = 0. By considering several UV-complete theories, we argue that such poles can emerge naturally from the MFF integral representation and suggest how they may be eliminated.

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Publication Details

Journal
White Rose Research Online (University of Leeds, The University of Sheffield, University of York)
Published
2025-12-05
Primary Topic
Black Holes and Theoretical Physics
Type
article
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article

TT¯ Deformations and Form Factor Program

Olalla A. Castro-Alvaredo, Stefano Negro, Fabio Sailis
White Rose Research Online (University of Leeds, The University of Sheffield, University of York)
Black Holes and Theoretical Physics
article

TT¯ Deformations and Form Factor Program

Olalla A. Castro-Alvaredo, Stefano Negro, Fabio Sailis
article en

Abstract

In this proceeding contribution, we review a recently proposed method to compute the minimal form factors (MFFs) of diagonal integrable field theories perturbed by irrelevant fields of the TT¯ family. Our construction generalizes standard form factor techniques to deal with the deformed two-body scattering amplitudes, which are typical in this setting. The results are minimal form factors which are the product of the undeformed solution and a new function. This function can be fixed by requiring constant asymptotics for large rapidities, smoothness in the limit when the perturbation parameters go to zero, and agreement with standard MFF formulae for particular choices of the perturbation couplings. We observe that, for a certain range of parameters, the new MFF develops a pole at θ = 0. By considering several UV-complete theories, we argue that such poles can emerge naturally from the MFF integral representation and suggest how they may be eliminated.

White Rose Research Online (University of Leeds, The University of Sheffield, University of York)
Openalex Percentile: Top 19%
Black Holes and Theoretical Physics
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