A nonlocal Schwinger model

Abstract We solve a system of massless fermions constrained to two space-time dimensions interacting via a d space-time dimensional Maxwell field. Through dimensional reduction to the defect and bosonization, the system maps to a massless scalar interacting with a nonlocal Maxwell field through a Fϕ...

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Main Authors: Ludo Fraser-Taliente, Christopher P. Herzog, Abhay Shrestha
Format: Article
Language:English
Published: SpringerOpen 2025-06-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP06(2025)252
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author Ludo Fraser-Taliente
Christopher P. Herzog
Abhay Shrestha
author_facet Ludo Fraser-Taliente
Christopher P. Herzog
Abhay Shrestha
author_sort Ludo Fraser-Taliente
collection DOAJ
description Abstract We solve a system of massless fermions constrained to two space-time dimensions interacting via a d space-time dimensional Maxwell field. Through dimensional reduction to the defect and bosonization, the system maps to a massless scalar interacting with a nonlocal Maxwell field through a Fϕ-coupling. The d = 2 dimensional case is the usual Schwinger model where the photon gets a mass. More generally, in 2 < d < 4 dimensions, the degrees of freedom map to a scalar which undergoes a renormalization group flow; in the ultraviolet, the scalar is free, while in the infrared it has scaling dimension (4 – d)/2. The infrared is similar to the Wilson-Fisher fixed point, and the physically relevant case d = 4 becomes infrared trivial in the limit of infinite ultraviolet cut-off, consistent with earlier work on the triviality of conformal surface defects in Maxwell theory.
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series Journal of High Energy Physics
spelling doaj-art-9c5c0ebd3c064052bca0a98e5f7152012025-08-20T03:45:39ZengSpringerOpenJournal of High Energy Physics1029-84792025-06-012025612810.1007/JHEP06(2025)252A nonlocal Schwinger modelLudo Fraser-Taliente0Christopher P. Herzog1Abhay Shrestha2Physics Department, Oxford UniversityDepartment of Mathematics, King’s College LondonDepartment of Mathematics, King’s College LondonAbstract We solve a system of massless fermions constrained to two space-time dimensions interacting via a d space-time dimensional Maxwell field. Through dimensional reduction to the defect and bosonization, the system maps to a massless scalar interacting with a nonlocal Maxwell field through a Fϕ-coupling. The d = 2 dimensional case is the usual Schwinger model where the photon gets a mass. More generally, in 2 < d < 4 dimensions, the degrees of freedom map to a scalar which undergoes a renormalization group flow; in the ultraviolet, the scalar is free, while in the infrared it has scaling dimension (4 – d)/2. The infrared is similar to the Wilson-Fisher fixed point, and the physically relevant case d = 4 becomes infrared trivial in the limit of infinite ultraviolet cut-off, consistent with earlier work on the triviality of conformal surface defects in Maxwell theory.https://doi.org/10.1007/JHEP06(2025)252Renormalization and RegularizationRenormalization GroupNonperturbative EffectsWilson’t Hooft and Polyakov loops
spellingShingle Ludo Fraser-Taliente
Christopher P. Herzog
Abhay Shrestha
A nonlocal Schwinger model
Journal of High Energy Physics
Renormalization and Regularization
Renormalization Group
Nonperturbative Effects
Wilson
’t Hooft and Polyakov loops
title A nonlocal Schwinger model
title_full A nonlocal Schwinger model
title_fullStr A nonlocal Schwinger model
title_full_unstemmed A nonlocal Schwinger model
title_short A nonlocal Schwinger model
title_sort nonlocal schwinger model
topic Renormalization and Regularization
Renormalization Group
Nonperturbative Effects
Wilson
’t Hooft and Polyakov loops
url https://doi.org/10.1007/JHEP06(2025)252
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