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Holographic beta functions for the generalized sine-Gordon theory

2018/09/30 by Prafulla Oak, B. Sathiapalan
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Geometry #Mathematical analysis #Mathematical physics #Mathematics #Particle physics theoretical and experimental studies #Physics #Quantum gravity #Quantum mechanics #Renormalization #Scalar (mathematics) #Scalar field #Scalar field theory #hep-th

paper · pdf · doi:10.1103/physrevd.99.046009

published as Phys. Rev. D 99, 046009 (2019) · 43 pages, 3 figures, PRD version

openalex publication_date 2019/02/15 · arxiv created 2019/03/10 · arxiv updated 2019/03/12 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

The sine-Gordon theory is generalized to include many scalar fields and several cosine terms. This is similar to the world sheet description of a string propagating in a tachyon background. This model is studied as a (boundary) 2D Euclidean field theory and also using an AdS3 holographic bulk dual. The beta functions for the cosine vertex of this modified theory are first computed in the boundary using techniques based on the exact RG. The beta functions are also computed holographically using position space and momentum space techniques. The results are in agreement with each other and with earlier computations. The cosine perturbation is of the form cosbX. Due to wave function renormalization the parameter b, and thus the dimension of the cosine, get renormalized. The beta function for this parameter is thus directly related to the anomalous dimension of the X field. We compute this beta function in position space. They match with the earlier results in [P. Oak and B. Sathiapalan, Exact renormalization group and sine-Gordon theory, J. High Energy Phys. 07 (2017) 103; P. Oak and B. SathiapalanJ. High Energy Phys. 09 (2017) 77.].

Citations