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Renormalization group and decoupling in curved space, II. The standard model and beyond

2003/03/14 by É. V. Gorbar, Eduard V. Gorbar, Ilya L. Shapiro · 5 citations
Mathematics · Physics and Astronomy · #Black Holes and Theoretical Physics #Conformal map #Cosmology and Gravitation Theories #Curved space #Decoupling (probability) #Effective action #Fermion #Functional renormalization group #Massless particle #Mathematical analysis #Mathematical physics #Mathematics #Particle physics #Particle physics theoretical and experimental studies #Physics #Quantum chromodynamics #Quantum electrodynamics #Renormalization #Renormalization group #Scalar (mathematics) #Supersymmetry #Theoretical physics #gr-qc #hep-ph #hep-th

paper · pdf · doi:10.1088/1126-6708/2003/06/004

published as JHEP 0306:004,2003 · 27 pages, 8 figures

arxiv created 2003/03/14 · openalex publication_date 2003/06/04 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We continue the study of the renormalization group and decoupling of massive fields in curved space, started in the previous article and analyse the higher derivative sector of the vacuum metric-dependent action of the Standard Model. The QCD sector at low-energies is described in terms of the composite effective fields. For fermions and scalars the massless limit shows perfect correspondence with the conformal anomaly, but similar limit in a massive vector case requires an extra compensating scalar. In all three cases the decoupling goes smoothly and monotonic. A particularly interesting case is the renormalization group flow in the theory with broken supersymmetry, where the sign of one of the beta-functions changes on the way from the UV to IR.

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