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Non-tachyonic type 0B orientifolds, non-supersymmetric gauge theories and cosmological RG flow

1999/12/31 by Carlo Angelantonj, Adi Armoni · 49 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Cosmological constant #Cosmology and Gravitation Theories #Coupling constant #Dilaton #Gauge (firearms) #Gauge theory #Noncommutative and Quantum Gravity Theories #Spinor #String (physics) #String theory #Tadpole (physics) #Type (biology) #hep-th

paper · pdf · doi:10.1016/s0550-3213(00)00136-x

published in Nuclear Physics B 578(1-2), 239-258 (Elsevier BV) · 26 pages. Minor changes. Refs added. To appear in Nucl. Phys. B

arxiv created 2000/03/09 · openalex publication_date 2000/07/01 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

We discuss gauge theories on D3 branes embedded in special non-tachyonic orientifolds of the 0B string theory. In general, they correspond to non-supersymmetric SU(N) gauge theories with scalars in the adjoint representation and spinors in the (anti-)symmetric representation. We study these theories via the AdS/CFT correspondence and present evidence of their relation to N=4 SYM in the planar limit. We also discuss finite N properties, focusing in particular on the renormalization group flow. Up to two loops, the logarithmic running of the gauge coupling is described by the dilaton tadpole and the cosmological constant that naturally emerge on the string theory side.

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