Non-Tachyonic Type 0B Orientifolds, Non-Supersymmetric Gauge Theories and Cosmological RG Flow
Carlo Angelantonj (ENS), Adi Armoni (Ecole Polytechnique)

TL;DR
This paper explores non-tachyonic orientifolds of 0B string theory, analyzing non-supersymmetric gauge theories on D3 branes through AdS/CFT, and investigates their RG flow and string theory implications.
Contribution
It introduces non-tachyonic orientifolds of 0B string theory and studies associated non-supersymmetric gauge theories via AdS/CFT, linking RG flow to string theory parameters.
Findings
Evidence of relation to N=4 SYM in the planar limit
Logarithmic running of gauge coupling described by dilaton tadpole
Analysis of finite N properties and RG flow behavior
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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