Abstract
We examine the leading Regge string states relevant for semi-classical spinning string solutions. Using elementary RNS techniques, quadratic terms in an effective Lagrangian are constructed which describe massive NSNS strings in a space–time with five-form flux. We then examine the specific case of AdS 5 × S 5 , finding the dependence of AdS “energy” ( E 0 ) on spin in AdS ( S), spin on the sphere ( J), and orbital angular momentum on the sphere ( ∇ a ∇ a ).
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