TY - JOUR
T1 - Superstring perturbation theory and Ramond-Ramond backgrounds
AU - Berenstein, David
AU - Leigh, Robert G.
PY - 1999
Y1 - 1999
N2 - We consider perturbative type II superstring theory in the covariant NSR formalism in the presence of NSNS and RR backgrounds. A concrete example that we have in mind is the geometry of D3-branes which in the near-horizon region is (Formula presented) although our methods may be applied to other backgrounds as well. We show how conformal invariance of the string path integral is maintained order by order in the number of holes. This procedure makes uses of the Fischler-Susskind mechanism to build up the background geometry. A simple formal expression is given for a (Formula presented)-model Lagrangian. This suggests a perturbative expansion in (Formula presented) and (Formula presented) As applications, we consider at leading order the mixing of RR and NSNS states, and the realization of the spacetime supersymmetry algebra.
AB - We consider perturbative type II superstring theory in the covariant NSR formalism in the presence of NSNS and RR backgrounds. A concrete example that we have in mind is the geometry of D3-branes which in the near-horizon region is (Formula presented) although our methods may be applied to other backgrounds as well. We show how conformal invariance of the string path integral is maintained order by order in the number of holes. This procedure makes uses of the Fischler-Susskind mechanism to build up the background geometry. A simple formal expression is given for a (Formula presented)-model Lagrangian. This suggests a perturbative expansion in (Formula presented) and (Formula presented) As applications, we consider at leading order the mixing of RR and NSNS states, and the realization of the spacetime supersymmetry algebra.
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U2 - 10.1103/PhysRevD.60.106002
DO - 10.1103/PhysRevD.60.106002
M3 - Article
AN - SCOPUS:18144363255
SN - 1550-7998
VL - 60
JO - Physical Review D - Particles, Fields, Gravitation and Cosmology
JF - Physical Review D - Particles, Fields, Gravitation and Cosmology
IS - 10
ER -