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MSSM vacua from Flux Compactifications
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We construct the first D = 4 Minkowski string theory vacua of flux compactification which are (i) chiral, (ii) free of NSNS and RR tadpoles, and (iii) N = 1 or N = 0 supersymmetric. In the latter case SUSY is softly broken by the fluxes, with soft terms being generated in the gauge and chiral sectors of the theory. In addition, the low energy spectrum of the theory is MSSM-like, the dilaton/complex structure moduli are stabilized and the supergravity background involves a warped metric.
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Cited by 2 Pith papers
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Three-Family Supersymmetric Pati-Salam Flux Models from Rigid D-Branes
New three-family Pati-Salam flux models from rigid D-branes in Type IIB on T^6/(Z2 x Z2) stabilize moduli via G3 flux and meet N=1 supersymmetry, RR tadpole, and K-theory constraints.
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Three-family supersymmetric Pati-Salam models from intersecting D6-branes on rigid cycles
Ten explicit three-family supersymmetric Pati-Salam models from rigid intersecting D6-branes on factorizable rectangular tori; four of the ten are asymptotically free.
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