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RR Flux on Calabi-Yau and Partial Supersymmetry Breaking

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arxiv hep-th/9912152 v2 pith:UJDVWSJB submitted 1999-12-16 hep-th

T.R. Taylor , C. Vafa This is my paper · ORCID
classification hep-th
keywords calabi-yaufluxfreezingmasssupersymmetrybreakbreakingdeformation
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We show how turning on Flux for RR (and NS-NS) field strengths on non-compact Calabi-Yau 3-folds can serve as a way to partially break supersymmetry from N=2 to N=1 by mass deformation. The freezing of the moduli of Calabi-Yau in the presence of the flux is the familiar phenomenon of freezing of fields in supersymmetric theories upon mass deformations.

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Cited by 4 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. F-theory flux vacua at large complex structure

    hep-th 2021-05 unverdicted novelty 7.0 of 10

    At large complex structure in F-theory, the F-term potential simplifies to V = Z^{AB} ρ_A ρ_B, yielding two families of flux vacua with all complex structure moduli fixed, one with bounded saxion vevs and one with unb...

  2. Tetra-quadric CY Threefold and Assisted Fibre Inflation

    hep-th 2026-08 conditional novelty 6.0 of 10

    Three Kähler moduli on a tetra-quadric CY orientifold collectively drive assisted fibre inflation with individual shifts near 2.2 M_p instead of the effective 5.7 M_p.

  3. A Landscape of AdS Flux Vacua

    hep-th 2019-08 conditional novelty 6.0 of 10

    A bilinear flux-axion polynomial technique yields new branches of type IIA Calabi-Yau flux vacua, including a tachyon-free non-supersymmetric AdS branch.

  4. Assisted Fibre Inflation in Perturbative LVS

    hep-th 2025-06 unverdicted novelty 4.0 of 10

    Multi-field fibre inflation in perturbative LVS uses collective dynamics of several moduli to achieve viable cosmology with sub-Planckian individual field ranges given by total range divided by sqrt(n).

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