Skip to content
DraconiticResearch
Search Sources API
197,693 studies31 sourcesUpdated 19 min ago
PreprintCC BY 4.0arXiv

Data analysis of millions of Type IIB flux vacua

Abstract

We study the vacuum structure of flux compactifications of type IIB string theory on the degree 18 hypersurface in ℂℙ41,1,1,6,9 with two effective complex structure moduli. We scan 30,770,178 flux choices compatible with the tadpole bound, and use a gradient-based constrained minimization based on the SLSQP algorithm to identify candidates for local minima of the scalar potential, yielding a dataset of millions of candidate flux vacua. Using the 1,296,633 reliable solutions selected from this dataset, we analyze distributions and correlations of various physical quantities such as vacuum expectation values of moduli and vacuum energy. Using quadratic flux invariants as input features, we train a classifier to identify solutions satisfying the numerical SUSY criterion |V|<10−4.5. On a randomly selected test set, selecting the top-ranked 5% recovers 47.2% of the SUSY test solutions. We also use supervised regression to predict the potential and moduli field values. In the regression comparison, quadratic flux invariant inputs improve prediction of potential value and the complex-structure coordinates, while the vanilla six flux parameters give better predictions for the axio-dilaton coordinates under the tested settings.

Related

  1. Scale-separated AdS2 flux vacua from type II
    George Tringas, Timm Wrase
    arXivPreprintarXiv licenceFull textHigh-energy & particle physicsarXiv
  2. Phases of flux vacua and their quantum symmetries
    Dan Israel, Ilarion V. Melnikov, Yann Proto
    arXivPreprintCC BY 4.0Full textHigh-energy & particle physicsarXivHAL
  3. Note on arithmetic structure of modulus vacua in flux compactifications
    Yukiya Furuta, Tatsuo Kobayashi, Tomoyasu Kori +3
    arXivPreprintCC BY 4.0Full textHigh-energy & particle physicsarXiv
  4. Note on arithmetic structure of modulus vacua in flux compactifications
    Yukiya Furuta, Tatsuo Kobayashi, Tomoyasu Kori +3
    Journal of High Energy PhysicsPeer-reviewedCC BY 4.0Full textHigh-energy & particle physicsCrossref
  5. Low-energy brane decoupling in AdS flux vacua
    Fien Apers, Noelia Sánchez González
    arXivPreprintarXiv licenceFull textHigh-energy & particle physicsarXiv
BibTeX
@misc{hamada2026data,
  title = {{Data analysis of millions of Type IIB flux vacua}},
  author = {Yuta Hamada and Yuma Uematsu and Masahito Yamazaki},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2610.30273},
  eprint = {2610.30273},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2610.30273},
  note = {CC BY 4.0},
}
RIS
TY  - UNPB
TI  - Data analysis of millions of Type IIB flux vacua
AU  - Yuta Hamada
AU  - Yuma Uematsu
AU  - Masahito Yamazaki
PY  - 2026
DA  - 2026/10/21
PB  - arXiv
DO  - 10.48550/arxiv.2610.30273
UR  - https://arxiv.org/abs/2610.30273
AB  - We study the vacuum structure of flux compactifications of type IIB string theory on the degree 18 hypersurface in ℂℙ^4_1,1,1,6,9 with two effective complex structure moduli. We scan 30,770,178 flux choices compatible with the tadpole bound, and use a gradient-based constrained minimization based on the SLSQP algorithm to identify candidates for local minima of the scalar potential, yielding a dataset of millions of candidate flux vacua. Using the 1,296,633 reliable solutions selected from this dataset, we analyze distributions and correlations of various physical quantities such as vacuum expectation values of moduli and vacuum energy. Using quadratic flux invariants as input features, we train a classifier to identify solutions satisfying the numerical SUSY criterion |V|<10^−4.5. On a randomly selected test set, selecting the top-ranked 5% recovers 47.2% of the SUSY test solutions. We also use supervised regression to predict the potential and moduli field values. In the regression comparison, quadratic flux invariant inputs improve prediction of potential value and the complex-structure coordinates, while the vanilla six flux parameters give better predictions for the axio-dilaton coordinates under the tested settings.
ER  -