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Systematics of type IIB moduli stabilisation with odd axions,

3 Pith papers cite this work. Polarity classification is still indexing.

3 Pith papers citing it

citation-role summary

background 1

citation-polarity summary

fields

hep-th 3

years

2026 2 2025 1

verdicts

UNVERDICTED 3

roles

background 1

polarities

background 1

representative citing papers

On Calabi-Yau Threefolds For Unified LVS Inflation

hep-th · 2026-06-09 · unverdicted · novelty 6.0

A database scan identifies 2+14+45 Calabi-Yau threefolds with specified fibration and divisor structures that unify three LVS Kähler moduli inflation models.

Testing F-theory GUTs with the Axiverse

hep-th · 2026-06-08 · unverdicted · novelty 6.0

In F-theory GUTs, non-universal ALPs induced by hypercharge flux satisfy g_aγ/m_a well below the QCD axion prediction when gauge couplings unify near the string scale.

Assisted Fibre Inflation in Perturbative LVS

hep-th · 2025-06-27 · unverdicted · novelty 4.0

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).

citing papers explorer

Showing 3 of 3 citing papers.

  • On Calabi-Yau Threefolds For Unified LVS Inflation hep-th · 2026-06-09 · unverdicted · none · ref 54

    A database scan identifies 2+14+45 Calabi-Yau threefolds with specified fibration and divisor structures that unify three LVS Kähler moduli inflation models.

  • Testing F-theory GUTs with the Axiverse hep-th · 2026-06-08 · unverdicted · none · ref 79

    In F-theory GUTs, non-universal ALPs induced by hypercharge flux satisfy g_aγ/m_a well below the QCD axion prediction when gauge couplings unify near the string scale.

  • Assisted Fibre Inflation in Perturbative LVS hep-th · 2025-06-27 · unverdicted · none · ref 81

    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).