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

3 Pith papers citing it

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years

2026 3

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UNVERDICTED 3

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background 2

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background 2

representative citing papers

Automorphic Structures of Heterotic Vacua

hep-th · 2026-05-06 · unverdicted · novelty 7.0

Fixed points of Sp(4,Z) are extrema of the moduli potential in these heterotic models, with genus-2 no-go theorems for de Sitter vacua and possible metastable minima after SUSY breaking via nonperturbative Kähler terms.

Quark hierarchies and CP violation from the Siegel modular group

hep-ph · 2026-04-23 · unverdicted · novelty 7.0

A benchmark model using genus-2 modular invariance generates quark mass hierarchies and CP violation via moduli VEVs near invariant points, with mass ratios vanishing in the symmetric limit and mixing angles reproduced.

Finite modular Coleman-Weinberg inflation

hep-ph · 2026-07-01 · unverdicted · novelty 6.0

A finite modular symmetric model generates inflation via a Coleman-Weinberg potential from vector-like quarks, with Im(τ) as inflaton and Re(τ) as heavy axion, matching cosmological observations and predicting possible isocurvature perturbations.

citing papers explorer

Showing 3 of 3 citing papers.

  • Automorphic Structures of Heterotic Vacua hep-th · 2026-05-06 · unverdicted · none · ref 62

    Fixed points of Sp(4,Z) are extrema of the moduli potential in these heterotic models, with genus-2 no-go theorems for de Sitter vacua and possible metastable minima after SUSY breaking via nonperturbative Kähler terms.

  • Quark hierarchies and CP violation from the Siegel modular group hep-ph · 2026-04-23 · unverdicted · none · ref 89

    A benchmark model using genus-2 modular invariance generates quark mass hierarchies and CP violation via moduli VEVs near invariant points, with mass ratios vanishing in the symmetric limit and mixing angles reproduced.

  • Finite modular Coleman-Weinberg inflation hep-ph · 2026-07-01 · unverdicted · none · ref 26

    A finite modular symmetric model generates inflation via a Coleman-Weinberg potential from vector-like quarks, with Im(τ) as inflaton and Re(τ) as heavy axion, matching cosmological observations and predicting possible isocurvature perturbations.