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Symplectic modular symmetry in heterotic string vacua: flavor, CP, and $R$-symmetries

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arxiv 2107.00487 v2 pith:HHN2N6G5 submitted 2021-07-01 hep-th hep-ph

classification hep-thhep-ph
keywords symmetriesflavormathbbsymmetrycalabi-yaumodularthreefoldsheterotic
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

We examine a common origin of four-dimensional flavor, CP, and $U(1)_R$ symmetries in the context of heterotic string theory with standard embedding. We find that flavor and $U(1)_R$ symmetries are unified into the $Sp(2h+2, \mathbb{C})$ modular symmetries of Calabi-Yau threefolds with $h$ being the number of moduli fields. Together with the $\mathbb{Z}_2^{\rm CP}$ CP symmetry, they are enhanced to $GSp(2h+2, \mathbb{C})\simeq Sp(2h+2, \mathbb{C})\rtimes \mathbb{Z}_2^{\rm CP}$ generalized symplectic modular symmetry. We exemplify the $S_3, S_4, T^\prime, S_9$ non-Abelian flavor symmetries on explicit toroidal orbifolds with and without resolutions and $\mathbb{Z}_2,S_4$ flavor symmetries on three-parameter examples of Calabi-Yau threefolds. Thus, non-trivial flavor symmetries appear in not only the exact orbifold limit but also a certain class of Calabi-Yau threefolds. These flavor symmetries are further enlarged to non-Abelian discrete groups by the CP symmetry.

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Cited by 2 Pith papers

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

  1. Stringy Constraints on Modular Flavor Models

    hep-ph 2025-08 conditional novelty 6.0 of 10

    Heterotic one-loop threshold corrections imply upper bounds on the modulus in modular flavor models, ruling out tau near i infinity for typical dilaton and beta-function values and disfavoring tau = i at large volume.

  2. Inflationary constraints on the moduli-dependent species scale in modular invariant theories

    hep-th 2024-11 conditional novelty 5.0 of 10

    For SL(2,Z) modular inflation models, the CMB spectral index and tensor-to-scalar ratio imply a gravitational species scale of about 10^16 GeV.

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