The Peccei-Quinn (PQ) mechanism provides an elegant solution to the strong charge parity (𝐶⁢𝑃) problem. However astrophysical constraints on axions require the PQ breaking scale to be far higher than the electroweak scale. In supersymmetric models the PQ symmetry can be broken at an acceptable scale if the effective potential for the pseudomodulus in the axion multiplet develops a minimum at large enough field values. In this work we classify systematically hadronic axion models in the context of gauge mediation and study their effective potentials at one loop. We find that some models generate a PQ scale comparable to the messenger scale. Our result may prove useful for constructing full realistic models of gauge mediation that address the strong 𝐶⁢𝑃 problem. We also comment briefly on the cosmological aspects related to the saxion and axino, and on the quality of the PQ symmetry.

Dynamical Generation of the Peccei-Quinn Scale in Gauge Mediation / Festuccia, Guido; Opferkuch, Toby; Ubaldi, Lorenzo. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - 92:(2015), pp. 1-13. [10.1103/PhysRevD.92.015020]

Dynamical Generation of the Peccei-Quinn Scale in Gauge Mediation

Guido Festuccia;Toby Opferkuch;Lorenzo Ubaldi
2015-01-01

Abstract

The Peccei-Quinn (PQ) mechanism provides an elegant solution to the strong charge parity (𝐶⁢𝑃) problem. However astrophysical constraints on axions require the PQ breaking scale to be far higher than the electroweak scale. In supersymmetric models the PQ symmetry can be broken at an acceptable scale if the effective potential for the pseudomodulus in the axion multiplet develops a minimum at large enough field values. In this work we classify systematically hadronic axion models in the context of gauge mediation and study their effective potentials at one loop. We find that some models generate a PQ scale comparable to the messenger scale. Our result may prove useful for constructing full realistic models of gauge mediation that address the strong 𝐶⁢𝑃 problem. We also comment briefly on the cosmological aspects related to the saxion and axino, and on the quality of the PQ symmetry.
2015
92
1
13
015020
https://doi.org/10.1103/PhysRevD.92.015020
https://arxiv.org/abs/1504.07634
Festuccia, Guido; Opferkuch, Toby; Ubaldi, Lorenzo
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11767/143193
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