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Feebly-interacting Peccei-Quinn model
by
Yin, Wen
in
Astronomical models
/ Axions and ALPs
/ Classical and Quantum Gravitation
/ Cosmology
/ Cosmology of Theories BSM
/ Dark matter
/ Decay rate
/ Elementary Particles
/ Gauge theory
/ Gravitational waves
/ Higgs bosons
/ Hypothetical particles
/ New Light Particles
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Quantum Physics
/ Quarks
/ Regular Article - Theoretical Physics
/ Relativity Theory
/ Scalars
/ Standard model (particle physics)
/ String Theory
/ Wave functions
2025
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Feebly-interacting Peccei-Quinn model
by
Yin, Wen
in
Astronomical models
/ Axions and ALPs
/ Classical and Quantum Gravitation
/ Cosmology
/ Cosmology of Theories BSM
/ Dark matter
/ Decay rate
/ Elementary Particles
/ Gauge theory
/ Gravitational waves
/ Higgs bosons
/ Hypothetical particles
/ New Light Particles
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Quantum Physics
/ Quarks
/ Regular Article - Theoretical Physics
/ Relativity Theory
/ Scalars
/ Standard model (particle physics)
/ String Theory
/ Wave functions
2025
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Feebly-interacting Peccei-Quinn model
by
Yin, Wen
in
Astronomical models
/ Axions and ALPs
/ Classical and Quantum Gravitation
/ Cosmology
/ Cosmology of Theories BSM
/ Dark matter
/ Decay rate
/ Elementary Particles
/ Gauge theory
/ Gravitational waves
/ Higgs bosons
/ Hypothetical particles
/ New Light Particles
/ Physics
/ Physics and Astronomy
/ Quantum Field Theories
/ Quantum Field Theory
/ Quantum Physics
/ Quarks
/ Regular Article - Theoretical Physics
/ Relativity Theory
/ Scalars
/ Standard model (particle physics)
/ String Theory
/ Wave functions
2025
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Journal Article
Feebly-interacting Peccei-Quinn model
2025
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Overview
A
bstract
The QCD axion is widely studied as a dark matter (DM) candidate and as a solution to the strong CP problem of the Standard Model. In conventional field-theoretic models, a much larger mass scale than the electroweak (EW) scale is typically introduced to spontaneously break Peccei-Quinn (PQ) symmetry with a large enough axion decay constant,
f
a
, thereby avoiding constraints from star cooling. In this paper, I propose an alternative approach to achieving the large decay constant: a PQ scalar field with a large wave function renormalization constant, analogous to a feebly coupled gauge theory. Other dimensionless parameters are
O
1
in the unit of the EW scale for the naturalness. This framework predicts a light PQ Higgs boson with a mass ~ (EW scale)
2
/
f
a
. Exotic particles associated with the PQ anomaly are expected to have masses around the EW scale. The proposed model alleviates both the PQ quality and EW scale fine-tuning problems and introduces interesting axion-PQ Higgs cosmologies, encompassing: slim axion DM from a fat string network, heavy axion DM from PQ Higgs condensate fragmentation, PQ Higgs DM, and axion-PQ Higgs co-DM scenarios. Potential experimental signatures are explored, including fifth-force tests, DM detections, accelerator searches, and gravitational wave observations by employing lattice simulation. Possible extensions of the scenario are also discussed.
Publisher
Springer Berlin Heidelberg,Springer Nature B.V,SpringerOpen
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