Axion quality from the (anti)symmetric of SU( N $$ \mathcal{N} $$ )
Abstract We propose two models where a U(1) Peccei-Quinn global symmetry arises accidentally and is respected up to high-dimensional operators, so that the axion solution to the strong CP problem is successful even in the presence of Planck-suppressed operators. One model is SU( N $$ \mathcal{N} $$...
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doaj-6a50246d5db945a9a7bc82ecd04eb52d2020-11-25T04:01:05ZengSpringerOpenJournal of High Energy Physics1029-84792020-11-0120201112410.1007/JHEP11(2020)090Axion quality from the (anti)symmetric of SU( N $$ \mathcal{N} $$ )Marco Ardu0Luca Di Luzio1Giacomo Landini2Alessandro Strumia3Daniele Teresi4Jin-Wei Wang5Dipartimento di Fisica “E. Fermi”, Università di PisaDESYDipartimento di Fisica “E. Fermi”, Università di PisaDipartimento di Fisica “E. Fermi”, Università di PisaDipartimento di Fisica “E. Fermi”, Università di PisaDipartimento di Fisica “E. Fermi”, Università di PisaAbstract We propose two models where a U(1) Peccei-Quinn global symmetry arises accidentally and is respected up to high-dimensional operators, so that the axion solution to the strong CP problem is successful even in the presence of Planck-suppressed operators. One model is SU( N $$ \mathcal{N} $$ ) gauge interactions with fermions in the fundamental and a scalar in the symmetric. The axion arises from spontaneous symmetry breaking to SO( N $$ \mathcal{N} $$ ), that confines at a lower energy scale. Axion quality in the model needs N $$ \mathcal{N} $$ ≳ 10. SO bound states and possibly monopoles provide extra Dark Matter candidates beyond the axion. In the second model the scalar is in the anti-symmetric: SU( N $$ \mathcal{N} $$ ) broken to Sp( N $$ \mathcal{N} $$ ) needs even N $$ \mathcal{N} $$ ≳ 20. The cosmological DM abundance, consisting of axions and/or super-heavy relics, can be reproduced if the PQ symmetry is broken before inflation (Boltzmann-suppressed production of super-heavy relics) or after (super-heavy relics in thermal equilibrium get partially diluted by dark glue-ball decays).http://link.springer.com/article/10.1007/JHEP11(2020)090Beyond Standard ModelCosmology of Theories beyond the SMGlobal Symmetries |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Marco Ardu Luca Di Luzio Giacomo Landini Alessandro Strumia Daniele Teresi Jin-Wei Wang |
spellingShingle |
Marco Ardu Luca Di Luzio Giacomo Landini Alessandro Strumia Daniele Teresi Jin-Wei Wang Axion quality from the (anti)symmetric of SU( N $$ \mathcal{N} $$ ) Journal of High Energy Physics Beyond Standard Model Cosmology of Theories beyond the SM Global Symmetries |
author_facet |
Marco Ardu Luca Di Luzio Giacomo Landini Alessandro Strumia Daniele Teresi Jin-Wei Wang |
author_sort |
Marco Ardu |
title |
Axion quality from the (anti)symmetric of SU( N $$ \mathcal{N} $$ ) |
title_short |
Axion quality from the (anti)symmetric of SU( N $$ \mathcal{N} $$ ) |
title_full |
Axion quality from the (anti)symmetric of SU( N $$ \mathcal{N} $$ ) |
title_fullStr |
Axion quality from the (anti)symmetric of SU( N $$ \mathcal{N} $$ ) |
title_full_unstemmed |
Axion quality from the (anti)symmetric of SU( N $$ \mathcal{N} $$ ) |
title_sort |
axion quality from the (anti)symmetric of su( n $$ \mathcal{n} $$ ) |
publisher |
SpringerOpen |
series |
Journal of High Energy Physics |
issn |
1029-8479 |
publishDate |
2020-11-01 |
description |
Abstract We propose two models where a U(1) Peccei-Quinn global symmetry arises accidentally and is respected up to high-dimensional operators, so that the axion solution to the strong CP problem is successful even in the presence of Planck-suppressed operators. One model is SU( N $$ \mathcal{N} $$ ) gauge interactions with fermions in the fundamental and a scalar in the symmetric. The axion arises from spontaneous symmetry breaking to SO( N $$ \mathcal{N} $$ ), that confines at a lower energy scale. Axion quality in the model needs N $$ \mathcal{N} $$ ≳ 10. SO bound states and possibly monopoles provide extra Dark Matter candidates beyond the axion. In the second model the scalar is in the anti-symmetric: SU( N $$ \mathcal{N} $$ ) broken to Sp( N $$ \mathcal{N} $$ ) needs even N $$ \mathcal{N} $$ ≳ 20. The cosmological DM abundance, consisting of axions and/or super-heavy relics, can be reproduced if the PQ symmetry is broken before inflation (Boltzmann-suppressed production of super-heavy relics) or after (super-heavy relics in thermal equilibrium get partially diluted by dark glue-ball decays). |
topic |
Beyond Standard Model Cosmology of Theories beyond the SM Global Symmetries |
url |
http://link.springer.com/article/10.1007/JHEP11(2020)090 |
work_keys_str_mv |
AT marcoardu axionqualityfromtheantisymmetricofsunmathcaln AT lucadiluzio axionqualityfromtheantisymmetricofsunmathcaln AT giacomolandini axionqualityfromtheantisymmetricofsunmathcaln AT alessandrostrumia axionqualityfromtheantisymmetricofsunmathcaln AT danieleteresi axionqualityfromtheantisymmetricofsunmathcaln AT jinweiwang axionqualityfromtheantisymmetricofsunmathcaln |
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