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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Main Authors: Marco Ardu, Luca Di Luzio, Giacomo Landini, Alessandro Strumia, Daniele Teresi, Jin-Wei Wang
Format: Article
Language:English
Published: SpringerOpen 2020-11-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP11(2020)090
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spelling 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
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