Axions in string theory

• Verfasst von: Cicoli, Michele [VerfasserIn]
• Verfasst von: Hebecker, Arthur [VerfasserIn]
• Verfasst von: Jaeckel, Joerg [VerfasserIn]
• Verfasst von: Wittner, Manuel [VerfasserIn]
• Titel: Axions in string theory
• Titelzusatz: slaying the Hydra of dark radiation
• Verf.angabe: Michele Cicoli, Arthur Hebecker, Joerg Jaeckel and Manuel Wittner
• E-Jahr: 2022
• Jahr: September 23, 2022
• Umfang: 65 S.
• Fussnoten: Gesehen am 22.11.2022
• Titel Quelle: Enthalten in: Journal of high energy physics
• Ort Quelle: Berlin : Springer, 1997
• Jahr Quelle: 2022
• Band/Heft Quelle: (2022), 9, Artikel-ID 198, Seite 1-65
• ISSN Quelle: 1029-8479
• DOI: doi:10.1007/JHEP09(2022)198
• Datenträger: Online-Ressource
• Sprache: eng
• Sach-SW: Axions and ALPs
• Sach-SW: Early Universe Particle Physics
• Sach-SW: Flux Compactifications
• Sach-SW: String and Brane Phenomenology
• K10plus-PPN: 1823135137

Abstract

It is widely believed that string theory easily allows for a QCD axion in the cosmologically favored mass range. The required small decay constant, fa ≪ MP, can be implemented by using a large compactification volume. This points to the Large Volume Scenario which in turn makes certain cosmological predictions: first, the closed string axion behaves similarly to a field-theoretic axion in the pre-inflationary scenario, i.e. the initial value can be tuned but one is constrained by isocurvature fluctuations. In addition, the volume represents a long-lived modulus that may lead to an early matter-dominated phase. Finally, the decay of the volume modulus to its own axion tends to overproduce dark radiation. In this paper we aim to carefully analyze the cosmology by studying models that not only allow for a QCD axion but also include inflation. Quite generally, limits on isocurvature fluctuations restrict us to relatively low-scale inflation, which in the present stringy context points to Kähler moduli inflation. As a novel feature we find that the lightest (volume) modulus couples strongly to the Higgs. It hence quickly decays to the SM, thus resolving the original dark radiation problem. This decay is much faster than that of the inflaton, implying that reheating is determined by the inflaton decay. The inflaton could potentially reintroduce a dark radiation problem since it decays to lighter moduli and their axions with equal rates. However, due its mixing with the QCD-saxion, the inflaton has also a direct decay rate to the SM, enhanced by the number of SM gauge bosons. This results in an amount of dark radiation that is consistent with present limits but potentially detectable in future measurements.