Foamy dark matter from monodromies

We investigate the dynamics of axion-like particle (ALP) dark matter where the field range is enlarged by a monodromy. The monodromy potential allows sufficient production of dark matter also at larger couplings to the Standard Model particles. The potential typically features a number of “wiggles”...

Ausführliche Beschreibung

Gespeichert in:
Bibliographische Detailangaben
Hauptverfasser: Berges, Jürgen (VerfasserIn) , Chatrchyan, Aleksandr (VerfasserIn) , Jaeckel, Joerg (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: 19 August 2019
In: Journal of cosmology and astroparticle physics
Year: 2019, Heft: 8, Pages: 1-25
ISSN:1475-7516
DOI:10.1088/1475-7516/2019/08/020
Online-Zugang:Verlag, Volltext: https://doi.org/10.1088/1475-7516/2019/08/020
Verlag: https://doi.org/10.1088%2F1475-7516%2F2019%2F08%2F020
Volltext
Verfasserangaben:Jürgen Berges, Aleksandr Chatrchyan, Joerg Jaeckel
Beschreibung
Zusammenfassung:We investigate the dynamics of axion-like particle (ALP) dark matter where the field range is enlarged by a monodromy. The monodromy potential allows sufficient production of dark matter also at larger couplings to the Standard Model particles. The potential typically features a number of “wiggles” that lead to a rapid growth of fluctuations. Using classical-statistical field theory simulations we go beyond the linear regime and treat the system in the non-linear and even non-perturbative regime. For sufficiently strong wiggles the initially homogeneous field is completely converted into fluctuations. The fluctuations correspond to dark matter particles with a non-vanishing velocity and we consider the corresponding restrictions from structure formation as well as the effects on today's dark matter density.
Beschreibung:Gesehen am 08.11.2019
Beschreibung:Online Resource
ISSN:1475-7516
DOI:10.1088/1475-7516/2019/08/020