Home > Publications database > Fuzzy Dark Matter Candidates from String Theory |
Preprint | PUBDB-2021-03948 |
; ; ;
2021
This record in other databases:
Please use a persistent id in citations: doi:10.3204/PUBDB-2021-03948
Report No.: DESY-21-153; arXiv:2110.02964
Abstract: String theory has been claimed to give rise to natural fuzzy dark matter candidates in the form of ultralight axions. In this paper we revisit this claim by a detailed study of how moduli stabilisation affects the masses and decay constants of different axion fields which arise in type IIB flux compactifications. We find that obtaining a considerable contribution to the observed dark matter abundance without tuning the axion initial misalignment angle is not a generic feature of 4D string models since it requires a mild violation of the $S f\lesssim M_P$ bound, where $S$ is the instanton action and $f$ the axion decay constant. Our analysis singles out $C_4$-axions, $C_2$-axions and thraxions as the best candidates to realise fuzzy dark matter in string theory. For all these ultralight axions we provide predictions which can be confronted with present and forthcoming observations.
Keyword(s): dark matter, fuzzy ; moduli, stability ; axion, decay constant ; compactification, flux ; instanton, action ; string model ; string ; alignment ; Fuzzy dark matter ; ultralight axions ; 4D string models
![]() |
The record appears in these collections: |
Journal Article
Fuzzy Dark Matter candidates from string theory
Journal of high energy physics 05(5), 107 (2022) [10.1007/JHEP05(2022)107]
Files
Fulltext by arXiv.org
BibTeX |
EndNote:
XML,
Text |
RIS