Miniclusters from axion string simulations
Resumen: The properties of axion miniclusters and of the voids between them can have very strong implications for the discovery of axions and the dark matter of the Universe. These properties can be strongly affected by axion dynamics in the early Universe, such as the axion string network and the non-linear dynamics around the QCD phase transition. Recently, improvements in numerical simulation techniques have allowed us to calculate the dark matter axion field from axion strings and QCD effects using different methods: directly with low-tension strings but high resolution [1], directly with effective high-tension strings [2], or indirectly by extrapolating an attractor solution [3]. In this work, we study the properties of miniclusters in the different approaches used in the literature. We find that, while there are substantial differences in the mass distribution and internal density profiles, globally there is a similar energy distribution between minicluster halos and voids.
Idioma: Inglés
DOI: 10.1088/1475-7516/2026/05/060
Año: 2026
Publicado en: Journal of Cosmology and Astroparticle Physics 2026, 05 (2026), [23 pp.]
ISSN: 1475-7516

Financiación: info:eu-repo/grantAgreement/ES/MICINN/PGC2022-126078NB-C21
Financiación: info:eu-repo/grantAgreement/ES/MICINN/RYC2020-030244-I
Tipo y forma: Article (Published version)
Área (Departamento): Área Física Teórica (Dpto. Física Teórica)
Exportado de SIDERAL (2026-06-03-11:04:26)


Visitas y descargas

Este artículo se encuentra en las siguientes colecciones:
articulos > articulos-por-area > fisica_teorica



 Notice créée le 2026-06-03, modifiée le 2026-06-03


Versión publicada:
 PDF
Évaluer ce document:

Rate this document:
1
2
3
 
(Pas encore évalué)