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: Artículo (Versión definitiva) Área (Departamento): Área Física Teórica (Dpto. Física Teórica)