Miniclusters from axion string simulations
The University of Sydney · UNSW Sydney · +5 more institutions
Abstract
Abstract 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…
Citation impact
- FWCI
- 0.00
- Percentile
- 98%
- References
- 0
Authors
5- GPGiovanni PierobonCorresponding
The University of Sydney, UNSW Sydney
- JRJavier Redondo
Universidad de Zaragoza, Max Planck Institute for Physics
- KSKen’ichi Saikawa
Kanazawa University
- AVAlejandro Vaquero
Universidad de Zaragoza
- GDGuy D. Moore
Darmstadt University of Applied Sciences, Technische Universität Darmstadt
Topics & keywords
- Axion
- Physics
- Dark matter
- Quantum chromodynamics
- String (physics)
- Particle physics
- Universe
- Attractor
- Affordable and clean energy
Funding
- NCNational Computational Infrastructure
- AGAustralian Government
- ECEuropean CommissionAwards: 13039/501100011033, 501100011033
- UOUniversity of New South Wales
- EREuropean Regional Development FundAwards: 13039/501100011033, 501100011033
- AEAgencia Estatal de InvestigaciónAwards: 501100011033, 13039, 2020-E21-17R, RYC2020-030244-I, PGC2022-126078NB-C21, 13039/501100011033
- NCNational Cancer Institute