Bose–Einstein condensate of ultra-light axions as a candidate for the dark matter galaxy halos

DOI10.1142/S0217732319503619zbMath1422.85002WikidataQ127236466 ScholiaQ127236466MaRDI QIDQ5235538

Vladimir I. Tsifrinovich, Marco Merkli, Xidi Wang, Gennady P. Berman, Vyacheslav Gorshkov

Publication date: 11 October 2019

Published in: Modern Physics Letters A (Search for Journal in Brave)

zbMATH Keywords

ground statedark matterdensity distributionmean-fieldaxions

Mathematics Subject Classification ID

Quantum dynamics and nonequilibrium statistical mechanics (general) (82C10) Galactic and stellar structure (85A15)

Related Items (2)

Dark matter spin–spin interaction through the pseudo-scalar vacuum field ⋮ Two-component axionic dark matter halos

Cites Work

• Effective Evolution Equations from Quantum Dynamics
• A numerical study of the Schr dinger Newton equations

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