Three problems of superfluid dark matter and their solution

DOI10.1088/1475-7516/2021/01/025zbMath1484.83046arXiv2009.03003OpenAlexW3124734375MaRDI QIDQ5025270

Tobias Mistele

Publication date: 1 February 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2009.03003

zbMATH Keywords

modified gravitydark matter theorygalaxy dynamics

Mathematics Subject Classification ID

Hydro- and aero-acoustics (76Q05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Galactic and stellar structure (85A15) Superfluids (classical aspects) (76A25) Dark matter and dark energy (83C56)

Related Items (3)

Acausality in superfluid dark matter and MOND-like theories ⋮ Quantized vortices in superfluid dark matter ⋮ Cherenkov radiation from stars constrains hybrid MOND dark matter models

Cites Work

• UV-completion by classicalization
• Decay of ultralight axion condensates
• Recovering P(X) from a canonical complex field
• The role of the chemical potential in coupling superfluid dark matter to baryons
• The equation of state of dark matter superfluids
• Unnamed Item

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