Decay of ultralight axion condensates

DOI10.1007/JHEP01(2018)066zbMath1384.85002arXiv1705.05385OpenAlexW3100707761MaRDI QIDQ1745484

L. C. R. Wijewardhana, Michael Ma, Joshua Eby, Peter Suranyi

Publication date: 17 April 2018

Published in: Journal of High Energy Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1705.05385

zbMATH Keywords

classical theories of gravitycosmology of theories beyond the SMFuzzy Dark Matter

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Astrophysical cosmology (85A40)

Related Items (7)

The role of the chemical potential in coupling superfluid dark matter to baryons ⋮ Classical decay rates of oscillons ⋮ Dark photon stars: formation and role as dark matter substructure ⋮ Quantum decay of scalar and vector boson stars and oscillons into gravitons ⋮ Expansion in higher harmonics of boson stars using a generalized Ruffini-Bonazzola approach. Part 1. Bound states ⋮ Three problems of superfluid dark matter and their solution ⋮ Ultralight DM bosons with an axion-like potential: scale-dependent constraints revisited

Cites Work

• QCD axion star collapse with the chiral potential
• Erratum to: Axion stars in the infrared limit
• On longevity of I-ball/oscillon
• The lifetime of axion stars
• Galactic collapse of scalar field dark matter

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