Merger of dark matter axion clumps and resonant photon emission

DOI10.1088/1475-7516/2020/07/067zbMath1492.83038arXiv2005.02405OpenAlexW3104213467WikidataQ109745380 ScholiaQ109745380MaRDI QIDQ5070305

Mark P. Hertzberg, Enrico D. Schiappacasse, Yao Li

Publication date: 11 April 2022

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

Full work available at URL: https://arxiv.org/abs/2005.02405

zbMATH Keywords

starsaxionsparticle physics-cosmology connectiondark matter simulations

Mathematics Subject Classification ID

Unified quantum theories (81V22) Relativistic cosmology (83F05) Other elementary particle theory in quantum theory (81V25) Quantum optics (81V80) Galactic and stellar structure (85A15) Resonance in context of PDEs (35B34) Collisions in celestial mechanics, regularization (70F16) Dark matter and dark energy (83C56) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)

Related Items (7)

Two-scalar Bose-Einstein condensates: from stars to galaxies ⋮ Gravitational decoherence of dark matter ⋮ How to suppress exponential growth—on the parametric resonance of photons in an axion background ⋮ Ultralight scalar decay and the Hubble tension ⋮ Small-scale structure in vector dark matter ⋮ Beyond Schrödinger-Poisson: nonrelativistic effective field theory for scalar dark matter ⋮ Electromagnetic bursts from mergers of oscillons in axion-like fields

Cites Work

• Dark energy-like stars from nonminimally coupled scalar field
• Flux compactification
• Scalar dark matter clumps with angular momentum
• Can axion clumps be formed in a pre-inflationary scenario?
• Probing dynamics of boson stars by fast radio bursts and gravitational wave detection
• How to suppress exponential growth—on the parametric resonance of photons in an axion background
• Dynamical boson stars

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