Warm decaying dark matter and the hubble tension

DOI10.1088/1475-7516/2020/06/005zbMath1492.83028arXiv2004.06114OpenAlexW3099308362MaRDI QIDQ5069151

Celeste Keith, Dan Hooper, Nikita G. Blinov

Publication date: 8 April 2022

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

Full work available at URL: https://arxiv.org/abs/2004.06114

zbMATH Keywords

cosmology of theories beyond the SMdark matter theorycosmological parameters from LSScosmological parameters from CMBR

Mathematics Subject Classification ID

Unified quantum theories (81V22) Relativistic cosmology (83F05) Quantum optics (81V80) Perturbations in context of PDEs (35B20) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Dark matter and dark energy (83C56)

Related Items (3)

Interacting ω(q) dark energy model with phase space analysis ⋮ Decaying warm dark matter revisited ⋮ How warm are non-thermal relics? Lyman-α bounds on out-of-equilibrium dark matter

Cites Work

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• Stellar cooling bounds on new light particles: plasma mixing effects
• Inference from iterative simulation using multiple sequences
• Precision big bang nucleosynthesis with improved helium-4 predictions

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