Baryon isocurvature constraints on the primordial hypermagnetic fields

DOI10.1088/1475-7516/2021/04/034zbMath1485.83148arXiv2012.14435OpenAlexW3155608896MaRDI QIDQ5026114

Kohei Kamada, Fumio Uchida, Jun'ichi Yokoyama

Publication date: 7 February 2022

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

Full work available at URL: https://arxiv.org/abs/2012.14435

zbMATH Keywords

baryon asymmetryprimordial magnetic fieldsbig bang nucleosynthesiscosmic magnetic fields theory

Mathematics Subject Classification ID

Unified quantum theories (81V22) Relativistic cosmology (83F05) Nuclear physics (81V35) Electromagnetic fields in general relativity and gravitational theory (83C50) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Weak interaction in quantum theory (81V15) Electro- and magnetostatics (78A30) Particle decays (81U90)

Related Items (5)

Effective treatment of U(1) gauge field and charged particles in axion inflation ⋮ Inflationary magnetogenesis: solving the strong coupling and its non-Gaussian signatures ⋮ Gauge field production and Schwinger reheating in runaway axion inflation ⋮ New description of the scaling evolution of the cosmological magneto-hydrodynamic system ⋮ Baryogenesis via gauge field production from a relaxing Higgs

Cites Work

• Baryogenesis from flat directions of the supersymmetric standard model
• Statistical properties of scale-invariant helical magnetic fields and applications to cosmology
• Gauge field and fermion production during axion inflation
• Baryogenesis from axion inflation
• Big Bounce Baryogenesis
• Cosmological Constraints on Isocurvature and Tensor Perturbations

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