Chiral gravitational waves produced in a helical magnetogenesis model
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Publication:5025993
DOI10.1088/1475-7516/2021/03/026zbMath1484.83146arXiv2005.13833OpenAlexW3030569586MaRDI QIDQ5025993
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/2005.13833
Relativistic cosmology (83F05) Magnetohydrodynamics and electrohydrodynamics (76W05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Gravitational waves (83C35)
Related Items (4)
Chiral gravitational waves from thermalized neutrinos in the early Universe ⋮ When does the Schwinger preheating occur? ⋮ Gauge field production and Schwinger reheating in runaway axion inflation ⋮ Inflation with two-form field: the production of primordial black holes and gravitational waves
Cites Work
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- Energetics of turbulence generated by chiral MHD dynamos
- Baryogenesis from axion inflation
- Big Bounce Baryogenesis
- Model-independent constraints in inflationary magnetogenesis
- On Gauge Invariance and Vacuum Polarization
- Scale-invariant helical magnetic fields from inflation
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