Constraints in inflationary magnetogenesis
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Publication:2671557
DOI10.1007/s40065-021-00340-2zbMath1490.81111OpenAlexW3194859477MaRDI QIDQ2671557
Publication date: 3 June 2022
Published in: Arabian Journal of Mathematics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s40065-021-00340-2
Relativistic cosmology (83F05) Quantum field theory on curved space or space-time backgrounds (81T20) Electromagnetic fields in general relativity and gravitational theory (83C50)
Uses Software
Cites Work
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- Schwinger effect in 4D de Sitter space and constraints on magnetogenesis in the early universe
- Schwinger effect impacting primordial magnetogenesis
- A new type of isotropic cosmological models without singularity
- Inflationary magneto-(non)genesis, increasing kinetic couplings, and the strong coupling problem
- THE MAGNETIZED UNIVERSE
- Magnetogenesis by non-minimal coupling to gravity in the Starobinsky inflationary model
- Gauge field and fermion production during axion inflation
- Narrowing the window of inflationary magnetogenesis
- Viable inflationary magnetogenesis with helical coupling
- Baryogenesis from axion inflation
- Model-independent constraints in inflationary magnetogenesis
- Scale-invariant helical magnetic fields from inflation
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