HELICAL MAGNETIC FIELDS FROM INFLATION
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Publication:3401060
DOI10.1142/S0218271809015175zbMath1181.83216arXiv0805.0575OpenAlexW3103136689MaRDI QIDQ3401060
Publication date: 28 January 2010
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/0805.0575
Relativistic cosmology (83F05) Electromagnetic fields in general relativity and gravitational theory (83C50)
Related Items (9)
Hypermagnetic knots and gravitational radiation at intermediate frequencies ⋮ Viable inflationary magnetogenesis with helical coupling ⋮ Inflationary magnetogenesis: solving the strong coupling and its non-Gaussian signatures ⋮ Statistical properties of scale-invariant helical magnetic fields and applications to cosmology ⋮ Enhancing the cross-correlations between magnetic fields and scalar perturbations through parity violation ⋮ Probing non-classicality of primordial gravitational waves and magnetic field through quantum Poincaré sphere ⋮ Reduced bispectrum seeded by helical primordial magnetic fields ⋮ Inflationary magnetogenesis with reheating phase from higher curvature coupling ⋮ Effective theory of inflationary magnetogenesis and constraints on reheating
Cites Work
- Generation of electromagnetic fields in string cosmology with a massive scalar field on the anti-D-brane
- Effects of cosmological magnetic helicity on the CMB
- ON SIGNATURES OF SHORT DISTANCE PHYSICS IN THE COSMIC MICROWAVE BACKGROUND
- THE MAGNETIZED UNIVERSE
- Generation of Large Scale Magnetic Fields by Coupling to Curvature and Dilaton Field
- Entropy perturbations and large-scale magnetic fields
- Magnetic fields in the aftermath of phase transitions
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