Scale-invariant helical magnetic fields from inflation

DOI10.1088/1475-7516/2019/09/008OpenAlexW2994726023MaRDI QIDQ5861825

Ruth Durrer, Tomohiro Fujita

Publication date: 2 March 2022

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

Full work available at URL: https://arxiv.org/abs/1904.11428

zbMATH Keywords

inflationprimordial magnetic fieldsextragalactic magnetic fields

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items

Effective treatment of U(1) gauge field and charged particles in axion inflation, Palatini approach and large-scale magnetogenesis, Baryogenesis from axion inflation, Resonant magnetogenesis from axions, Generation of primordial black holes and gravitational waves from dilaton-gauge field dynamics, Model-independent constraints in inflationary magnetogenesis, Constraints in inflationary magnetogenesis, When does the Schwinger preheating occur?, Geometric structure of multi-form-field isotropic inflation and primordial fluctuations, Gravitational wave trispectrum in the axion-SU(2) model, Impact of helical electromagnetic fields on the axion window, Chiral gravitational waves produced in a helical magnetogenesis model, Small-scale CMB anisotropies induced by the primordial magnetic fields, Observing primordial magnetic fields through Dark Matter

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