Skip to Main content Skip to Navigation
New interface

Magnetogenesis at Cosmic Dawn

Abstract : We present a mechanism for generating cosmological magnetic fields during the Epoch of Reionization, based on the photoionization of intergalactic hydrogen. A general formula is presented, together with an example numerical application which yields magnetic field strengths between 10 −23 to 10 −19 G on intersource scales. This mechanism, which operates all along Reionization around any ionizing source, participates to the premagnetization of the whole intergalactic medium. Also, the spatial configuration of these fields may help discriminate them from those produced by other mechanisms in future observations.
Complete list of metadata
Contributor : Mathieu Langer Connect in order to contact the contributor
Submitted on : Tuesday, November 22, 2022 - 11:18:33 AM
Last modification on : Tuesday, December 6, 2022 - 4:10:00 AM

Links full text



J-B. Durrive, M. Langer. Magnetogenesis at Cosmic Dawn. Proceedings of the International Astronomical Union, 11 (S308), pp.378-379, 2014, ⟨10.1017/S1743921316010206⟩. ⟨hal-03865278⟩



Record views