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CMB Bispectrum Generated from Primordial Magnetic Fields

  • Maresuke Shiraishi
Chapter
Part of the Springer Theses book series (Springer Theses)

Abstract

Recent observational consequences have shown the existence of \({\fancyscript{O}}(10^{-6}) ~\mathrm{{G}}\) magnetic fields in galaxies and clusters of galaxies at redshift \(z \sim 0.7 - 2.0\) [1-3]. One of the scenarios to realize this is an amplification of the magnetic fields by the galactic dynamo mechanism (e.g. [4]), which requires \({\fancyscript{O}}(10^{-20}) ~ \mathrm{{G}}\) seed fields prior to the galaxy formation.

Keywords

Cosmic Microwave Background Vector Mode Anisotropic Stress Tensor Mode Angular Integral 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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Copyright information

© Springer Japan 2013

Authors and Affiliations

  1. 1.Department of Physics and AstrophysicsNagoya UniversityNagoyaJapan

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