The turbulent chiral-magnetic cascade in the early universe

The presence of asymmetry between fermions of opposite handedness in plasmas of relativistic particles can lead to exponential growth of a helical magnetic field via a small-scale chiral dynamo instability known as the chiral magnetic effect. Here, we show, using dimensional arguments and numerical...

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Veröffentlicht in:	arXiv.org 2017-08
Hauptverfasser:	Brandenburg, Axel, Schober, Jennifer, Rogachevskii, Igor, Kahniashvili, Tina, Boyarsky, Alexey, Frohlich, Jurg, Ruchayskiy, Oleg, Kleeorin, Nathan
Format:	Artikel
Sprache:	eng
Schlagworte:	Chemical potential Chirality Computer simulation Energy spectra Fermions Helicity Lorentz force Magnetic effects Magnetic fields Organic chemistry Physics - Cosmology and Nongalactic Astrophysics Physics - High Energy Astrophysical Phenomena Plasmas Relativistic particles Stability Turbulence Universe
Online-Zugang:	Volltext
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