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Energetics of turbulence generated by chiral MHD dynamos
Authors:J Schober  A Brandenburg  I Rogachevskii  N Kleeorin
Institution:1. Laboratoire d'Astrophysique, EPFL , Sauverny, Switzerland jennifer.schober@epfl.ch;3. Nordita, KTH Royal Institute of Technology and Stockholm University , Stockholm, Sweden;4. Laboratory for Atmospheric and Space Physics, JILA and Department of Astrophysical and Planetary Sciences, University of Colorado , Boulder, CO, USA;5. Department of Astronomy, Stockholm University , Stockholm, Sweden;6. Department of Mechanical Engineering, Ben-Gurion University of the Negev , Beer-Sheva, Israel
Abstract:
Keywords:Relativistic magnetohydrodynamics (MHD)  chiral MHD dynamos  turbulence  early universe
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