Back Reaction to the Spectrum of Magnetic Field in the Kinetic Dynamo Theory : Modified Kulsrud-Anderson Equation : Astrophysics and Relativity

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概要

• 論文の詳細を見る

• We take account of the lowest order back reaction on a fluid and modify the Kulsrud-Anderson equation, ∂_tε_M = 2_γε_M , obtained in the kinetic dynamo theory, where ε_M is the energy density of the magnetic field. We apply our results to certain astrophysical stages where the magnetic field is expected to be amplified by the dynamo mechanism.

• 理論物理学刊行会の論文
• 1999-01-25

著者

• NISHI Ryoichi

  Department of Physics,Kyoto University

• Nishi R

  Department Of Physics Niigata University

• Nishi Ryoichi

  Department Of Physics Kyoto University

• SHIROMlZU Tetsuya

  Department of Physics, Tokyo Institute, of Technology

• NISHI Ryoichi

  Physics Department, Kyoto University

• SHIROMUZI Tetsuya

  Department of Physics, The University of Tokyo

• Shiromizu Tetsuya

  Damtp University Of Cambridge:department Of Physics The University Of Tokyo:research Center For The

• Shiromizu Tetsuya

  Damtp University Of Cambridge:department Of Physics And Resceu The University Of Tokyo

• NISHI Ryoichi

  Department of Physics, Kyoto Urhiversity

• SHIROMIZU Tetsuya

  DAMTP, University of Cambridge:Department of Physics, The University of Tokyo:Research Center for the Early Universe (RESCEU) The University of Tokyo

• SHIROMIZU Tetsuya

  Research Center for the Early Universe (RESCEU), The University of Tokyo

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