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ROBUSTLY UNSTABLE EIGENMODESOF THE MAGNETOSHEARING INSTABILITY IN ACCRETION DISK

ROBUSTLY UNSTABLE EIGENMODESOF THE MAGNETOSHEARING INSTABILITY IN ACCRETION DISK

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その他
Author
松元, 亮治
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Digital
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NDC
440
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出版タイプ: AOtype:textThe stability of nonaxisymmetric perturbations in dierentially rotating astrophysical accretion disksis analyzed by fully incorporat...

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Material Type
その他
Author/Editor
松元, 亮治
NDC
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一般
Note (General)
出版タイプ: AO
type:text
The stability of nonaxisymmetric perturbations in dierentially rotating astrophysical accretion disksis analyzed by fully incorporating the properties of shear flows. We verify the presence of discrete unstableeigenmodes with complex and pure imaginary eigenvalues, without any artificial disk edge boundaries,unlike Ogilvie & Pringle(1996)'s claim. By developing the mathematical theory of a non-self-adjointsystem, we investigate the nonlocal behavior of eigenmodes in the vicinity of Alfv´en singularities at!D = ±!A, where !D is the Doppler-shifted wave frequency and !A = kkvA is the Alfv´en frequency.The structure of the spectrum of discrete eigenmodes is discussed and the magnetic field and wavenumberdependence of the growth rate are obtained. Exponentially growing modes are present even in a regionwhere the local dispersion relation theory claims to have stable eigenvalues. The velocity field created byan eigenmode is obtained, which explains the anomalous angular momentum transport in the nonlinearstage of this stability.
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国立情報学研究所 : 学術機関リポジトリデータベース(IRDB)(機関リポジトリ)
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千葉大学 : 千葉大学学術成果リポジトリ