Gravitational-Wave Driven Instability of Rotating Relativistic Stars

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概要

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• A brief review of the stability of rotating relativistic stars is followed by a more detailed discussion of recent work on an instability of γ-modes, modes of rotating stars that have axial parity in the slow-rotation limit. These modes may dominate the spin-down of neutron stars that are rapidly rotating at birth, and the gravitational waves they emit may be detectable.

• 理論物理学刊行会の論文
• 2000-01-31

著者

• Friedman John

  Department Of Physics University Of Wisconsin-milwavkee

• LOCKITCH Keith

  Department of Pennsylvania State University

• FRIEDMAN John

  Department of Physics, University of Wisconsin-Milwavkee

関連論文

• Gravitational-Wave Driven Instability of Rotating Relativistic Stars

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