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Gravitational Waves from Relativistic Stars

Yasufumi Kojima
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Abstract

Stellar pulsations in rotating relativistic stars are reviewed. Slow rotation approximation is applied to solving the Einstein equations. The rotational effects on the non-axisymmetric oscillations are explicitly shown in the polar and axial modes.

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Yasufumi Kojima. 2000-02-23. Gravitational Waves from Relativistic Stars. https://doi.org/10.1143/ptps.136.135

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