Kerr quasinormal mode frequencies and excitation factors
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Kerr quasinormal mode frequencies and excitation factors for gravitational waves (s=-2). Normalization is 2M=1 except for the spin parameter a/M. Data format is: a/M, Re(2M\omega), Im(2M\omega), Re(A), Im(A), Re(\nu), Im(\nu), Re(B), Im(B) M: massa: spin parameter\omega: quasinormal mode frequencyA: separation constant\nu: renormalized angular momentumB: excitation factor Version 0.1.0: s=-2, l=2--3, n=0--7
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Zenodo创建时间：
2024-07-20
