Published July 23, 2024
| Version 0.1.1
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Kerr quasinormal mode frequencies and excitation factors
Description
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: mass
a: spin parameter
\omega: quasinormal mode frequency
A: separation constant
\nu: renormalized angular momentum
B: excitation factor
Version 0.1.1: gif animation
Version 0.1.0: s=-2, l=2--3, n=0--7
Files
s-2l2m2_w.gif
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Additional details
Related works
- Is documented by
- Preprint: arXiv:2407.15191 (arXiv)
Funding
- Japan Society for the Promotion of Science
- Grants-in-Aid for Scientific Research (KAKENHI) JP22K03639