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Kerr quasinormal mode frequencies and excitation factors

<p>Kerr quasinormal mode frequencies and excitation factors for gravitational ($s=-2$), electromagnetic ($s=-1$), and scalar fields ($s=0$). &nbsp;Normalization is $2M=1$ except for the spin parameter $a/M$.</p> <h2>Data Format</h2> <p>$a/M$, $\mathrm{Re}(2M\omega)$, $\mathrm{Im}(2M\omega)$, $\mathrm{Re}(A)$, $\mathrm{Im}(A)$, $\mathrm{Re}(\nu)$, $\mathrm{Im}(\nu)$, $\mathrm{Re}(B)$, $\mathrm{Im}(B)$</p> <p>$M$: Mass<br>$a$: Spin parameter<br>$\omega$: Quasinormal mode frequency<br>$A$: Separation constant<br>$\nu$: Renormalized angular momentum<br>$B$: Excitation factor</p> <h2>Version History</h2> <p>Version 0.2.0: Expanded dataset with additional modes:&nbsp;<br>&nbsp; $s=-2$, $\ell=4&ndash;6$, $n=0&ndash;7$&nbsp;<br>&nbsp; $s=-1$, $\ell=2&ndash;6$, $n=0&ndash;7$<br>&nbsp; $s=0$, $\ell=1&ndash;6$, $n=0&ndash;7$<br>Version 0.1.1: Added GIF animation (no changes to dataset)<br>Version 0.1.0: Initial release with $s=-2$, $\ell=2&ndash;3$, $n=0&ndash;7$</p>

ShareScore

40/100

Overall dataset sharing score

Score breakdown

These five areas show where the dataset supports — or may limit — practical reuse.

Stewardship
4
Harmonization
4
Access
16
Reuse readiness
8
Engagement
8