pith:ICESHCAA
Polarization Analysis of Ringdown Signals
Ringdown signals from binary black hole mergers carry measurable circular polarization that directly infers the source inclination angle.
arxiv:2605.15271 v1 · 2026-05-14 · gr-qc · astro-ph.HE
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Claims
We show that we can measure the degree of circular polarization and handedness of ringdown signals like those of GW150914, even if only the two LIGO detectors are available; such a polarization measurement can be translated into an inferred source inclination assuming the reflection symmetry above, again using the ringdown signal alone.
The assumption that merging black holes with spins (anti)aligned to the orbital angular momentum excite modes with equatorial reflection symmetry, which constrains two of the four degrees of freedom per mode and fixes the relationship between polarization amplitudes and phases via the inclination angle.
Constrained polarization model for Kerr ringdown modes enables inclination inference from two-detector data for non-precessing mergers but introduces biases when applied to precessing systems.
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| First computed | 2026-05-20T00:00:49.864705Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
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Canonical record JSON
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