pith:4VMPT7HY
Recoil kicks from binary black hole mergers in GWTC catalogs: implications for retention and hierarchical mergers
Gravitational wave data show binary black hole mergers impart recoil kicks that eject most remnants from globular clusters.
arxiv:2604.04546 v2 · 2026-04-06 · astro-ph.HE · gr-qc
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\pithnumber{4VMPT7HYUA2G2GFAHBHP3ILQBN}
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Record completeness
Claims
We obtain informative kick constraints for GW231028_153006 (839^{+1018}_{-681} km s^{-1}) and GW231123_135430 (974^{+944}_{-760} km s^{-1}); typical retention probabilities are ~1-5% for globular clusters and ~70-100% for elliptical galaxies.
The inference assumes that mass ratio and spin magnitude measurements dominate the kick posterior while spin orientation angles remain subdominant, without explicit checks on how waveform model systematics or population priors alter the reported kick values.
Recoil kicks are inferred for GWTC-4 binary black hole events with values up to nearly 1000 km/s for some, yielding retention probabilities of 1-5% in globular clusters and 70-100% in elliptical galaxies.
Formal links
Receipt and verification
| First computed | 2026-06-23T01:12:04.379243Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
e558f9fcf8a0346d18a0384efda1700b7754c735eb20a982563d87987afb5ef4
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/4VMPT7HYUA2G2GFAHBHP3ILQBN \
| jq -c '.canonical_record' \
| python3 -c "import sys,json,hashlib; b=json.dumps(json.loads(sys.stdin.read()), sort_keys=True, separators=(',',':'), ensure_ascii=False).encode(); print(hashlib.sha256(b).hexdigest())"
# expect: e558f9fcf8a0346d18a0384efda1700b7754c735eb20a982563d87987afb5ef4
Canonical record JSON
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