pith:RWIZ4KLQ
$N$-body modelling of the ED-2 stream progenitor shows Gaia BH3's formation involved dynamical interactions
N-body simulations of the ED-2 stream progenitor show that Gaia BH3 formed through multiple dynamical interactions in the cluster.
arxiv:2604.24874 v2 · 2026-04-27 · astro-ph.GA · astro-ph.SR
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Claims
We determine that Gaia BH3 most likely formed as an exchange binary which underwent multiple strong dynamical interactions. We highlight the importance of cluster dynamics in assembling Gaia BH3, and disfavour a formation scenario where it evolved in isolation and/or in a low-density cluster.
The N-body simulations with chosen initial conditions for the progenitor cluster accurately reproduce the observed properties of the ED-2 stream and allow reliable distinction between isolated and dynamical formation channels for Gaia BH3.
N-body modeling of the ED-2 progenitor shows Gaia BH3 formed as an exchange binary via multiple dynamical interactions in a dense cluster, not in isolation.
Receipt and verification
| First computed | 2026-06-29T01:15:04.912567Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
8d919e29701e53ed2cba41f4c4b9c558f9008569229a7e4389eb31ccdb2c987c
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curl -sH 'Accept: application/ld+json' https://pith.science/pith/RWIZ4KLQDZJ62LF2IH2MJOOFLD \
| 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())"
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Canonical record JSON
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