pith:O2LCRIVQ
Fuzzy dark matter dynamical friction: stalling of globular clusters induced by dynamical heatings
Fuzzy dark matter dynamical friction stalls globular cluster sinking in dwarf galaxies over a Hubble time.
arxiv:2510.00927 v2 · 2025-10-01 · astro-ph.GA · astro-ph.CO
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Claims
FDM dynamical friction can stall the inspiral of GCs over a Hubble time in the dwarf-galaxy regime, thereby preventing their sinking into galactic centers and halting the canonical galactic cannibalism of clusters.
The heating induced by FDM density granules is modeled accurately enough in the galpy implementation to suppress dynamical friction across the explored range of halo-to-GC mass ratios and boson masses, with the FDM-only case serving as a conservative lower bound on GC survival.
Fuzzy dark matter suppresses dynamical friction on globular clusters via granule heating, stalling their orbital decay in dwarf galaxies over a Hubble time and producing bimodal radial distributions that encode the boson mass.
Receipt and verification
| First computed | 2026-06-19T16:10:31.528221Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
769628a2b0f38fe3b3a34e36788658c664fa0032eb0f83170e36ef5c0e6162b1
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Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/O2LCRIVQ6OH6HM5DJY3HRBSYYZ \
| 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: 769628a2b0f38fe3b3a34e36788658c664fa0032eb0f83170e36ef5c0e6162b1
Canonical record JSON
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