pith:32KD3RDK
Reviving primordial black hole formation in slow first-order phase transitions
Slow reheating after supercooled phase transitions revives primordial black hole formation from curvature perturbations.
arxiv:2605.11332 v2 · 2026-05-11 · hep-ph · astro-ph.CO · gr-qc
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\pithnumber{32KD3RDKOTGGPRYAGCHYL2FTK7}
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Claims
we show that this mechanism remains viable: after a supercooled transition, reheating can be sufficiently slow that the Universe enters an early matter-dominated era, during which even small overdensities grow and collapse into primordial black holes.
Reheating after the supercooled transition is sufficiently slow to allow the Universe to enter an early matter-dominated era.
Primordial black hole formation from slow first-order phase transitions remains viable if slow reheating after supercooling creates an early matter-dominated era allowing small overdensities to grow, producing black holes with large spins.
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| First computed | 2026-05-22T01:04:05.989118Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
de943dc46a74cc67c700308f85e8b357f9459307b698085abfd60592c7710222
Aliases
· · · · ·Agent API
Verify this Pith Number yourself
curl -sH 'Accept: application/ld+json' https://pith.science/pith/32KD3RDKOTGGPRYAGCHYL2FTK7 \
| 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: de943dc46a74cc67c700308f85e8b357f9459307b698085abfd60592c7710222
Canonical record JSON
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