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frontier-owneddeclared
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evidence atoms
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review context
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Locator and citation
locator
title:Primordial cosmology and inflation theory
imported
2026-05-29T02:16:32.199405+00:00
extraction mode
manual_curation
authors
reviewer:will-blair
Caveats
No source-specific caveats are recorded.
Primordial black hole binaries formed in the early universe have spin distributions decoupled from stellar formation pathways and can exhibit very high spins (χ → 1) if assembled from vacuum fluctuations without dissipative processes.
events
vev_08845ae91f50243cfinding.assertedManual finding added to frontier state
reviewer:will-blair · 2026-05-29
vev_f91581c9c55068eafinding.caveatedVerifier caution: Primordial BH spin reaching χ → 1 from vacuum fluctuations is highly speculative. PBH spins depend critically on formation mechanism; no canonical reference supports the claim that vacuum fluctuation assembly yields maximum spin.
reviewer:will-blair · 2026-05-29
reviewable changes
vpr_ebaf6b2c47205dc2finding.addManual finding added to frontier state
applied · reviewer:will-blair · 2026-05-29
vpr_4b367ebea6b381c0finding.caveatVerifier caution: Primordial BH spin reaching χ → 1 from vacuum fluctuations is highly speculative. PBH spins depend critically on formation mechanism; no canonical reference supports the claim that vacuum fluctuation assembly yields maximum spin.
applied · reviewer:will-blair · 2026-05-29
evaluations
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