record state
frontier-ownedReview status
This finding is part of accepted frontier state. Review events, reviewable changes, and proof state explain how it can change.
unreviewed
frontiers / frontier
Finding bundle
back to staterecord state
frontier-ownedThis finding is part of accepted frontier state. Review events, reviewable changes, and proof state explain how it can change.
finding statement
finding typeNo entity list is declared.
evidence
source-boundtheoretical · manual state transition
proof impact
packet context2 reviewable changes and 0 evaluation records are attached to this finding id.
Evidence and conditions
method
manual state transition
evidence type
theoretical
conditions
Provenance
source title
Primordial cosmology and inflation theory
authors
reviewer:will-blair
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.
vs_41f8db1ec7085fbc · manual_curation
outgoing
No outgoing links.
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
No evaluation record targets this finding id.