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 stateno incoming links yet
record 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
Post-merger nucleosynthesis constraints and GW190814 outlier studies
authors
reviewer:will-blair
Binary neutron star merger mass ratio (secondary/primary) follows a relatively narrow distribution with mean ~0.8-0.9, contrasting with the broader mass ratio distribution observed in binary black holes.
vs_154e60d114d32515 · manual_curation
outgoing
vf_38cb93da8114310fNarrow neutron star mass ratio distribution is consistent with common envelope channel signature, whereas broad black hole mass ratios indicate multiple formation pathways
incoming
No incoming links.
events
vev_7c27801ab7578e31finding.assertedManual finding added to frontier state
reviewer:will-blair · 2026-05-29
vev_d370355e2f6f05b6finding.caveatedVerifier caution: Claim of BNS mass ratio mean 0.8-0.9 is problematic. Web search shows Galactic BNS population has q>0.9 (nearly equal masses), with q=0.7-0.8 only proposed theoretically. The stated 'mean 0.8-0.9' does not match observational data for known merging systems. This appears unverifia
reviewer:will-blair · 2026-05-29
reviewable changes
vpr_1c91357dae425a3afinding.addManual finding added to frontier state
applied · reviewer:will-blair · 2026-05-29
vpr_d97f148df1977df3finding.caveatVerifier caution: Claim of BNS mass ratio mean 0.8-0.9 is problematic. Web search shows Galactic BNS population has q>0.9 (nearly equal masses), with q=0.7-0.8 only proposed theoretically. The stated 'mean 0.8-0.9' does not match observational data for known merging systems. This appears unverifia
applied · reviewer:will-blair · 2026-05-29
evaluations
No evaluation record targets this finding id.