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 context1 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
Numerical relativity simulations of BHNS mergers with low mass ratio
authors
reviewer:will-blair
Black hole-neutron star mergers with symmetric mass ratios (q ≤ 1/3) leave behind massive accretion disks capable of powering bright electromagnetic transients, with numerical relativity showing 1-radian dephasing discrepancies in gravitational waveform models.
vs_441eeb042616ae90 · manual_curation
outgoing
vf_6cf7fe18126b111dSymmetric BHNS mergers with electromagnetic signatures provide multi-messenger constraints on mass-gap progenitor properties
incoming
No incoming links.
events
vev_c7fce04b3405a7fbfinding.assertedManual finding added to frontier state
reviewer:will-blair · 2026-05-29
reviewable changes
vpr_b29f1ef99a9cadb4finding.addManual finding added to frontier state
applied · reviewer:will-blair · 2026-05-29
evaluations
No evaluation record targets this finding id.