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Replaypropertyblackholes

blackholes: dup-flood

The same posts ingested in two orders (arm B shuffled with seed 1): two graphs built side by side, with the claims the agreement metric paired linked across them. Matching is stateful, so where the graphs differ is where order mattered.

generated 2026-09-182 arms53 eventscost $0.63

Fingerprints: what built each arm

blackholes (a) · baseline snapshot bh_small

epoch       unknown
commit      unknown
profile     none: development defaults, not production
models from run
caps        not recorded
scored      2026-09-18
judge cost  none

blackholes (b) · same configuration, second run

epoch       2026-09-domain-skills
commit      2b6d590
profile     none: development defaults, not production
matcher     z-ai/glm-5.3-flash
steward     z-ai/glm-5.3-flash
curator     z-ai/glm-5.3-flash
extractor   z-ai/glm-5.3-flash
models from run
caps        stewardMaxRuns=2 stewardMaxIterations=25 curatorMaxRuns=2 curatorSweepRate=1 llmDailyTokenLimit=0 llmHourlyTokenLimit=0
scored      2026-09-18
judge cost  none
arms step by← → step · space play · esc close
1 / 21 · blackholes (a) leads
baseline snapshot bh_small0 claims · 0 edges · $0 so far
Astrophysical implications of hypothetical stable TeV-scale black holes
same configuration, second run10 claims · 11 edges · $0 so far
Astrophysical implications of hypothetical stable TeV-scale black holes0113797d-cf41-4008-a94d-42a1d3a8a33e2a6d7766-6dd3-4a70-9a2e-95d879c33f32no sourcerequiresrequirescontradictscontradictscontradictscontradictscontradictsrequiresrequirescontradictssupports
Unassessed
A microscopic black hole's accretion rate in matter is far too low to grow it significantly on planetary timescales
A microscopic black hole's accretion rate in matter is far too low to grow it significantly on planetary timescales
Contradicted0.01
Stable microscopic black holes produced at the LHC would endanger Earth.
×6
Stable microscopic black holes produced at the LHC would endanger Earth.
Unassessed
Observed white dwarfs and neutron stars exclude dangerous LHC black hole accretion scenarios.
×2
Observed white dwarfs and neutron stars exclude dangerous LHC black hole accretion scenarios.
Unassessed
The astrophysical exclusion of dangerous microscopic black hole accretion holds even without Hawking radiation.
×2
The astrophysical exclusion of dangerous microscopic black hole accretion holds even without Hawking radiation.
Unassessed
Any microscopic black hole produced at colliders evaporates essentially instantly via Hawking radiation.
×5
Any microscopic black hole produced at colliders evaporates essentially instantly via Hawking radiation.
Unassessed
Cosmic ray collisions at energies above the LHC's have struck Earth, the Moon, and dense stars for billions of years without producing dangerous black holes.
×4
Cosmic ray collisions at energies above the LHC's have struck Earth, the Moon, and dense stars for billions of years without producing dangerous black holes.
Contradicted0.02
A stable microscopic black hole trapped on Earth would accrete matter fast enough to grow and destroy the planet.
×3
A stable microscopic black hole trapped on Earth would accrete matter fast enough to grow and destroy the planet.
Unassessed
The LHC could produce microscopic black holes if large extra dimensions lower the true Planck scale to the TeV range.
The LHC could produce microscopic black holes if large extra dimensions lower the true Planck scale to the TeV range.
Unassessed
A microscopic black hole produced in a particle collision could have a velocity low enough to be gravitationally trapped inside Earth
A microscopic black hole produced in a particle collision could have a velocity low enough to be gravitationally trapped inside Earth
Unassessed
A black hole stable against Hawking evaporation must have a mass of roughly 10^15 grams or more
A black hole stable against Hawking evaporation must have a mass of roughly 10^15 grams or more

System #0 Source submitted: «Astrophysical implications of hypothetical stable TeV-scale black holes»

Agreement a ↔ b: 10 claims paired, 10 unpaired · claim-set F1 0.67 · status agreement 100% · mean credence gap 0.00 · edge edit distance 2 · hover a claim to see its pair; “no pair” marks the rest

System#017:09:36

Source submitted: «Astrophysical implications of hypothetical stable TeV-scale black holes»

Steps · none recorded

Changed the graph · attribution: harness

  • Source submitted: “Astrophysical implications of hypothetical stable TeV-scale black holes”
Past events · 0
    Legend

    System Extractor ↗ Matcher ↗ Claim Steward ↗ Curator ↗

    verified supported inconclusive doubtful contradicted unknown unassessed (hatched: pending, not a verdict) merged away touched by the current event

    Edges: requires grey, supports green, contradicts red dashed, assumes amber dotted. Gists in lists are derived by the exporter; anything marked verbatim is the model’s own text. Attribution “run-window” means a change was credited to a run by time and claim, not by a tool call that names it.