{"public_id":"cl_4c657f7302f3c241f73acbf85826a65c","status":"active","superseded_by_public_id":null,"corpus_id":8718439,"text":"There is a direct correlation between the strength of turbulence in the gain layer and the susceptibility to explosion in neutrino-driven core-collapse supernovae.","confidence":0.9,"paper":{"corpus_id":8718439,"title":"THE ROLE OF TURBULENCE IN NEUTRINO-DRIVEN CORE-COLLAPSE SUPERNOVA EXPLOSIONS","url":"https://sah.borca.ai/papers/8718439"},"contributors":[{"id":2,"public_id":"4715169a40","public_label":"AK (4715169a40)","roles":["extraction"],"url":"https://sah.borca.ai/u/4715169a40"},{"id":1,"public_id":"12632b8b5f","public_label":"Anonymous (12632b8b5f)","roles":["review"],"url":"https://sah.borca.ai/u/12632b8b5f"},{"id":171,"public_id":"b9tnx83g25","public_label":"eunsjani (b9tnx83g25)","roles":["review"],"url":"https://sah.borca.ai/u/b9tnx83g25"}],"origin_summary":{"object_type":"claim","status":"active","confidence":0.9,"origin_kinds":["extraction","extraction_create"],"contribution_count":1,"contribution_task_types":["extraction"],"contribution_statuses":["applied"],"verifier_verdict_count":3,"verifier_classes":["system","user_agent"],"verifier_class_counts":{"system":2,"user_agent":1},"verdict_counts":{"approve":2,"reject":1},"verifier_state":"mixed","basis":["kg_settlement_results.decision_payload.legacy_bridge","kg_entity_origin_refs","kg_assertion_proposals","contributions","verifications","claim.status","claim.confidence"],"limits":["ledger provenance is aggregated; raw contribution and verifier audit rows are not expanded","entity matching uses settlement bridge refs and edge commands"]},"concepts":[{"public_id":"co_9d92b244eee6afa61da6d57c8da328af","name":"susceptibility to explosion","description":"The likelihood or ease with which a core-collapse supernova model transitions to explosion.","types":["outcome"],"url":"https://sah.borca.ai/concepts/co_9d92b244eee6afa61da6d57c8da328af"},{"public_id":"co_d76bb8d128c5c64274165ea759144cb9","name":"turbulence in the gain layer","description":"High-Reynolds-number turbulent convection in the neutrino-heated gain layer immediately behind the stalled shock in a core-collapse supernova.","types":["phenomenon"],"url":"https://sah.borca.ai/concepts/co_d76bb8d128c5c64274165ea759144cb9"}],"related_claims":[],"url":"https://sah.borca.ai/claims/cl_4c657f7302f3c241f73acbf85826a65c"}