{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:GVJCUIPG3P3PKJX6ZRPQIKIMZN","short_pith_number":"pith:GVJCUIPG","canonical_record":{"source":{"id":"1711.00477","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-11-01T18:00:06Z","cross_cats_sorted":["hep-ph","nucl-th"],"title_canon_sha256":"1904ed8b58c926219028513d93f5696f3123ab8fdc9cfac9c3051f45a879d450","abstract_canon_sha256":"cf2f90dffe301d483ef52b2be20582d3904ae0b5e9665145b5fe97a5099cbd0c"},"schema_version":"1.0"},"canonical_sha256":"35522a21e6dbf6f526fecc5f04290ccb525eb49025ab8f43fda47bd01aed1149","source":{"kind":"arxiv","id":"1711.00477","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1711.00477","created_at":"2026-05-18T00:26:53Z"},{"alias_kind":"arxiv_version","alias_value":"1711.00477v2","created_at":"2026-05-18T00:26:53Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.00477","created_at":"2026-05-18T00:26:53Z"},{"alias_kind":"pith_short_12","alias_value":"GVJCUIPG3P3P","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_16","alias_value":"GVJCUIPG3P3PKJX6","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_8","alias_value":"GVJCUIPG","created_at":"2026-05-18T12:31:18Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:GVJCUIPG3P3PKJX6ZRPQIKIMZN","target":"record","payload":{"canonical_record":{"source":{"id":"1711.00477","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-11-01T18:00:06Z","cross_cats_sorted":["hep-ph","nucl-th"],"title_canon_sha256":"1904ed8b58c926219028513d93f5696f3123ab8fdc9cfac9c3051f45a879d450","abstract_canon_sha256":"cf2f90dffe301d483ef52b2be20582d3904ae0b5e9665145b5fe97a5099cbd0c"},"schema_version":"1.0"},"canonical_sha256":"35522a21e6dbf6f526fecc5f04290ccb525eb49025ab8f43fda47bd01aed1149","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:26:53.683954Z","signature_b64":"NQpoXFLNVrbHJ5ou2bPPqYCjvVcIZEMfpiWnvaBpuu/by2+TlPjxJKXwsuQhQvz0eFi5a9erYjTCOH8GtovsCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"35522a21e6dbf6f526fecc5f04290ccb525eb49025ab8f43fda47bd01aed1149","last_reissued_at":"2026-05-18T00:26:53.683288Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:26:53.683288Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1711.00477","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:26:53Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"SiUv76hXpyvbm0EyCofcelc/zXD+cmtZkEppVwtEbw6NYnls5vTj88SDgb07K99c2O77GWErlb7hRnmQbU7ZDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T21:09:57.336231Z"},"content_sha256":"85b44edd6dae75ab3d525d25ae18223a98645ced434f5074dfb37c8d58dea34a","schema_version":"1.0","event_id":"sha256:85b44edd6dae75ab3d525d25ae18223a98645ced434f5074dfb37c8d58dea34a"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:GVJCUIPG3P3PKJX6ZRPQIKIMZN","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Imprints of neutrino-pair flavor conversions on nucleosynthesis in ejecta from neutron-star merger remnants","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"Hans-Thomas Janka, Irene Tamborra, Meng-Ru Wu, Oliver Just","submitted_at":"2017-11-01T18:00:06Z","abstract_excerpt":"The remnant of neutron star mergers is dense in neutrinos. By employing inputs from one hydrodynamical simulation of a binary neutron star merger remnant with a black hole of $3\\ M_\\odot$ in the center, dimensionless spin parameter $0.8$ and an accretion torus of $0.3\\ M_\\odot$, the neutrino emission properties are investigated as the merger remnant evolves. Initially, the local number density of $\\bar{\\nu}_e$ is larger than that of $\\nu_e$ everywhere above the remnant. Then, as the torus approaches self-regulated equilibrium, the local abundance of neutrinos overcomes that of antineutrinos in"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.00477","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:26:53Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"lm5As3Z0Z8NZSMFg8ACUBEPkDT3gyzbB6dT3eQ2/zPr1t/coBfKwImxEE8anTLEBuBuogDgFIZ5e/fTWeNwvCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-28T21:09:57.336972Z"},"content_sha256":"b96b5e5df5d209b20517e5880bf2c839d66e96646fc9e38d77cd490bdb42b90f","schema_version":"1.0","event_id":"sha256:b96b5e5df5d209b20517e5880bf2c839d66e96646fc9e38d77cd490bdb42b90f"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/GVJCUIPG3P3PKJX6ZRPQIKIMZN/bundle.json","state_url":"https://pith.science/pith/GVJCUIPG3P3PKJX6ZRPQIKIMZN/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/GVJCUIPG3P3PKJX6ZRPQIKIMZN/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-28T21:09:57Z","links":{"resolver":"https://pith.science/pith/GVJCUIPG3P3PKJX6ZRPQIKIMZN","bundle":"https://pith.science/pith/GVJCUIPG3P3PKJX6ZRPQIKIMZN/bundle.json","state":"https://pith.science/pith/GVJCUIPG3P3PKJX6ZRPQIKIMZN/state.json","well_known_bundle":"https://pith.science/.well-known/pith/GVJCUIPG3P3PKJX6ZRPQIKIMZN/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:GVJCUIPG3P3PKJX6ZRPQIKIMZN","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"cf2f90dffe301d483ef52b2be20582d3904ae0b5e9665145b5fe97a5099cbd0c","cross_cats_sorted":["hep-ph","nucl-th"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-11-01T18:00:06Z","title_canon_sha256":"1904ed8b58c926219028513d93f5696f3123ab8fdc9cfac9c3051f45a879d450"},"schema_version":"1.0","source":{"id":"1711.00477","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1711.00477","created_at":"2026-05-18T00:26:53Z"},{"alias_kind":"arxiv_version","alias_value":"1711.00477v2","created_at":"2026-05-18T00:26:53Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.00477","created_at":"2026-05-18T00:26:53Z"},{"alias_kind":"pith_short_12","alias_value":"GVJCUIPG3P3P","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_16","alias_value":"GVJCUIPG3P3PKJX6","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_8","alias_value":"GVJCUIPG","created_at":"2026-05-18T12:31:18Z"}],"graph_snapshots":[{"event_id":"sha256:b96b5e5df5d209b20517e5880bf2c839d66e96646fc9e38d77cd490bdb42b90f","target":"graph","created_at":"2026-05-18T00:26:53Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"The remnant of neutron star mergers is dense in neutrinos. By employing inputs from one hydrodynamical simulation of a binary neutron star merger remnant with a black hole of $3\\ M_\\odot$ in the center, dimensionless spin parameter $0.8$ and an accretion torus of $0.3\\ M_\\odot$, the neutrino emission properties are investigated as the merger remnant evolves. Initially, the local number density of $\\bar{\\nu}_e$ is larger than that of $\\nu_e$ everywhere above the remnant. Then, as the torus approaches self-regulated equilibrium, the local abundance of neutrinos overcomes that of antineutrinos in","authors_text":"Hans-Thomas Janka, Irene Tamborra, Meng-Ru Wu, Oliver Just","cross_cats":["hep-ph","nucl-th"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-11-01T18:00:06Z","title":"Imprints of neutrino-pair flavor conversions on nucleosynthesis in ejecta from neutron-star merger remnants"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.00477","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:85b44edd6dae75ab3d525d25ae18223a98645ced434f5074dfb37c8d58dea34a","target":"record","created_at":"2026-05-18T00:26:53Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"cf2f90dffe301d483ef52b2be20582d3904ae0b5e9665145b5fe97a5099cbd0c","cross_cats_sorted":["hep-ph","nucl-th"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-11-01T18:00:06Z","title_canon_sha256":"1904ed8b58c926219028513d93f5696f3123ab8fdc9cfac9c3051f45a879d450"},"schema_version":"1.0","source":{"id":"1711.00477","kind":"arxiv","version":2}},"canonical_sha256":"35522a21e6dbf6f526fecc5f04290ccb525eb49025ab8f43fda47bd01aed1149","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"35522a21e6dbf6f526fecc5f04290ccb525eb49025ab8f43fda47bd01aed1149","first_computed_at":"2026-05-18T00:26:53.683288Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:26:53.683288Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"NQpoXFLNVrbHJ5ou2bPPqYCjvVcIZEMfpiWnvaBpuu/by2+TlPjxJKXwsuQhQvz0eFi5a9erYjTCOH8GtovsCg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:26:53.683954Z","signed_message":"canonical_sha256_bytes"},"source_id":"1711.00477","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:85b44edd6dae75ab3d525d25ae18223a98645ced434f5074dfb37c8d58dea34a","sha256:b96b5e5df5d209b20517e5880bf2c839d66e96646fc9e38d77cd490bdb42b90f"],"state_sha256":"d136ed15b21b82c1ddb8f2ec047f39b5b1e0431c0dc65599b3e7f74dcf4e1976"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"G3Li4i/qXAMBtW9A3BMB58xZncRwb/SRuh7SBq07V6zyyZTacDfDLXqdqX7K5uc7b0712nGhBZonFIBuT15BCA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-28T21:09:57.341116Z","bundle_sha256":"d3c89ea8eedcf85f600216bb9bbf2ffd1c58d2c0ce68830c6ab98147da68c959"}}