{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2014:JQOTUWUWCICQGWLH2R3SR3EDT4","short_pith_number":"pith:JQOTUWUW","canonical_record":{"source":{"id":"1411.0974","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-11-04T17:24:40Z","cross_cats_sorted":["nucl-th"],"title_canon_sha256":"88c740df5c68a6c62bbf3a4af10406ec1a34cf830d6707283705eb7e4c2b3eaf","abstract_canon_sha256":"b04beb581ee04c21cb08378157ef8ec84a2cf2bce979d28795bcc4f69993d440"},"schema_version":"1.0"},"canonical_sha256":"4c1d3a5a961205035967d47728ec839f0f41749d4240b19e4d5a4c6edcfcd1f0","source":{"kind":"arxiv","id":"1411.0974","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1411.0974","created_at":"2026-05-18T01:35:51Z"},{"alias_kind":"arxiv_version","alias_value":"1411.0974v2","created_at":"2026-05-18T01:35:51Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.0974","created_at":"2026-05-18T01:35:51Z"},{"alias_kind":"pith_short_12","alias_value":"JQOTUWUWCICQ","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_16","alias_value":"JQOTUWUWCICQGWLH","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_8","alias_value":"JQOTUWUW","created_at":"2026-05-18T12:28:35Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2014:JQOTUWUWCICQGWLH2R3SR3EDT4","target":"record","payload":{"canonical_record":{"source":{"id":"1411.0974","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-11-04T17:24:40Z","cross_cats_sorted":["nucl-th"],"title_canon_sha256":"88c740df5c68a6c62bbf3a4af10406ec1a34cf830d6707283705eb7e4c2b3eaf","abstract_canon_sha256":"b04beb581ee04c21cb08378157ef8ec84a2cf2bce979d28795bcc4f69993d440"},"schema_version":"1.0"},"canonical_sha256":"4c1d3a5a961205035967d47728ec839f0f41749d4240b19e4d5a4c6edcfcd1f0","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:35:51.649437Z","signature_b64":"JtKtNJuNn6p8YUj02cmuIYNlGGaGd3Ua+wYdGqO6hDYmTJo4THpObb4ZtFuIpPhLn0CrvKdjVpIdd7bcssylDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4c1d3a5a961205035967d47728ec839f0f41749d4240b19e4d5a4c6edcfcd1f0","last_reissued_at":"2026-05-18T01:35:51.648656Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:35:51.648656Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1411.0974","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":"2026-05-18T01:35:51Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"nAEt0vtarIrvjsw9pDQOX8x3yyRFjtvW10FAwMCDYjfLN1tHJQJTlsUcuHfIDYHxqOg/dkwprTRK3LvTFwKGAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T23:09:00.308931Z"},"content_sha256":"ce4a451feb885b18dc4d88842dee1a3c91799d9476a771db1957d02e01a6a887","schema_version":"1.0","event_id":"sha256:ce4a451feb885b18dc4d88842dee1a3c91799d9476a771db1957d02e01a6a887"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2014:JQOTUWUWCICQGWLH2R3SR3EDT4","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The Role of Fission in Neutron Star Mergers and its Impact on the r-Process Peaks","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"Alexandra Kelic, Almudena Arcones, Christian Winteler, Friedrich-Karl Thielemann, Gabriel Martinez-Pinedo, Igor V. Panov, Karlheinz Langanke, Marius Eichler, Nikolaj T. Zinner, Oleg Korobkin, Stephan Rosswog, Thomas Rauscher, Tomislav Marketin","submitted_at":"2014-11-04T17:24:40Z","abstract_excerpt":"Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or explosion simulations can scrutinize two aspects: (a) the conditions in the astrophysical production site and (b) the quality of the nuclear physics input utilized. We test the abundance features of r-process nucleosynthesis calculations for the dynamical ejecta of neutron star merger simulations based on three different nuclear mass models: The Finite Range Droplet Model (FRDM), the (quenched version of the) Extended Thomas Fermi Model with Strutinsky Integral (ETFSI-Q), and the Hartree-Fock-Bo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.0974","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":"2026-05-18T01:35:51Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"8oiwGNZFQ+q3BRA+rrOoFzWAFUhnFGUsdXql/X2eLA9yY6Mjw2L+Lpvr5ucqiih7enGRSCvao5wKZamq9tEjCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T23:09:00.309607Z"},"content_sha256":"3517c2e88f62fd4f7438e6543eb7b1ac96ca25c83b69c0fd7f9fc69956be0ddc","schema_version":"1.0","event_id":"sha256:3517c2e88f62fd4f7438e6543eb7b1ac96ca25c83b69c0fd7f9fc69956be0ddc"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/JQOTUWUWCICQGWLH2R3SR3EDT4/bundle.json","state_url":"https://pith.science/pith/JQOTUWUWCICQGWLH2R3SR3EDT4/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/JQOTUWUWCICQGWLH2R3SR3EDT4/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":"2026-06-04T23:09:00Z","links":{"resolver":"https://pith.science/pith/JQOTUWUWCICQGWLH2R3SR3EDT4","bundle":"https://pith.science/pith/JQOTUWUWCICQGWLH2R3SR3EDT4/bundle.json","state":"https://pith.science/pith/JQOTUWUWCICQGWLH2R3SR3EDT4/state.json","well_known_bundle":"https://pith.science/.well-known/pith/JQOTUWUWCICQGWLH2R3SR3EDT4/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2014:JQOTUWUWCICQGWLH2R3SR3EDT4","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":"b04beb581ee04c21cb08378157ef8ec84a2cf2bce979d28795bcc4f69993d440","cross_cats_sorted":["nucl-th"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-11-04T17:24:40Z","title_canon_sha256":"88c740df5c68a6c62bbf3a4af10406ec1a34cf830d6707283705eb7e4c2b3eaf"},"schema_version":"1.0","source":{"id":"1411.0974","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1411.0974","created_at":"2026-05-18T01:35:51Z"},{"alias_kind":"arxiv_version","alias_value":"1411.0974v2","created_at":"2026-05-18T01:35:51Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1411.0974","created_at":"2026-05-18T01:35:51Z"},{"alias_kind":"pith_short_12","alias_value":"JQOTUWUWCICQ","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_16","alias_value":"JQOTUWUWCICQGWLH","created_at":"2026-05-18T12:28:35Z"},{"alias_kind":"pith_short_8","alias_value":"JQOTUWUW","created_at":"2026-05-18T12:28:35Z"}],"graph_snapshots":[{"event_id":"sha256:3517c2e88f62fd4f7438e6543eb7b1ac96ca25c83b69c0fd7f9fc69956be0ddc","target":"graph","created_at":"2026-05-18T01:35:51Z","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":"Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or explosion simulations can scrutinize two aspects: (a) the conditions in the astrophysical production site and (b) the quality of the nuclear physics input utilized. We test the abundance features of r-process nucleosynthesis calculations for the dynamical ejecta of neutron star merger simulations based on three different nuclear mass models: The Finite Range Droplet Model (FRDM), the (quenched version of the) Extended Thomas Fermi Model with Strutinsky Integral (ETFSI-Q), and the Hartree-Fock-Bo","authors_text":"Alexandra Kelic, Almudena Arcones, Christian Winteler, Friedrich-Karl Thielemann, Gabriel Martinez-Pinedo, Igor V. Panov, Karlheinz Langanke, Marius Eichler, Nikolaj T. Zinner, Oleg Korobkin, Stephan Rosswog, Thomas Rauscher, Tomislav Marketin","cross_cats":["nucl-th"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-11-04T17:24:40Z","title":"The Role of Fission in Neutron Star Mergers and its Impact on the r-Process Peaks"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1411.0974","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:ce4a451feb885b18dc4d88842dee1a3c91799d9476a771db1957d02e01a6a887","target":"record","created_at":"2026-05-18T01:35:51Z","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":"b04beb581ee04c21cb08378157ef8ec84a2cf2bce979d28795bcc4f69993d440","cross_cats_sorted":["nucl-th"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-11-04T17:24:40Z","title_canon_sha256":"88c740df5c68a6c62bbf3a4af10406ec1a34cf830d6707283705eb7e4c2b3eaf"},"schema_version":"1.0","source":{"id":"1411.0974","kind":"arxiv","version":2}},"canonical_sha256":"4c1d3a5a961205035967d47728ec839f0f41749d4240b19e4d5a4c6edcfcd1f0","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"4c1d3a5a961205035967d47728ec839f0f41749d4240b19e4d5a4c6edcfcd1f0","first_computed_at":"2026-05-18T01:35:51.648656Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:35:51.648656Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"JtKtNJuNn6p8YUj02cmuIYNlGGaGd3Ua+wYdGqO6hDYmTJo4THpObb4ZtFuIpPhLn0CrvKdjVpIdd7bcssylDg==","signature_status":"signed_v1","signed_at":"2026-05-18T01:35:51.649437Z","signed_message":"canonical_sha256_bytes"},"source_id":"1411.0974","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:ce4a451feb885b18dc4d88842dee1a3c91799d9476a771db1957d02e01a6a887","sha256:3517c2e88f62fd4f7438e6543eb7b1ac96ca25c83b69c0fd7f9fc69956be0ddc"],"state_sha256":"f13d223999d7e0674f009cb52d2458878562bb2fc2a18cb743bcba674e8119ff"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"8A4UngEg7n+e5Ua0Z1qfa0/QcjeMkvLPklaICeZRdRt3ytis4uW4qzJ2lJ0SVrLgkn5glfO+yrHvCIiEm7M8BQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-04T23:09:00.314490Z","bundle_sha256":"d9de49ab829636f2dea1d89b58d27aa2e326a59d38c80b484128cc7ba820deef"}}