{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:PGUFMWFF7W465TWBPKD3YKX2TD","short_pith_number":"pith:PGUFMWFF","canonical_record":{"source":{"id":"1011.6073","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2010-11-28T19:35:13Z","cross_cats_sorted":["astro-ph.CO","astro-ph.SR","gr-qc","nucl-ex"],"title_canon_sha256":"8d7434830f24184ad5746028d375e3834a5af120270cf022b59cc20784414d41","abstract_canon_sha256":"42d6babe26a8b74e3f9b2d4f5826781758bf19eec152a11d0bf2fc79607d23c5"},"schema_version":"1.0"},"canonical_sha256":"79a85658a5fdb9eecec17a87bc2afa98d9a09fb36fa6d92e565ea3c44a1a891a","source":{"kind":"arxiv","id":"1011.6073","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1011.6073","created_at":"2026-05-18T04:23:02Z"},{"alias_kind":"arxiv_version","alias_value":"1011.6073v1","created_at":"2026-05-18T04:23:02Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1011.6073","created_at":"2026-05-18T04:23:02Z"},{"alias_kind":"pith_short_12","alias_value":"PGUFMWFF7W46","created_at":"2026-05-18T12:26:12Z"},{"alias_kind":"pith_short_16","alias_value":"PGUFMWFF7W465TWB","created_at":"2026-05-18T12:26:12Z"},{"alias_kind":"pith_short_8","alias_value":"PGUFMWFF","created_at":"2026-05-18T12:26:12Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:PGUFMWFF7W465TWBPKD3YKX2TD","target":"record","payload":{"canonical_record":{"source":{"id":"1011.6073","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2010-11-28T19:35:13Z","cross_cats_sorted":["astro-ph.CO","astro-ph.SR","gr-qc","nucl-ex"],"title_canon_sha256":"8d7434830f24184ad5746028d375e3834a5af120270cf022b59cc20784414d41","abstract_canon_sha256":"42d6babe26a8b74e3f9b2d4f5826781758bf19eec152a11d0bf2fc79607d23c5"},"schema_version":"1.0"},"canonical_sha256":"79a85658a5fdb9eecec17a87bc2afa98d9a09fb36fa6d92e565ea3c44a1a891a","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:23:02.649819Z","signature_b64":"/+dkDj17VknTgzqXZl3ozda9STzMmxuN9O+Ia266H10uOd0uClwwhZIot8uZhhzTAEgcNqP+0gcXMLoccjcuAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"79a85658a5fdb9eecec17a87bc2afa98d9a09fb36fa6d92e565ea3c44a1a891a","last_reissued_at":"2026-05-18T04:23:02.649188Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:23:02.649188Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1011.6073","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T04:23:02Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Uzr1l6+lc61XvHLI0QZ/cXgLRK/7MK7XZ8dvmGLrOdncs2Gi8McZJXNMEmaYhNJwsmjd7wEGEba5jNSxOD/pDA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-06T10:32:29.240692Z"},"content_sha256":"954cbb51522dbf708939256d4a5d3a4801086593557b3b486243261a8534925e","schema_version":"1.0","event_id":"sha256:954cbb51522dbf708939256d4a5d3a4801086593557b3b486243261a8534925e"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:PGUFMWFF7W465TWBPKD3YKX2TD","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Energy release from hadron-quark phase transition in neutron stars and the axial $w$-mode of gravitational waves","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.SR","gr-qc","nucl-ex"],"primary_cat":"nucl-th","authors_text":"Bao-An Li, Che Ming Ko, De-Hua Wen, Jun Xu, Weikang Lin","submitted_at":"2010-11-28T19:35:13Z","abstract_excerpt":"Describing the hyperonic and quark phases of neutron stars with an isospin- and momentum-dependent effective interaction for the baryon octet and the MIT bag model, respectively, and using the Gibbs conditions to construct the mixed phase, we study the energy release due to the hadron-quark phase transition. Moreover, the frequency and damping time of the first axial $w$-mode of gravitational waves are studied for both hyperonic and hybrid stars. We find that the energy release is much more sensitive to the bag constant than the density dependence of the nuclear symmetry energy. Also, the freq"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1011.6073","kind":"arxiv","version":1},"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":"2026-05-18T04:23:02Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"LOZKbCDARkh1jU8n/gB2KqDZd2GmH78Tco0AjvmTT+xUMLHMcY5K+FUarLwigRozGDPvr2TDVIZY3D7AupDaAw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-06T10:32:29.241340Z"},"content_sha256":"0b403c46b68e97e51b3dc7114d4600a3b800f491fdc423e1e582308974639111","schema_version":"1.0","event_id":"sha256:0b403c46b68e97e51b3dc7114d4600a3b800f491fdc423e1e582308974639111"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/PGUFMWFF7W465TWBPKD3YKX2TD/bundle.json","state_url":"https://pith.science/pith/PGUFMWFF7W465TWBPKD3YKX2TD/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/PGUFMWFF7W465TWBPKD3YKX2TD/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":"2026-06-06T10:32:29Z","links":{"resolver":"https://pith.science/pith/PGUFMWFF7W465TWBPKD3YKX2TD","bundle":"https://pith.science/pith/PGUFMWFF7W465TWBPKD3YKX2TD/bundle.json","state":"https://pith.science/pith/PGUFMWFF7W465TWBPKD3YKX2TD/state.json","well_known_bundle":"https://pith.science/.well-known/pith/PGUFMWFF7W465TWBPKD3YKX2TD/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:PGUFMWFF7W465TWBPKD3YKX2TD","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":"42d6babe26a8b74e3f9b2d4f5826781758bf19eec152a11d0bf2fc79607d23c5","cross_cats_sorted":["astro-ph.CO","astro-ph.SR","gr-qc","nucl-ex"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2010-11-28T19:35:13Z","title_canon_sha256":"8d7434830f24184ad5746028d375e3834a5af120270cf022b59cc20784414d41"},"schema_version":"1.0","source":{"id":"1011.6073","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1011.6073","created_at":"2026-05-18T04:23:02Z"},{"alias_kind":"arxiv_version","alias_value":"1011.6073v1","created_at":"2026-05-18T04:23:02Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1011.6073","created_at":"2026-05-18T04:23:02Z"},{"alias_kind":"pith_short_12","alias_value":"PGUFMWFF7W46","created_at":"2026-05-18T12:26:12Z"},{"alias_kind":"pith_short_16","alias_value":"PGUFMWFF7W465TWB","created_at":"2026-05-18T12:26:12Z"},{"alias_kind":"pith_short_8","alias_value":"PGUFMWFF","created_at":"2026-05-18T12:26:12Z"}],"graph_snapshots":[{"event_id":"sha256:0b403c46b68e97e51b3dc7114d4600a3b800f491fdc423e1e582308974639111","target":"graph","created_at":"2026-05-18T04:23:02Z","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":"Describing the hyperonic and quark phases of neutron stars with an isospin- and momentum-dependent effective interaction for the baryon octet and the MIT bag model, respectively, and using the Gibbs conditions to construct the mixed phase, we study the energy release due to the hadron-quark phase transition. Moreover, the frequency and damping time of the first axial $w$-mode of gravitational waves are studied for both hyperonic and hybrid stars. We find that the energy release is much more sensitive to the bag constant than the density dependence of the nuclear symmetry energy. Also, the freq","authors_text":"Bao-An Li, Che Ming Ko, De-Hua Wen, Jun Xu, Weikang Lin","cross_cats":["astro-ph.CO","astro-ph.SR","gr-qc","nucl-ex"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2010-11-28T19:35:13Z","title":"Energy release from hadron-quark phase transition in neutron stars and the axial $w$-mode of gravitational waves"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1011.6073","kind":"arxiv","version":1},"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":"sha256:954cbb51522dbf708939256d4a5d3a4801086593557b3b486243261a8534925e","target":"record","created_at":"2026-05-18T04:23:02Z","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":"42d6babe26a8b74e3f9b2d4f5826781758bf19eec152a11d0bf2fc79607d23c5","cross_cats_sorted":["astro-ph.CO","astro-ph.SR","gr-qc","nucl-ex"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2010-11-28T19:35:13Z","title_canon_sha256":"8d7434830f24184ad5746028d375e3834a5af120270cf022b59cc20784414d41"},"schema_version":"1.0","source":{"id":"1011.6073","kind":"arxiv","version":1}},"canonical_sha256":"79a85658a5fdb9eecec17a87bc2afa98d9a09fb36fa6d92e565ea3c44a1a891a","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"79a85658a5fdb9eecec17a87bc2afa98d9a09fb36fa6d92e565ea3c44a1a891a","first_computed_at":"2026-05-18T04:23:02.649188Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T04:23:02.649188Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"/+dkDj17VknTgzqXZl3ozda9STzMmxuN9O+Ia266H10uOd0uClwwhZIot8uZhhzTAEgcNqP+0gcXMLoccjcuAQ==","signature_status":"signed_v1","signed_at":"2026-05-18T04:23:02.649819Z","signed_message":"canonical_sha256_bytes"},"source_id":"1011.6073","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:954cbb51522dbf708939256d4a5d3a4801086593557b3b486243261a8534925e","sha256:0b403c46b68e97e51b3dc7114d4600a3b800f491fdc423e1e582308974639111"],"state_sha256":"a5cce31f82cbab2611d433bf23f57d1591a31425db6a77ea396924f8762b5d33"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"hUNCRUhd7wCR4EUcSTufBNlUDt56qieYCgoyF7vtmY6NONtRrfqI5AAc9wQARlaIX3eI6HC9cthhPMQ67Se3BA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-06T10:32:29.246164Z","bundle_sha256":"a63e782961cad023723a950bc185a62acdca36b68d567f7977531c7b5f617574"}}