{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:H6WKEQUA777DRAAHL6WW7ASUFN","short_pith_number":"pith:H6WKEQUA","canonical_record":{"source":{"id":"1706.02913","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2017-06-09T12:03:46Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"081092b91281afd2bf508da18ac80845ddbffc5efeff6359e047117fb7655618","abstract_canon_sha256":"3c39e477c6e93757f022a9c1afb67b76c1a3228fdca8662a96276bc24b83bdfc"},"schema_version":"1.0"},"canonical_sha256":"3faca24280fffe3880075fad6f82542b42649b3042c3dfebed436c765c1c35a6","source":{"kind":"arxiv","id":"1706.02913","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1706.02913","created_at":"2026-05-18T00:32:42Z"},{"alias_kind":"arxiv_version","alias_value":"1706.02913v2","created_at":"2026-05-18T00:32:42Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.02913","created_at":"2026-05-18T00:32:42Z"},{"alias_kind":"pith_short_12","alias_value":"H6WKEQUA777D","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_16","alias_value":"H6WKEQUA777DRAAH","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_8","alias_value":"H6WKEQUA","created_at":"2026-05-18T12:31:18Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:H6WKEQUA777DRAAHL6WW7ASUFN","target":"record","payload":{"canonical_record":{"source":{"id":"1706.02913","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2017-06-09T12:03:46Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"081092b91281afd2bf508da18ac80845ddbffc5efeff6359e047117fb7655618","abstract_canon_sha256":"3c39e477c6e93757f022a9c1afb67b76c1a3228fdca8662a96276bc24b83bdfc"},"schema_version":"1.0"},"canonical_sha256":"3faca24280fffe3880075fad6f82542b42649b3042c3dfebed436c765c1c35a6","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:32:42.841918Z","signature_b64":"u/cnCszBx0bKBa1xXs1xLxEK46KdsTKckP6//gfuLRy35zV+hHgF0njstDCNgrnyD/ob62CIdzSkbHDQt3qSAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3faca24280fffe3880075fad6f82542b42649b3042c3dfebed436c765c1c35a6","last_reissued_at":"2026-05-18T00:32:42.841213Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:32:42.841213Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1706.02913","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":"2026-05-18T00:32:42Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"CRKnlN7671eiccvZ3e/1QAtUVY84ApcJTl3+4umj96tTGHyYMUn0sSFNA8Oi+JMNESp6I9qZKqGJuSxzO3+EDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-26T15:46:14.945154Z"},"content_sha256":"49cdae8d16857e1d58c0addbb9ff43b56708f18861fa15026b34302ae5a383fe","schema_version":"1.0","event_id":"sha256:49cdae8d16857e1d58c0addbb9ff43b56708f18861fa15026b34302ae5a383fe"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:H6WKEQUA777DRAAHL6WW7ASUFN","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"A new temperature dependent hyperonic equation of state: application to rotating neutron star models and I-Q-relations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"nucl-th","authors_text":"J\\'er\\^ome Novak, Matthias Hempel, Micaela Oertel, Miguel Marques","submitted_at":"2017-06-09T12:03:46Z","abstract_excerpt":"In this work we present a newly constructed equation of state (EoS) --applicable to stellar core collapse and neutron star mergers--, including the entire baryon octet. Our EoS is compatible with the main constraints from nuclear physics and, in particular, with a maximum mass for cold beta-equilibrated neutron stars of 2 solar masses in agreement with recent observations. As an application of our new EoS, we compute numerical stationary models for rapidly (rigidly) rotating hot neutron stars. We consider maximum masses of hot stars, such as proto-neutron stars or hypermassive neutron stars in"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.02913","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":"2026-05-18T00:32:42Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"DXkhISjfbsrbMM5sT1BTEjcCpE0eyLcFo/IWgmKYquF9IpqGUmy+aHzxVS4yPfSxrWYPxozQVSz5uTLSZYIOBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-26T15:46:14.945519Z"},"content_sha256":"074aa53789281c781a7131630558574f300cf610f94ad468c0fe85e75dbe30a2","schema_version":"1.0","event_id":"sha256:074aa53789281c781a7131630558574f300cf610f94ad468c0fe85e75dbe30a2"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/H6WKEQUA777DRAAHL6WW7ASUFN/bundle.json","state_url":"https://pith.science/pith/H6WKEQUA777DRAAHL6WW7ASUFN/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/H6WKEQUA777DRAAHL6WW7ASUFN/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":"2026-06-26T15:46:14Z","links":{"resolver":"https://pith.science/pith/H6WKEQUA777DRAAHL6WW7ASUFN","bundle":"https://pith.science/pith/H6WKEQUA777DRAAHL6WW7ASUFN/bundle.json","state":"https://pith.science/pith/H6WKEQUA777DRAAHL6WW7ASUFN/state.json","well_known_bundle":"https://pith.science/.well-known/pith/H6WKEQUA777DRAAHL6WW7ASUFN/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:H6WKEQUA777DRAAHL6WW7ASUFN","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":"3c39e477c6e93757f022a9c1afb67b76c1a3228fdca8662a96276bc24b83bdfc","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2017-06-09T12:03:46Z","title_canon_sha256":"081092b91281afd2bf508da18ac80845ddbffc5efeff6359e047117fb7655618"},"schema_version":"1.0","source":{"id":"1706.02913","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1706.02913","created_at":"2026-05-18T00:32:42Z"},{"alias_kind":"arxiv_version","alias_value":"1706.02913v2","created_at":"2026-05-18T00:32:42Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1706.02913","created_at":"2026-05-18T00:32:42Z"},{"alias_kind":"pith_short_12","alias_value":"H6WKEQUA777D","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_16","alias_value":"H6WKEQUA777DRAAH","created_at":"2026-05-18T12:31:18Z"},{"alias_kind":"pith_short_8","alias_value":"H6WKEQUA","created_at":"2026-05-18T12:31:18Z"}],"graph_snapshots":[{"event_id":"sha256:074aa53789281c781a7131630558574f300cf610f94ad468c0fe85e75dbe30a2","target":"graph","created_at":"2026-05-18T00:32:42Z","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":"In this work we present a newly constructed equation of state (EoS) --applicable to stellar core collapse and neutron star mergers--, including the entire baryon octet. Our EoS is compatible with the main constraints from nuclear physics and, in particular, with a maximum mass for cold beta-equilibrated neutron stars of 2 solar masses in agreement with recent observations. As an application of our new EoS, we compute numerical stationary models for rapidly (rigidly) rotating hot neutron stars. We consider maximum masses of hot stars, such as proto-neutron stars or hypermassive neutron stars in","authors_text":"J\\'er\\^ome Novak, Matthias Hempel, Micaela Oertel, Miguel Marques","cross_cats":["astro-ph.HE"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2017-06-09T12:03:46Z","title":"A new temperature dependent hyperonic equation of state: application to rotating neutron star models and I-Q-relations"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1706.02913","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":"sha256:49cdae8d16857e1d58c0addbb9ff43b56708f18861fa15026b34302ae5a383fe","target":"record","created_at":"2026-05-18T00:32:42Z","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":"3c39e477c6e93757f022a9c1afb67b76c1a3228fdca8662a96276bc24b83bdfc","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2017-06-09T12:03:46Z","title_canon_sha256":"081092b91281afd2bf508da18ac80845ddbffc5efeff6359e047117fb7655618"},"schema_version":"1.0","source":{"id":"1706.02913","kind":"arxiv","version":2}},"canonical_sha256":"3faca24280fffe3880075fad6f82542b42649b3042c3dfebed436c765c1c35a6","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"3faca24280fffe3880075fad6f82542b42649b3042c3dfebed436c765c1c35a6","first_computed_at":"2026-05-18T00:32:42.841213Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:32:42.841213Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"u/cnCszBx0bKBa1xXs1xLxEK46KdsTKckP6//gfuLRy35zV+hHgF0njstDCNgrnyD/ob62CIdzSkbHDQt3qSAA==","signature_status":"signed_v1","signed_at":"2026-05-18T00:32:42.841918Z","signed_message":"canonical_sha256_bytes"},"source_id":"1706.02913","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:49cdae8d16857e1d58c0addbb9ff43b56708f18861fa15026b34302ae5a383fe","sha256:074aa53789281c781a7131630558574f300cf610f94ad468c0fe85e75dbe30a2"],"state_sha256":"9037e3af8706ddcc4b712e6d5f2c130d89472c5b6853549893c024ee6f563679"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"swdkzwsqaKFBp4FNH+8mv0/VRWgN49Le9bNCRDs4MTHcC/brNNuZ/T5UN6UQ+GbbkUpmXyL4vHbmmyeNu7TrAg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-26T15:46:14.947455Z","bundle_sha256":"988892761b0ed22c104dacb08bca2b8191074de7bf284162ac0f4817c28c15f1"}}