{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:QLHPC4DCXBNQ66C2VN4IDPND7T","short_pith_number":"pith:QLHPC4DC","schema_version":"1.0","canonical_sha256":"82cef17062b85b0f785aab7881bda3fcde0f12d0f74874f5213800a98c3916c3","source":{"kind":"arxiv","id":"1408.1305","version":2},"attestation_state":"computed","paper":{"title":"Numerical models of blackbody-dominated gamma-ray bursts -- I. Hydrodynamics and the origin of the thermal emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Carlos F. Cuesta-Mart\\'inez, Miguel-\\'Angel Aloy, Petar Mimica","submitted_at":"2014-08-06T14:53:52Z","abstract_excerpt":"GRB 101225A is a prototype of the class of blackbody-dominated (BBD) gamma-ray bursts (GRBs). It has been suggested that BBD-GRBs result from the merger of a binary system formed by a neutron star and the helium core of an evolved star. We have modelled the propagation of ultrarelativistic jets through the environment left behind the merger by means of relativistic hydrodynamic simulations. In this paper, the output of our numerical models is post-processed to obtain the (thermal) radiative signature of the resulting outflow. We outline the most relevant dynamical details of the jet propagatio"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"1408.1305","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-08-06T14:53:52Z","cross_cats_sorted":[],"title_canon_sha256":"f4afa61c87515b3627fabe590673d94feadad824bafdef3debda7cc876d87509","abstract_canon_sha256":"09b10dd78775828ca7922c9c02508c13c9cc8e97be4fffe8151adf02a453ce22"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:42:23.289790Z","signature_b64":"waqa7mflZ3qKMhKl3nZL9phSLF7dRPN+Mta5UZ3M+KEwHfsm6KHzw74BshETp2dAsMsc/08QHNbV++qEwWW/Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"82cef17062b85b0f785aab7881bda3fcde0f12d0f74874f5213800a98c3916c3","last_reissued_at":"2026-05-18T01:42:23.289350Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:42:23.289350Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Numerical models of blackbody-dominated gamma-ray bursts -- I. Hydrodynamics and the origin of the thermal emission","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Carlos F. Cuesta-Mart\\'inez, Miguel-\\'Angel Aloy, Petar Mimica","submitted_at":"2014-08-06T14:53:52Z","abstract_excerpt":"GRB 101225A is a prototype of the class of blackbody-dominated (BBD) gamma-ray bursts (GRBs). It has been suggested that BBD-GRBs result from the merger of a binary system formed by a neutron star and the helium core of an evolved star. We have modelled the propagation of ultrarelativistic jets through the environment left behind the merger by means of relativistic hydrodynamic simulations. In this paper, the output of our numerical models is post-processed to obtain the (thermal) radiative signature of the resulting outflow. We outline the most relevant dynamical details of the jet propagatio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1408.1305","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1408.1305","created_at":"2026-05-18T01:42:23.289412+00:00"},{"alias_kind":"arxiv_version","alias_value":"1408.1305v2","created_at":"2026-05-18T01:42:23.289412+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1408.1305","created_at":"2026-05-18T01:42:23.289412+00:00"},{"alias_kind":"pith_short_12","alias_value":"QLHPC4DCXBNQ","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_16","alias_value":"QLHPC4DCXBNQ66C2","created_at":"2026-05-18T12:28:46.137349+00:00"},{"alias_kind":"pith_short_8","alias_value":"QLHPC4DC","created_at":"2026-05-18T12:28:46.137349+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QLHPC4DCXBNQ66C2VN4IDPND7T","json":"https://pith.science/pith/QLHPC4DCXBNQ66C2VN4IDPND7T.json","graph_json":"https://pith.science/api/pith-number/QLHPC4DCXBNQ66C2VN4IDPND7T/graph.json","events_json":"https://pith.science/api/pith-number/QLHPC4DCXBNQ66C2VN4IDPND7T/events.json","paper":"https://pith.science/paper/QLHPC4DC"},"agent_actions":{"view_html":"https://pith.science/pith/QLHPC4DCXBNQ66C2VN4IDPND7T","download_json":"https://pith.science/pith/QLHPC4DCXBNQ66C2VN4IDPND7T.json","view_paper":"https://pith.science/paper/QLHPC4DC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1408.1305&json=true","fetch_graph":"https://pith.science/api/pith-number/QLHPC4DCXBNQ66C2VN4IDPND7T/graph.json","fetch_events":"https://pith.science/api/pith-number/QLHPC4DCXBNQ66C2VN4IDPND7T/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QLHPC4DCXBNQ66C2VN4IDPND7T/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QLHPC4DCXBNQ66C2VN4IDPND7T/action/storage_attestation","attest_author":"https://pith.science/pith/QLHPC4DCXBNQ66C2VN4IDPND7T/action/author_attestation","sign_citation":"https://pith.science/pith/QLHPC4DCXBNQ66C2VN4IDPND7T/action/citation_signature","submit_replication":"https://pith.science/pith/QLHPC4DCXBNQ66C2VN4IDPND7T/action/replication_record"}},"created_at":"2026-05-18T01:42:23.289412+00:00","updated_at":"2026-05-18T01:42:23.289412+00:00"}