{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:ZUXSQEYXHZKEXPRCADU7CKXLBD","short_pith_number":"pith:ZUXSQEYX","schema_version":"1.0","canonical_sha256":"cd2f2813173e544bbe2200e9f12aeb08d47580dbe9866689e387ae3fceddb37a","source":{"kind":"arxiv","id":"2009.08722","version":1},"attestation_state":"computed","paper":{"title":"Effects of modified theories of gravity on neutrino pair annihilation energy deposition near neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Gaetano Lambiase, Leonardo Mastrototaro","submitted_at":"2020-09-18T09:54:20Z","abstract_excerpt":"We study the neutrino pairs annihilation into electron-positron pairs ($\\nu+{\\bar \\nu}\\to e^- + e^+$) near the surface of a neutron star. The analysis is performed in the framework of extended theories of gravity. The latter induce a modification of the minimum photon-sphere radius ($R_{ph}$) and the maximum energy deposition rate near to $R_{ph}$, as compared to ones of General Relativity. These results might lead to an efficient mechanism for generating GRBs."},"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":"2009.08722","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-09-18T09:54:20Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"71e882c9a6dc87cdc27281a1504d35d8d7439b7dad73e0ec2c25fc7441e70b51","abstract_canon_sha256":"b48812457c09f29211fb7ba62b1354a00858d593b54aee979c7513e3ae96a902"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:53:10.044457Z","signature_b64":"rrt3SfnYqL+Jqn2QGUgrngU0wptxdNMRf+cRyUaAkwo8phxW8eyYXaft081BHshtg6NV76X7B4vAkX//yAcnAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cd2f2813173e544bbe2200e9f12aeb08d47580dbe9866689e387ae3fceddb37a","last_reissued_at":"2026-07-05T01:53:10.044038Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:53:10.044038Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Effects of modified theories of gravity on neutrino pair annihilation energy deposition near neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Gaetano Lambiase, Leonardo Mastrototaro","submitted_at":"2020-09-18T09:54:20Z","abstract_excerpt":"We study the neutrino pairs annihilation into electron-positron pairs ($\\nu+{\\bar \\nu}\\to e^- + e^+$) near the surface of a neutron star. The analysis is performed in the framework of extended theories of gravity. The latter induce a modification of the minimum photon-sphere radius ($R_{ph}$) and the maximum energy deposition rate near to $R_{ph}$, as compared to ones of General Relativity. These results might lead to an efficient mechanism for generating GRBs."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2009.08722","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2009.08722/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2009.08722","created_at":"2026-07-05T01:53:10.044093+00:00"},{"alias_kind":"arxiv_version","alias_value":"2009.08722v1","created_at":"2026-07-05T01:53:10.044093+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2009.08722","created_at":"2026-07-05T01:53:10.044093+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZUXSQEYXHZKE","created_at":"2026-07-05T01:53:10.044093+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZUXSQEYXHZKEXPRC","created_at":"2026-07-05T01:53:10.044093+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZUXSQEYX","created_at":"2026-07-05T01:53:10.044093+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.20931","citing_title":"Scattering, Hawking Radiation and Neutrino Energy Deposition in Euler-Heisenberg Black Holes Surrounded by Perfect Fluid Dark Matter","ref_index":29,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZUXSQEYXHZKEXPRCADU7CKXLBD","json":"https://pith.science/pith/ZUXSQEYXHZKEXPRCADU7CKXLBD.json","graph_json":"https://pith.science/api/pith-number/ZUXSQEYXHZKEXPRCADU7CKXLBD/graph.json","events_json":"https://pith.science/api/pith-number/ZUXSQEYXHZKEXPRCADU7CKXLBD/events.json","paper":"https://pith.science/paper/ZUXSQEYX"},"agent_actions":{"view_html":"https://pith.science/pith/ZUXSQEYXHZKEXPRCADU7CKXLBD","download_json":"https://pith.science/pith/ZUXSQEYXHZKEXPRCADU7CKXLBD.json","view_paper":"https://pith.science/paper/ZUXSQEYX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2009.08722&json=true","fetch_graph":"https://pith.science/api/pith-number/ZUXSQEYXHZKEXPRCADU7CKXLBD/graph.json","fetch_events":"https://pith.science/api/pith-number/ZUXSQEYXHZKEXPRCADU7CKXLBD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZUXSQEYXHZKEXPRCADU7CKXLBD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZUXSQEYXHZKEXPRCADU7CKXLBD/action/storage_attestation","attest_author":"https://pith.science/pith/ZUXSQEYXHZKEXPRCADU7CKXLBD/action/author_attestation","sign_citation":"https://pith.science/pith/ZUXSQEYXHZKEXPRCADU7CKXLBD/action/citation_signature","submit_replication":"https://pith.science/pith/ZUXSQEYXHZKEXPRCADU7CKXLBD/action/replication_record"}},"created_at":"2026-07-05T01:53:10.044093+00:00","updated_at":"2026-07-05T01:53:10.044093+00:00"}