{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:3MNF3MDVCNB6SKZUZKMF5S65FO","short_pith_number":"pith:3MNF3MDV","schema_version":"1.0","canonical_sha256":"db1a5db0751343e92b34ca985ecbdd2bbc85a9ce78602b6b382c1cf779f4b7af","source":{"kind":"arxiv","id":"1101.2433","version":1},"attestation_state":"computed","paper":{"title":"Massive particle production from accelerated sources in high magnetic fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alberto Saa, Douglas Fregolente","submitted_at":"2011-01-12T19:59:54Z","abstract_excerpt":"Non-electromagnetic emissions from high energy particles in extreme environments has been studied in the literature by using several variations of the semi-classical formalism. The detailed mechanisms behind such emissions are of great astrophysical interest since they can alter appreciably the associated energy loss rates. Here, we review the role played by the source proper acceleration $a$ in the particle production process. The acceleration $a$ determines the typical scale characterizing the particle production and, moreover, if the massive particle production is inertially forbidden, it w"},"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":"1101.2433","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2011-01-12T19:59:54Z","cross_cats_sorted":[],"title_canon_sha256":"52c13faceea6360d21dacbae54cbaef7c3c2032e1dda8dec298277786906b7fe","abstract_canon_sha256":"4f9abff3d1165718ca3395448c70b8acf6623d26788358525612f5872cc615a0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:31:43.043337Z","signature_b64":"HPNZt6Dt1iLKGhR3e0wW1hMkmQ6kyq3Cx7GrFCereIh4XYYZnkX9HkXvsDWvzo3Eq+34Sap2m/DMkBD+zKKgCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"db1a5db0751343e92b34ca985ecbdd2bbc85a9ce78602b6b382c1cf779f4b7af","last_reissued_at":"2026-05-18T04:31:43.042918Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:31:43.042918Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Massive particle production from accelerated sources in high magnetic fields","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Alberto Saa, Douglas Fregolente","submitted_at":"2011-01-12T19:59:54Z","abstract_excerpt":"Non-electromagnetic emissions from high energy particles in extreme environments has been studied in the literature by using several variations of the semi-classical formalism. The detailed mechanisms behind such emissions are of great astrophysical interest since they can alter appreciably the associated energy loss rates. Here, we review the role played by the source proper acceleration $a$ in the particle production process. The acceleration $a$ determines the typical scale characterizing the particle production and, moreover, if the massive particle production is inertially forbidden, it w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.2433","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1101.2433","created_at":"2026-05-18T04:31:43.042973+00:00"},{"alias_kind":"arxiv_version","alias_value":"1101.2433v1","created_at":"2026-05-18T04:31:43.042973+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.2433","created_at":"2026-05-18T04:31:43.042973+00:00"},{"alias_kind":"pith_short_12","alias_value":"3MNF3MDVCNB6","created_at":"2026-05-18T12:26:18.847500+00:00"},{"alias_kind":"pith_short_16","alias_value":"3MNF3MDVCNB6SKZU","created_at":"2026-05-18T12:26:18.847500+00:00"},{"alias_kind":"pith_short_8","alias_value":"3MNF3MDV","created_at":"2026-05-18T12:26:18.847500+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/3MNF3MDVCNB6SKZUZKMF5S65FO","json":"https://pith.science/pith/3MNF3MDVCNB6SKZUZKMF5S65FO.json","graph_json":"https://pith.science/api/pith-number/3MNF3MDVCNB6SKZUZKMF5S65FO/graph.json","events_json":"https://pith.science/api/pith-number/3MNF3MDVCNB6SKZUZKMF5S65FO/events.json","paper":"https://pith.science/paper/3MNF3MDV"},"agent_actions":{"view_html":"https://pith.science/pith/3MNF3MDVCNB6SKZUZKMF5S65FO","download_json":"https://pith.science/pith/3MNF3MDVCNB6SKZUZKMF5S65FO.json","view_paper":"https://pith.science/paper/3MNF3MDV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1101.2433&json=true","fetch_graph":"https://pith.science/api/pith-number/3MNF3MDVCNB6SKZUZKMF5S65FO/graph.json","fetch_events":"https://pith.science/api/pith-number/3MNF3MDVCNB6SKZUZKMF5S65FO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3MNF3MDVCNB6SKZUZKMF5S65FO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3MNF3MDVCNB6SKZUZKMF5S65FO/action/storage_attestation","attest_author":"https://pith.science/pith/3MNF3MDVCNB6SKZUZKMF5S65FO/action/author_attestation","sign_citation":"https://pith.science/pith/3MNF3MDVCNB6SKZUZKMF5S65FO/action/citation_signature","submit_replication":"https://pith.science/pith/3MNF3MDVCNB6SKZUZKMF5S65FO/action/replication_record"}},"created_at":"2026-05-18T04:31:43.042973+00:00","updated_at":"2026-05-18T04:31:43.042973+00:00"}