{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:47LFGSMV5SICUJ446KGISYKAEZ","short_pith_number":"pith:47LFGSMV","schema_version":"1.0","canonical_sha256":"e7d6534995ec902a279cf28c896140267bcfb4b5e860492120e4f1f70214b5c5","source":{"kind":"arxiv","id":"1304.2306","version":1},"attestation_state":"computed","paper":{"title":"Nonthermal emission model of isolated X-ray pulsar RX J0420.0-5022","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Iurii Babyk, Nino Chkheidze","submitted_at":"2013-04-08T18:43:13Z","abstract_excerpt":"In the present paper an alternative theoretical interpretation to the generally assumed thermal emission models of the observed X-ray spectrum of isolated pulsar RX J0420.0-5022 is presented. It is well known that the distribution function of relativistic particles is one-dimensional at the pulsar surface. However, cyclotron instability causes an appearance of transverse momenta of relativistic electrons, which as a result, start to radiate in the synchrotron regime. On the basis of the Vlasov's kinetic equation we study the process of the quasi-linear diffusion (QLD) developed by means of the"},"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":"1304.2306","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-04-08T18:43:13Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"7ee178e444cd2bc6c32386ad05cb0090cd167451c3977d60d3b5b17026e7e5d5","abstract_canon_sha256":"5871ca26474ab6a8c47d8c023431972396cfd790b8ef5dcfef7448a9d5d872c5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:28:43.465502Z","signature_b64":"VAR6n4Nu9+urLQ53iGVVIN/swkjVvnhdJOPdgYL3QkKWOfXBygMkGv6mq9VGXj6hZHY6SF0iD3a03NRXbykbCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e7d6534995ec902a279cf28c896140267bcfb4b5e860492120e4f1f70214b5c5","last_reissued_at":"2026-05-18T03:28:43.464817Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:28:43.464817Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Nonthermal emission model of isolated X-ray pulsar RX J0420.0-5022","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Iurii Babyk, Nino Chkheidze","submitted_at":"2013-04-08T18:43:13Z","abstract_excerpt":"In the present paper an alternative theoretical interpretation to the generally assumed thermal emission models of the observed X-ray spectrum of isolated pulsar RX J0420.0-5022 is presented. It is well known that the distribution function of relativistic particles is one-dimensional at the pulsar surface. However, cyclotron instability causes an appearance of transverse momenta of relativistic electrons, which as a result, start to radiate in the synchrotron regime. On the basis of the Vlasov's kinetic equation we study the process of the quasi-linear diffusion (QLD) developed by means of the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1304.2306","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":"1304.2306","created_at":"2026-05-18T03:28:43.464909+00:00"},{"alias_kind":"arxiv_version","alias_value":"1304.2306v1","created_at":"2026-05-18T03:28:43.464909+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1304.2306","created_at":"2026-05-18T03:28:43.464909+00:00"},{"alias_kind":"pith_short_12","alias_value":"47LFGSMV5SIC","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_16","alias_value":"47LFGSMV5SICUJ44","created_at":"2026-05-18T12:27:32.513160+00:00"},{"alias_kind":"pith_short_8","alias_value":"47LFGSMV","created_at":"2026-05-18T12:27:32.513160+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/47LFGSMV5SICUJ446KGISYKAEZ","json":"https://pith.science/pith/47LFGSMV5SICUJ446KGISYKAEZ.json","graph_json":"https://pith.science/api/pith-number/47LFGSMV5SICUJ446KGISYKAEZ/graph.json","events_json":"https://pith.science/api/pith-number/47LFGSMV5SICUJ446KGISYKAEZ/events.json","paper":"https://pith.science/paper/47LFGSMV"},"agent_actions":{"view_html":"https://pith.science/pith/47LFGSMV5SICUJ446KGISYKAEZ","download_json":"https://pith.science/pith/47LFGSMV5SICUJ446KGISYKAEZ.json","view_paper":"https://pith.science/paper/47LFGSMV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1304.2306&json=true","fetch_graph":"https://pith.science/api/pith-number/47LFGSMV5SICUJ446KGISYKAEZ/graph.json","fetch_events":"https://pith.science/api/pith-number/47LFGSMV5SICUJ446KGISYKAEZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/47LFGSMV5SICUJ446KGISYKAEZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/47LFGSMV5SICUJ446KGISYKAEZ/action/storage_attestation","attest_author":"https://pith.science/pith/47LFGSMV5SICUJ446KGISYKAEZ/action/author_attestation","sign_citation":"https://pith.science/pith/47LFGSMV5SICUJ446KGISYKAEZ/action/citation_signature","submit_replication":"https://pith.science/pith/47LFGSMV5SICUJ446KGISYKAEZ/action/replication_record"}},"created_at":"2026-05-18T03:28:43.464909+00:00","updated_at":"2026-05-18T03:28:43.464909+00:00"}