{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:TWKO2DDJVWALKRB5TOYT3YQY2F","short_pith_number":"pith:TWKO2DDJ","schema_version":"1.0","canonical_sha256":"9d94ed0c69ad80b5443d9bb13de218d1502fde1f0bb552994d478e74b18a18bd","source":{"kind":"arxiv","id":"2010.14089","version":1},"attestation_state":"computed","paper":{"title":"Fermi-type particle acceleration from magnetic reconnection at the termination shock of a relativistic striped wind","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.HE","authors_text":"Chengkun Huang, Edison Liang, Fan Guo, Hui Li, Patrick Kilian, Yingchao Lu","submitted_at":"2020-10-27T06:14:01Z","abstract_excerpt":"An oblique-rotating pulsar generates a relativistic striped wind in a pulsar wind nebula (PWN). The termination shock of the PWN compresses the Poynting-flux-dominated flow and drives magnetic reconnection. By carrying out particle-in-cell (PIC) simulations of the termination shock of the PWN, we study the shock structure as well as the energy conversion processes and particle acceleration mechanisms. With the recent advances in the numerical methods, we extend the simulations to the ultra-relativistic regime with bulk Lorentz factor up to \\gamma_{0}=10^{6}. Magnetic reconnection at the termin"},"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":"2010.14089","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-10-27T06:14:01Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"497fb2b19dbd0e2dc134eb43dd8b5c9787ea49068555bc94d838142f8d736197","abstract_canon_sha256":"1e3bd56055b76cd66ddfc61938cbf9e5fff8688c6a5cbf043a2616fedc415118"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:19:35.490967Z","signature_b64":"5nTwqK5Wd/3mIN0Om4mIrJ+ZmEVR/gfdhHM1oP8I9IEegwiIJOplrIh9ccKZd5OO5VrcwesiNY5/8qeObHf9Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9d94ed0c69ad80b5443d9bb13de218d1502fde1f0bb552994d478e74b18a18bd","last_reissued_at":"2026-07-05T02:19:35.490510Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:19:35.490510Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fermi-type particle acceleration from magnetic reconnection at the termination shock of a relativistic striped wind","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.HE","authors_text":"Chengkun Huang, Edison Liang, Fan Guo, Hui Li, Patrick Kilian, Yingchao Lu","submitted_at":"2020-10-27T06:14:01Z","abstract_excerpt":"An oblique-rotating pulsar generates a relativistic striped wind in a pulsar wind nebula (PWN). The termination shock of the PWN compresses the Poynting-flux-dominated flow and drives magnetic reconnection. By carrying out particle-in-cell (PIC) simulations of the termination shock of the PWN, we study the shock structure as well as the energy conversion processes and particle acceleration mechanisms. With the recent advances in the numerical methods, we extend the simulations to the ultra-relativistic regime with bulk Lorentz factor up to \\gamma_{0}=10^{6}. Magnetic reconnection at the termin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2010.14089","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/2010.14089/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":"2010.14089","created_at":"2026-07-05T02:19:35.490572+00:00"},{"alias_kind":"arxiv_version","alias_value":"2010.14089v1","created_at":"2026-07-05T02:19:35.490572+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2010.14089","created_at":"2026-07-05T02:19:35.490572+00:00"},{"alias_kind":"pith_short_12","alias_value":"TWKO2DDJVWAL","created_at":"2026-07-05T02:19:35.490572+00:00"},{"alias_kind":"pith_short_16","alias_value":"TWKO2DDJVWALKRB5","created_at":"2026-07-05T02:19:35.490572+00:00"},{"alias_kind":"pith_short_8","alias_value":"TWKO2DDJ","created_at":"2026-07-05T02:19:35.490572+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/TWKO2DDJVWALKRB5TOYT3YQY2F","json":"https://pith.science/pith/TWKO2DDJVWALKRB5TOYT3YQY2F.json","graph_json":"https://pith.science/api/pith-number/TWKO2DDJVWALKRB5TOYT3YQY2F/graph.json","events_json":"https://pith.science/api/pith-number/TWKO2DDJVWALKRB5TOYT3YQY2F/events.json","paper":"https://pith.science/paper/TWKO2DDJ"},"agent_actions":{"view_html":"https://pith.science/pith/TWKO2DDJVWALKRB5TOYT3YQY2F","download_json":"https://pith.science/pith/TWKO2DDJVWALKRB5TOYT3YQY2F.json","view_paper":"https://pith.science/paper/TWKO2DDJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2010.14089&json=true","fetch_graph":"https://pith.science/api/pith-number/TWKO2DDJVWALKRB5TOYT3YQY2F/graph.json","fetch_events":"https://pith.science/api/pith-number/TWKO2DDJVWALKRB5TOYT3YQY2F/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TWKO2DDJVWALKRB5TOYT3YQY2F/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TWKO2DDJVWALKRB5TOYT3YQY2F/action/storage_attestation","attest_author":"https://pith.science/pith/TWKO2DDJVWALKRB5TOYT3YQY2F/action/author_attestation","sign_citation":"https://pith.science/pith/TWKO2DDJVWALKRB5TOYT3YQY2F/action/citation_signature","submit_replication":"https://pith.science/pith/TWKO2DDJVWALKRB5TOYT3YQY2F/action/replication_record"}},"created_at":"2026-07-05T02:19:35.490572+00:00","updated_at":"2026-07-05T02:19:35.490572+00:00"}