{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:FPSJ26YE4L26IK4BKXY7Y4U5IR","short_pith_number":"pith:FPSJ26YE","schema_version":"1.0","canonical_sha256":"2be49d7b04e2f5e42b8155f1fc729d4447f1a3569effcfc38c76d11cbb27629b","source":{"kind":"arxiv","id":"2007.09063","version":2},"attestation_state":"computed","paper":{"title":"Cosmic ray propagation in the Universe in presence of a random magnetic field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. D. Supanitsky","submitted_at":"2020-07-17T15:43:31Z","abstract_excerpt":"The origin of the ultrahigh energy cosmic ray remains being a mystery. However, a considerable progress has been made in the past few years due to the good quality data recorded by current cosmic ray observatories. One of the recent achievements is obtaining firm observational evidence about the extragalactic origin of the most energetic cosmic rays by the Pierre Auger observatory. On the other hand, it is believed that there is a non-null turbulent magnetic field that fills the intergalactic medium. Therefore, the presence of the intergalactic magnetic field can play an important role on 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":"2007.09063","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-07-17T15:43:31Z","cross_cats_sorted":[],"title_canon_sha256":"7169159b345992fb7344b3104b8050bb24db570da4a2664c9cf13cc8e71b392f","abstract_canon_sha256":"f5f3840b1d2be8ea10265c6be03b60014f25cd2d61484d834d00cb9df986dbd7"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:35:15.341870Z","signature_b64":"5ebyTOCgrz7rqwwwN3HZDbQH5AWkjBSerFLx/W92WOKhzz5FKIW3SKZx9bWkgouR4a4QsLUguIyeGAjeK8WyAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2be49d7b04e2f5e42b8155f1fc729d4447f1a3569effcfc38c76d11cbb27629b","last_reissued_at":"2026-07-05T02:35:15.341481Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:35:15.341481Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmic ray propagation in the Universe in presence of a random magnetic field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. D. Supanitsky","submitted_at":"2020-07-17T15:43:31Z","abstract_excerpt":"The origin of the ultrahigh energy cosmic ray remains being a mystery. However, a considerable progress has been made in the past few years due to the good quality data recorded by current cosmic ray observatories. One of the recent achievements is obtaining firm observational evidence about the extragalactic origin of the most energetic cosmic rays by the Pierre Auger observatory. On the other hand, it is believed that there is a non-null turbulent magnetic field that fills the intergalactic medium. Therefore, the presence of the intergalactic magnetic field can play an important role on the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2007.09063","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2007.09063/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":"2007.09063","created_at":"2026-07-05T02:35:15.341538+00:00"},{"alias_kind":"arxiv_version","alias_value":"2007.09063v2","created_at":"2026-07-05T02:35:15.341538+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2007.09063","created_at":"2026-07-05T02:35:15.341538+00:00"},{"alias_kind":"pith_short_12","alias_value":"FPSJ26YE4L26","created_at":"2026-07-05T02:35:15.341538+00:00"},{"alias_kind":"pith_short_16","alias_value":"FPSJ26YE4L26IK4B","created_at":"2026-07-05T02:35:15.341538+00:00"},{"alias_kind":"pith_short_8","alias_value":"FPSJ26YE","created_at":"2026-07-05T02:35:15.341538+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.17494","citing_title":"Analysing Ultra High Energy Cosmic Rays' Anisotropy in $\\boldsymbol{f(R, T)}$ Gravity Theory","ref_index":104,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FPSJ26YE4L26IK4BKXY7Y4U5IR","json":"https://pith.science/pith/FPSJ26YE4L26IK4BKXY7Y4U5IR.json","graph_json":"https://pith.science/api/pith-number/FPSJ26YE4L26IK4BKXY7Y4U5IR/graph.json","events_json":"https://pith.science/api/pith-number/FPSJ26YE4L26IK4BKXY7Y4U5IR/events.json","paper":"https://pith.science/paper/FPSJ26YE"},"agent_actions":{"view_html":"https://pith.science/pith/FPSJ26YE4L26IK4BKXY7Y4U5IR","download_json":"https://pith.science/pith/FPSJ26YE4L26IK4BKXY7Y4U5IR.json","view_paper":"https://pith.science/paper/FPSJ26YE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2007.09063&json=true","fetch_graph":"https://pith.science/api/pith-number/FPSJ26YE4L26IK4BKXY7Y4U5IR/graph.json","fetch_events":"https://pith.science/api/pith-number/FPSJ26YE4L26IK4BKXY7Y4U5IR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FPSJ26YE4L26IK4BKXY7Y4U5IR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FPSJ26YE4L26IK4BKXY7Y4U5IR/action/storage_attestation","attest_author":"https://pith.science/pith/FPSJ26YE4L26IK4BKXY7Y4U5IR/action/author_attestation","sign_citation":"https://pith.science/pith/FPSJ26YE4L26IK4BKXY7Y4U5IR/action/citation_signature","submit_replication":"https://pith.science/pith/FPSJ26YE4L26IK4BKXY7Y4U5IR/action/replication_record"}},"created_at":"2026-07-05T02:35:15.341538+00:00","updated_at":"2026-07-05T02:35:15.341538+00:00"}