{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:1996:4W2QH2VWXNPQG72YQILFDU4V2Z","short_pith_number":"pith:4W2QH2VW","canonical_record":{"source":{"id":"astro-ph/9610172","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1996-10-22T14:22:13Z","cross_cats_sorted":[],"title_canon_sha256":"178c511c7e22d3d63ae08918a28eecb7ace30b46945e585c2efe738620496dd2","abstract_canon_sha256":"356ea6e69077fcb61cedeec42776557d72366124ae52ffafdc25bddb95c36216"},"schema_version":"1.0"},"canonical_sha256":"e5b503eab6bb5f037f58821651d395d658f5eb3cf187c9283fc29b823e759d6e","source":{"kind":"arxiv","id":"astro-ph/9610172","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/9610172","created_at":"2026-05-18T04:21:40Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9610172v1","created_at":"2026-05-18T04:21:40Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9610172","created_at":"2026-05-18T04:21:40Z"},{"alias_kind":"pith_short_12","alias_value":"4W2QH2VWXNPQ","created_at":"2026-05-18T12:25:47Z"},{"alias_kind":"pith_short_16","alias_value":"4W2QH2VWXNPQG72Y","created_at":"2026-05-18T12:25:47Z"},{"alias_kind":"pith_short_8","alias_value":"4W2QH2VW","created_at":"2026-05-18T12:25:47Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:1996:4W2QH2VWXNPQG72YQILFDU4V2Z","target":"record","payload":{"canonical_record":{"source":{"id":"astro-ph/9610172","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"1996-10-22T14:22:13Z","cross_cats_sorted":[],"title_canon_sha256":"178c511c7e22d3d63ae08918a28eecb7ace30b46945e585c2efe738620496dd2","abstract_canon_sha256":"356ea6e69077fcb61cedeec42776557d72366124ae52ffafdc25bddb95c36216"},"schema_version":"1.0"},"canonical_sha256":"e5b503eab6bb5f037f58821651d395d658f5eb3cf187c9283fc29b823e759d6e","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:21:40.562137Z","signature_b64":"VyLWwBNd5Q0zKmjpnpD4Jbu3E0Jy3A1DAruX9RXwW9tpIm378l1pWmIL55bR7xE9sH9KeeYaoOnpVRONJiBsDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e5b503eab6bb5f037f58821651d395d658f5eb3cf187c9283fc29b823e759d6e","last_reissued_at":"2026-05-18T04:21:40.561383Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:21:40.561383Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"astro-ph/9610172","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T04:21:40Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"B6O1bTkLC/R3PkSiZuJMvFxCTBA3VHwTSqtLWSEqp1QJt/QZoE4ej+Bpw8JB5pcj0ADp8OUo5I8uXdN2wubNBw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-27T10:01:30.912636Z"},"content_sha256":"0ce5bea110b71442300ceac6946496d685aba6fa0f547fca2b5c97e4ebad5db0","schema_version":"1.0","event_id":"sha256:0ce5bea110b71442300ceac6946496d685aba6fa0f547fca2b5c97e4ebad5db0"},{"event_type":"graph_snapshot","subject_pith_number":"pith:1996:4W2QH2VWXNPQG72YQILFDU4V2Z","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Non-Diffusive Propagation of Ultra High Energy Cosmic Rays","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Elisabete M. de Gouveia Dal Pino, Gustavo A. Medina Tanco, Jorge E. Horvath","submitted_at":"1996-10-22T14:22:13Z","abstract_excerpt":"We report the results of 3-D simulations of non-diffusive propagation of Ultra-High Energy Cosmic Rays (UHECR) (E > 10^{20} eV) through the intergalactic and extended halo media. We quantify the expected angular and temporal correlations between the events and the sources, and the temporal delay between protons and gamma-ray counterparts with a common origin for both halo and extragalactic origins. It is shown that the proposed UHECR-supergalactic plane source associations require either extremely high values of the halo magnetic field over as much as 100 kpc length scale or a very large corre"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9610172","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T04:21:40Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"OZ59tz3wtC4HQJZl0Oj8CXhZKBFQhwzHWCrNuKaxoSrNHw1l2pk2yZ7UvmPtA6ZPaUYRx++nK0bXSdJlyeU+Bw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-27T10:01:30.912981Z"},"content_sha256":"f0b8c264ca17c6a493fecee8353e40259ac4e1046bf3feba2fa7e217de49d24c","schema_version":"1.0","event_id":"sha256:f0b8c264ca17c6a493fecee8353e40259ac4e1046bf3feba2fa7e217de49d24c"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/4W2QH2VWXNPQG72YQILFDU4V2Z/bundle.json","state_url":"https://pith.science/pith/4W2QH2VWXNPQG72YQILFDU4V2Z/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/4W2QH2VWXNPQG72YQILFDU4V2Z/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-06-27T10:01:30Z","links":{"resolver":"https://pith.science/pith/4W2QH2VWXNPQG72YQILFDU4V2Z","bundle":"https://pith.science/pith/4W2QH2VWXNPQG72YQILFDU4V2Z/bundle.json","state":"https://pith.science/pith/4W2QH2VWXNPQG72YQILFDU4V2Z/state.json","well_known_bundle":"https://pith.science/.well-known/pith/4W2QH2VWXNPQG72YQILFDU4V2Z/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:1996:4W2QH2VWXNPQG72YQILFDU4V2Z","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"356ea6e69077fcb61cedeec42776557d72366124ae52ffafdc25bddb95c36216","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"1996-10-22T14:22:13Z","title_canon_sha256":"178c511c7e22d3d63ae08918a28eecb7ace30b46945e585c2efe738620496dd2"},"schema_version":"1.0","source":{"id":"astro-ph/9610172","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/9610172","created_at":"2026-05-18T04:21:40Z"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/9610172v1","created_at":"2026-05-18T04:21:40Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/9610172","created_at":"2026-05-18T04:21:40Z"},{"alias_kind":"pith_short_12","alias_value":"4W2QH2VWXNPQ","created_at":"2026-05-18T12:25:47Z"},{"alias_kind":"pith_short_16","alias_value":"4W2QH2VWXNPQG72Y","created_at":"2026-05-18T12:25:47Z"},{"alias_kind":"pith_short_8","alias_value":"4W2QH2VW","created_at":"2026-05-18T12:25:47Z"}],"graph_snapshots":[{"event_id":"sha256:f0b8c264ca17c6a493fecee8353e40259ac4e1046bf3feba2fa7e217de49d24c","target":"graph","created_at":"2026-05-18T04:21:40Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"We report the results of 3-D simulations of non-diffusive propagation of Ultra-High Energy Cosmic Rays (UHECR) (E > 10^{20} eV) through the intergalactic and extended halo media. We quantify the expected angular and temporal correlations between the events and the sources, and the temporal delay between protons and gamma-ray counterparts with a common origin for both halo and extragalactic origins. It is shown that the proposed UHECR-supergalactic plane source associations require either extremely high values of the halo magnetic field over as much as 100 kpc length scale or a very large corre","authors_text":"Elisabete M. de Gouveia Dal Pino, Gustavo A. Medina Tanco, Jorge E. Horvath","cross_cats":[],"headline":"","license":"","primary_cat":"astro-ph","submitted_at":"1996-10-22T14:22:13Z","title":"Non-Diffusive Propagation of Ultra High Energy Cosmic Rays"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/9610172","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:0ce5bea110b71442300ceac6946496d685aba6fa0f547fca2b5c97e4ebad5db0","target":"record","created_at":"2026-05-18T04:21:40Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"356ea6e69077fcb61cedeec42776557d72366124ae52ffafdc25bddb95c36216","cross_cats_sorted":[],"license":"","primary_cat":"astro-ph","submitted_at":"1996-10-22T14:22:13Z","title_canon_sha256":"178c511c7e22d3d63ae08918a28eecb7ace30b46945e585c2efe738620496dd2"},"schema_version":"1.0","source":{"id":"astro-ph/9610172","kind":"arxiv","version":1}},"canonical_sha256":"e5b503eab6bb5f037f58821651d395d658f5eb3cf187c9283fc29b823e759d6e","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"e5b503eab6bb5f037f58821651d395d658f5eb3cf187c9283fc29b823e759d6e","first_computed_at":"2026-05-18T04:21:40.561383Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T04:21:40.561383Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"VyLWwBNd5Q0zKmjpnpD4Jbu3E0Jy3A1DAruX9RXwW9tpIm378l1pWmIL55bR7xE9sH9KeeYaoOnpVRONJiBsDw==","signature_status":"signed_v1","signed_at":"2026-05-18T04:21:40.562137Z","signed_message":"canonical_sha256_bytes"},"source_id":"astro-ph/9610172","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:0ce5bea110b71442300ceac6946496d685aba6fa0f547fca2b5c97e4ebad5db0","sha256:f0b8c264ca17c6a493fecee8353e40259ac4e1046bf3feba2fa7e217de49d24c"],"state_sha256":"bc8aff543a67e940b2543a232b6a313b04c8659b22631dfd1324795c7443bfb7"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"9wgq/quMUoKlzEijaGXikh/uY7q3Hneb1j0ZZUQ3AHJRYy0tMb+AZED0fMUucrztxowOulUXRNACaMYjZbHqAg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-27T10:01:30.914905Z","bundle_sha256":"068bc778e4287849b39345448a0cc0001d2fb1b0f736499d892f1751e423c10a"}}