{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:KWRRW7ZGSCTKJFSKK572YSUO53","short_pith_number":"pith:KWRRW7ZG","schema_version":"1.0","canonical_sha256":"55a31b7f2690a6a4964a577fac4a8eeecdd19aab0b7ab42d0239edbf90eadf23","source":{"kind":"arxiv","id":"1506.04893","version":1},"attestation_state":"computed","paper":{"title":"Diffusion of Cosmic Rays in a Multiphase Interstellar Medium Swept-Up by a Supernova Remnant Blast Wave","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Shu-ichiro Inutsuka, Soonyoung Roh, Tsuyoshi Inoue","submitted_at":"2015-06-16T09:50:14Z","abstract_excerpt":"Supernova remnants (SNRs) are one of the most energetic astrophysical events and are thought to be the dominant source of Galactic cosmic rays (CRs). A recent report on observations from the Fermi satellite has shown a signature of pion decay in the gamma-ray spectra of SNRs. This provides strong evidence that high-energy protons are accelerated in SNRs. The actual gamma-ray emission from pion decay should depend on the diffusion of CRs in the interstellar medium. In order to quantitatively analyse the diffusion of high-energy CRs from acceleration sites, we have performed test particle numeri"},"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":"1506.04893","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-06-16T09:50:14Z","cross_cats_sorted":[],"title_canon_sha256":"5e7bcb2495714cc578da2f2c415ef6f356993157274055001e6de5f078acff23","abstract_canon_sha256":"c1e184acaff39c4bf5dd1424864c2072ee4e882b1cbde45705b1e633e6b07137"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:34:48.001038Z","signature_b64":"LVL2ch7sM6BdrMlqZrkuJ3fjmepLDh7f2z4Z3NL1+KpFhGs6Z4BW3q4H9Qbn6dx90iRzgF3RkiIOP9H698q3Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"55a31b7f2690a6a4964a577fac4a8eeecdd19aab0b7ab42d0239edbf90eadf23","last_reissued_at":"2026-05-18T01:34:48.000558Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:34:48.000558Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Diffusion of Cosmic Rays in a Multiphase Interstellar Medium Swept-Up by a Supernova Remnant Blast Wave","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Shu-ichiro Inutsuka, Soonyoung Roh, Tsuyoshi Inoue","submitted_at":"2015-06-16T09:50:14Z","abstract_excerpt":"Supernova remnants (SNRs) are one of the most energetic astrophysical events and are thought to be the dominant source of Galactic cosmic rays (CRs). A recent report on observations from the Fermi satellite has shown a signature of pion decay in the gamma-ray spectra of SNRs. This provides strong evidence that high-energy protons are accelerated in SNRs. The actual gamma-ray emission from pion decay should depend on the diffusion of CRs in the interstellar medium. In order to quantitatively analyse the diffusion of high-energy CRs from acceleration sites, we have performed test particle numeri"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1506.04893","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":"1506.04893","created_at":"2026-05-18T01:34:48.000633+00:00"},{"alias_kind":"arxiv_version","alias_value":"1506.04893v1","created_at":"2026-05-18T01:34:48.000633+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1506.04893","created_at":"2026-05-18T01:34:48.000633+00:00"},{"alias_kind":"pith_short_12","alias_value":"KWRRW7ZGSCTK","created_at":"2026-05-18T12:29:29.992203+00:00"},{"alias_kind":"pith_short_16","alias_value":"KWRRW7ZGSCTKJFSK","created_at":"2026-05-18T12:29:29.992203+00:00"},{"alias_kind":"pith_short_8","alias_value":"KWRRW7ZG","created_at":"2026-05-18T12:29:29.992203+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/KWRRW7ZGSCTKJFSKK572YSUO53","json":"https://pith.science/pith/KWRRW7ZGSCTKJFSKK572YSUO53.json","graph_json":"https://pith.science/api/pith-number/KWRRW7ZGSCTKJFSKK572YSUO53/graph.json","events_json":"https://pith.science/api/pith-number/KWRRW7ZGSCTKJFSKK572YSUO53/events.json","paper":"https://pith.science/paper/KWRRW7ZG"},"agent_actions":{"view_html":"https://pith.science/pith/KWRRW7ZGSCTKJFSKK572YSUO53","download_json":"https://pith.science/pith/KWRRW7ZGSCTKJFSKK572YSUO53.json","view_paper":"https://pith.science/paper/KWRRW7ZG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1506.04893&json=true","fetch_graph":"https://pith.science/api/pith-number/KWRRW7ZGSCTKJFSKK572YSUO53/graph.json","fetch_events":"https://pith.science/api/pith-number/KWRRW7ZGSCTKJFSKK572YSUO53/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KWRRW7ZGSCTKJFSKK572YSUO53/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KWRRW7ZGSCTKJFSKK572YSUO53/action/storage_attestation","attest_author":"https://pith.science/pith/KWRRW7ZGSCTKJFSKK572YSUO53/action/author_attestation","sign_citation":"https://pith.science/pith/KWRRW7ZGSCTKJFSKK572YSUO53/action/citation_signature","submit_replication":"https://pith.science/pith/KWRRW7ZGSCTKJFSKK572YSUO53/action/replication_record"}},"created_at":"2026-05-18T01:34:48.000633+00:00","updated_at":"2026-05-18T01:34:48.000633+00:00"}