{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:BV74XPIQKNTQRRHSJUVYDSGNYT","short_pith_number":"pith:BV74XPIQ","schema_version":"1.0","canonical_sha256":"0d7fcbbd10536708c4f24d2b81c8cdc4cabf6ae8307d4393a9e44625ca792764","source":{"kind":"arxiv","id":"1801.02160","version":2},"attestation_state":"computed","paper":{"title":"On the Efficiency of Thermal Conduction in Galaxy Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Fulai Guo, Guobin Mou, Xiang-Er Fang, Ye-Fei Yuan","submitted_at":"2018-01-07T09:07:43Z","abstract_excerpt":"Galaxy clusters host a large reservoir of diffuse plasma with radially-varying temperature profiles. The efficiency of thermal conduction in the intracluster medium (ICM) is complicated by the existence of turbulence and magnetic fields, and has received a lot of attention in the literature. Previous studies suggest that the magnetothermal instability developed in outer regions of galaxy clusters would drive magnetic field lines preferentially radial, resulting in efficient conduction along the radial direction. Using a series of spherically-symmetric simulations, here we investigate the impac"},"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":"1801.02160","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-01-07T09:07:43Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"36ff068d53cefb885246d8648d3721cabd018a1ffce0aca60757dd42f1700088","abstract_canon_sha256":"2c5a34a0fbdaf291a8128e83913d7e459cb9b05f069cb0779388916354f32413"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:07:11.054493Z","signature_b64":"8Owi7C5WJ5JjyujaRgzSnTVzExRU0gsnO4uAK0pCxT3jEfiHw5WkLx74X1GwH4wVyCl6wH0DJrFl96FaWDucAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0d7fcbbd10536708c4f24d2b81c8cdc4cabf6ae8307d4393a9e44625ca792764","last_reissued_at":"2026-05-18T00:07:11.053850Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:07:11.053850Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the Efficiency of Thermal Conduction in Galaxy Clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"astro-ph.HE","authors_text":"Fulai Guo, Guobin Mou, Xiang-Er Fang, Ye-Fei Yuan","submitted_at":"2018-01-07T09:07:43Z","abstract_excerpt":"Galaxy clusters host a large reservoir of diffuse plasma with radially-varying temperature profiles. The efficiency of thermal conduction in the intracluster medium (ICM) is complicated by the existence of turbulence and magnetic fields, and has received a lot of attention in the literature. Previous studies suggest that the magnetothermal instability developed in outer regions of galaxy clusters would drive magnetic field lines preferentially radial, resulting in efficient conduction along the radial direction. Using a series of spherically-symmetric simulations, here we investigate the impac"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1801.02160","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":""},"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":"1801.02160","created_at":"2026-05-18T00:07:11.053956+00:00"},{"alias_kind":"arxiv_version","alias_value":"1801.02160v2","created_at":"2026-05-18T00:07:11.053956+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1801.02160","created_at":"2026-05-18T00:07:11.053956+00:00"},{"alias_kind":"pith_short_12","alias_value":"BV74XPIQKNTQ","created_at":"2026-05-18T12:32:16.446611+00:00"},{"alias_kind":"pith_short_16","alias_value":"BV74XPIQKNTQRRHS","created_at":"2026-05-18T12:32:16.446611+00:00"},{"alias_kind":"pith_short_8","alias_value":"BV74XPIQ","created_at":"2026-05-18T12:32:16.446611+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/BV74XPIQKNTQRRHSJUVYDSGNYT","json":"https://pith.science/pith/BV74XPIQKNTQRRHSJUVYDSGNYT.json","graph_json":"https://pith.science/api/pith-number/BV74XPIQKNTQRRHSJUVYDSGNYT/graph.json","events_json":"https://pith.science/api/pith-number/BV74XPIQKNTQRRHSJUVYDSGNYT/events.json","paper":"https://pith.science/paper/BV74XPIQ"},"agent_actions":{"view_html":"https://pith.science/pith/BV74XPIQKNTQRRHSJUVYDSGNYT","download_json":"https://pith.science/pith/BV74XPIQKNTQRRHSJUVYDSGNYT.json","view_paper":"https://pith.science/paper/BV74XPIQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1801.02160&json=true","fetch_graph":"https://pith.science/api/pith-number/BV74XPIQKNTQRRHSJUVYDSGNYT/graph.json","fetch_events":"https://pith.science/api/pith-number/BV74XPIQKNTQRRHSJUVYDSGNYT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BV74XPIQKNTQRRHSJUVYDSGNYT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BV74XPIQKNTQRRHSJUVYDSGNYT/action/storage_attestation","attest_author":"https://pith.science/pith/BV74XPIQKNTQRRHSJUVYDSGNYT/action/author_attestation","sign_citation":"https://pith.science/pith/BV74XPIQKNTQRRHSJUVYDSGNYT/action/citation_signature","submit_replication":"https://pith.science/pith/BV74XPIQKNTQRRHSJUVYDSGNYT/action/replication_record"}},"created_at":"2026-05-18T00:07:11.053956+00:00","updated_at":"2026-05-18T00:07:11.053956+00:00"}