{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:UYSLVMFAZP7Y4UPUVQYVVBUEUR","short_pith_number":"pith:UYSLVMFA","schema_version":"1.0","canonical_sha256":"a624bab0a0cbff8e51f4ac315a8684a467153c27d020164aa7173094b066d5a2","source":{"kind":"arxiv","id":"2502.00927","version":1},"attestation_state":"computed","paper":{"title":"Modeling Cosmic Rays at AGN Jet-Driven Shock Fronts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Greg L. Bryan, Kung-Yi Su, Philip F. Hopkins, Priyamvada Natarajan, Razieh Emami, Sam B. Ponnada, Yue Samuel Lu","submitted_at":"2025-02-02T21:30:34Z","abstract_excerpt":"Active Galactic Nuclei (AGN) feedback is a key physical mechanism proposed to regulate star formation, primarily in massive galaxies. In particular, cosmic rays associated with AGN jets have the potential to efficiently suppress cooling flows and quench star formation. The locus of cosmic ray production and their coupling to gas play a crucial role in the overall self-regulation process. To investigate this in detail, we conduct high-resolution, non-cosmological MHD simulations of a massive $10^{14} {\\rm M_\\odot}$ halo using the FIRE-2 (Feedback In Realistic Environments) stellar feedback mode"},"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":"2502.00927","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2025-02-02T21:30:34Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"9a8ada90bb3b9468860583d3e3f724d1d7fcd131caee9d51eee6ab5a41197eb0","abstract_canon_sha256":"6171236880d7ecd0595076830cec73fd02b1340c5cbcabcf54dc70d1ffd891a6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:08:40.260732Z","signature_b64":"42r+sgkXvWPoyzvES+XLKXUlIdE5B5Xa90m7/kEaOklLOCndnSDLeXWNC1fG4N8SpjdqSZMFmOMNr3NV/HVxCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a624bab0a0cbff8e51f4ac315a8684a467153c27d020164aa7173094b066d5a2","last_reissued_at":"2026-07-05T10:08:40.260255Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:08:40.260255Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Modeling Cosmic Rays at AGN Jet-Driven Shock Fronts","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"astro-ph.GA","authors_text":"Greg L. Bryan, Kung-Yi Su, Philip F. Hopkins, Priyamvada Natarajan, Razieh Emami, Sam B. Ponnada, Yue Samuel Lu","submitted_at":"2025-02-02T21:30:34Z","abstract_excerpt":"Active Galactic Nuclei (AGN) feedback is a key physical mechanism proposed to regulate star formation, primarily in massive galaxies. In particular, cosmic rays associated with AGN jets have the potential to efficiently suppress cooling flows and quench star formation. The locus of cosmic ray production and their coupling to gas play a crucial role in the overall self-regulation process. To investigate this in detail, we conduct high-resolution, non-cosmological MHD simulations of a massive $10^{14} {\\rm M_\\odot}$ halo using the FIRE-2 (Feedback In Realistic Environments) stellar feedback mode"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.00927","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/2502.00927/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":"2502.00927","created_at":"2026-07-05T10:08:40.260319+00:00"},{"alias_kind":"arxiv_version","alias_value":"2502.00927v1","created_at":"2026-07-05T10:08:40.260319+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.00927","created_at":"2026-07-05T10:08:40.260319+00:00"},{"alias_kind":"pith_short_12","alias_value":"UYSLVMFAZP7Y","created_at":"2026-07-05T10:08:40.260319+00:00"},{"alias_kind":"pith_short_16","alias_value":"UYSLVMFAZP7Y4UPU","created_at":"2026-07-05T10:08:40.260319+00:00"},{"alias_kind":"pith_short_8","alias_value":"UYSLVMFA","created_at":"2026-07-05T10:08:40.260319+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.04084","citing_title":"Simulating realistic radio morphologies of Fanaroff-Riley I jets in a self-regulating cool-core cluster","ref_index":298,"is_internal_anchor":false},{"citing_arxiv_id":"2509.07104","citing_title":"Cosmic Rays on Galaxy Scales: Progress and Pitfalls for CR-MHD Dynamical Models","ref_index":267,"is_internal_anchor":false},{"citing_arxiv_id":"2512.11062","citing_title":"Effects of Varied Cosmic Ray Feedback from AGN on Massive Galaxy Properties","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2605.08349","citing_title":"An Inverse-Compton-Boosted Cool Core Unifies Perseus's Radio and X-ray Halos","ref_index":270,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UYSLVMFAZP7Y4UPUVQYVVBUEUR","json":"https://pith.science/pith/UYSLVMFAZP7Y4UPUVQYVVBUEUR.json","graph_json":"https://pith.science/api/pith-number/UYSLVMFAZP7Y4UPUVQYVVBUEUR/graph.json","events_json":"https://pith.science/api/pith-number/UYSLVMFAZP7Y4UPUVQYVVBUEUR/events.json","paper":"https://pith.science/paper/UYSLVMFA"},"agent_actions":{"view_html":"https://pith.science/pith/UYSLVMFAZP7Y4UPUVQYVVBUEUR","download_json":"https://pith.science/pith/UYSLVMFAZP7Y4UPUVQYVVBUEUR.json","view_paper":"https://pith.science/paper/UYSLVMFA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2502.00927&json=true","fetch_graph":"https://pith.science/api/pith-number/UYSLVMFAZP7Y4UPUVQYVVBUEUR/graph.json","fetch_events":"https://pith.science/api/pith-number/UYSLVMFAZP7Y4UPUVQYVVBUEUR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UYSLVMFAZP7Y4UPUVQYVVBUEUR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UYSLVMFAZP7Y4UPUVQYVVBUEUR/action/storage_attestation","attest_author":"https://pith.science/pith/UYSLVMFAZP7Y4UPUVQYVVBUEUR/action/author_attestation","sign_citation":"https://pith.science/pith/UYSLVMFAZP7Y4UPUVQYVVBUEUR/action/citation_signature","submit_replication":"https://pith.science/pith/UYSLVMFAZP7Y4UPUVQYVVBUEUR/action/replication_record"}},"created_at":"2026-07-05T10:08:40.260319+00:00","updated_at":"2026-07-05T10:08:40.260319+00:00"}