{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:JCADVPCBZ6ERT2VLRH62TJQHX2","short_pith_number":"pith:JCADVPCB","schema_version":"1.0","canonical_sha256":"48803abc41cf8919eaab89fda9a607be9a456a27e697ef212b187e96e74c61af","source":{"kind":"arxiv","id":"1107.0968","version":1},"attestation_state":"computed","paper":{"title":"A non-ideal MHD Gadget: Simulating massive galaxy clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Bonafede, F. Stasyszyn, G. Murante, K. Dolag, S. Borgani","submitted_at":"2011-07-05T20:00:00Z","abstract_excerpt":"Magnetic fields in the intra-cluster medium of galaxy clusters have been studied in the past years through different methods. In the next years the up-coming generation of radio telescopes is going to provide new data that have the potential of setting constraints on the properties of magnetic fields in galaxy clusters. Here we present zoomed-in simulations for a set of massive galaxy clusters (M_v > 10^15 M_sun/h). This is an ideal sample to study the evolution of magnetic field during the process of structure formation in detail. Turbulent motions of the gas within the ICM will manifest them"},"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":"1107.0968","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2011-07-05T20:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"9113daa264baa6def7d373854dc22ebc17a6db10401ab4f3d89f8d5748f7d4f1","abstract_canon_sha256":"c05b5cddf6ee7dd99182604fe3577f1d91db656637f9f9f839efadfbaca41877"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:01:24.517389Z","signature_b64":"/7kgGlt0MWGs+THDSazcsoVJntOIuUdTIARAgSs3N3h+T/pP/0/Nn0JlLV9dAnIHAKD6sj6H9gOWoTE+IOQkDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"48803abc41cf8919eaab89fda9a607be9a456a27e697ef212b187e96e74c61af","last_reissued_at":"2026-05-18T02:01:24.516839Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:01:24.516839Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A non-ideal MHD Gadget: Simulating massive galaxy clusters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"A. Bonafede, F. Stasyszyn, G. Murante, K. Dolag, S. Borgani","submitted_at":"2011-07-05T20:00:00Z","abstract_excerpt":"Magnetic fields in the intra-cluster medium of galaxy clusters have been studied in the past years through different methods. In the next years the up-coming generation of radio telescopes is going to provide new data that have the potential of setting constraints on the properties of magnetic fields in galaxy clusters. Here we present zoomed-in simulations for a set of massive galaxy clusters (M_v > 10^15 M_sun/h). This is an ideal sample to study the evolution of magnetic field during the process of structure formation in detail. Turbulent motions of the gas within the ICM will manifest them"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1107.0968","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":"1107.0968","created_at":"2026-05-18T02:01:24.516917+00:00"},{"alias_kind":"arxiv_version","alias_value":"1107.0968v1","created_at":"2026-05-18T02:01:24.516917+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1107.0968","created_at":"2026-05-18T02:01:24.516917+00:00"},{"alias_kind":"pith_short_12","alias_value":"JCADVPCBZ6ER","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_16","alias_value":"JCADVPCBZ6ERT2VL","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_8","alias_value":"JCADVPCB","created_at":"2026-05-18T12:26:32.869790+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/JCADVPCBZ6ERT2VLRH62TJQHX2","json":"https://pith.science/pith/JCADVPCBZ6ERT2VLRH62TJQHX2.json","graph_json":"https://pith.science/api/pith-number/JCADVPCBZ6ERT2VLRH62TJQHX2/graph.json","events_json":"https://pith.science/api/pith-number/JCADVPCBZ6ERT2VLRH62TJQHX2/events.json","paper":"https://pith.science/paper/JCADVPCB"},"agent_actions":{"view_html":"https://pith.science/pith/JCADVPCBZ6ERT2VLRH62TJQHX2","download_json":"https://pith.science/pith/JCADVPCBZ6ERT2VLRH62TJQHX2.json","view_paper":"https://pith.science/paper/JCADVPCB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1107.0968&json=true","fetch_graph":"https://pith.science/api/pith-number/JCADVPCBZ6ERT2VLRH62TJQHX2/graph.json","fetch_events":"https://pith.science/api/pith-number/JCADVPCBZ6ERT2VLRH62TJQHX2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JCADVPCBZ6ERT2VLRH62TJQHX2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JCADVPCBZ6ERT2VLRH62TJQHX2/action/storage_attestation","attest_author":"https://pith.science/pith/JCADVPCBZ6ERT2VLRH62TJQHX2/action/author_attestation","sign_citation":"https://pith.science/pith/JCADVPCBZ6ERT2VLRH62TJQHX2/action/citation_signature","submit_replication":"https://pith.science/pith/JCADVPCBZ6ERT2VLRH62TJQHX2/action/replication_record"}},"created_at":"2026-05-18T02:01:24.516917+00:00","updated_at":"2026-05-18T02:01:24.516917+00:00"}