{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:OL6FSQASYSCNYHPPRPWKFFZSBU","short_pith_number":"pith:OL6FSQAS","schema_version":"1.0","canonical_sha256":"72fc594012c484dc1def8beca297320d279f41a2ce8313a8df34cdaace77549e","source":{"kind":"arxiv","id":"2403.16957","version":1},"attestation_state":"computed","paper":{"title":"Hydrodynamic fluctuations and topological susceptibility in chiral magnetohydrodynamics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph","nucl-th"],"primary_cat":"hep-th","authors_text":"Arpit Das, Nabil Iqbal, Napat Poovuttikul","submitted_at":"2024-03-25T17:17:38Z","abstract_excerpt":"Chiral magnetohydrodynamics is devoted to understanding the late-time and long-distance behavior of a system with an Adler-Bell-Jackiw anomaly at finite temperatures. The non-conservation of the axial charge is determined by the topological density $\\vec{E} \\cdot \\vec{B}$; in a classical hydrodynamic description this decay rate can be suppressed by tuning the background magnetic field to zero. However it is in principle possible for thermal fluctuations of $\\vec{E} \\cdot \\vec{B}$ to result in a non-conservation of the charge even at vanishing $B$-field; this would invalidate the classical hydr"},"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":"2403.16957","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2024-03-25T17:17:38Z","cross_cats_sorted":["astro-ph.HE","hep-ph","nucl-th"],"title_canon_sha256":"77ab9cad85ccf73499ed613860eb8d7bcffcb067807ca871baa13954359c87be","abstract_canon_sha256":"1590fc80bd227f3505fc5d16214813d95b960965ea3bd2fe7f523ed25b4ab129"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:54:48.577101Z","signature_b64":"/vFl4p4UxuOTBRZNlSERndCAbNPAVDs7mDeUnlg2PIZUGzQ/n2t3xB51GnfZ0ZrUkl8Ml+1Mh0JdYwnAgzXZAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"72fc594012c484dc1def8beca297320d279f41a2ce8313a8df34cdaace77549e","last_reissued_at":"2026-07-05T08:54:48.576591Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:54:48.576591Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hydrodynamic fluctuations and topological susceptibility in chiral magnetohydrodynamics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph","nucl-th"],"primary_cat":"hep-th","authors_text":"Arpit Das, Nabil Iqbal, Napat Poovuttikul","submitted_at":"2024-03-25T17:17:38Z","abstract_excerpt":"Chiral magnetohydrodynamics is devoted to understanding the late-time and long-distance behavior of a system with an Adler-Bell-Jackiw anomaly at finite temperatures. The non-conservation of the axial charge is determined by the topological density $\\vec{E} \\cdot \\vec{B}$; in a classical hydrodynamic description this decay rate can be suppressed by tuning the background magnetic field to zero. However it is in principle possible for thermal fluctuations of $\\vec{E} \\cdot \\vec{B}$ to result in a non-conservation of the charge even at vanishing $B$-field; this would invalidate the classical hydr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.16957","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/2403.16957/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":"2403.16957","created_at":"2026-07-05T08:54:48.576658+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.16957v1","created_at":"2026-07-05T08:54:48.576658+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.16957","created_at":"2026-07-05T08:54:48.576658+00:00"},{"alias_kind":"pith_short_12","alias_value":"OL6FSQASYSCN","created_at":"2026-07-05T08:54:48.576658+00:00"},{"alias_kind":"pith_short_16","alias_value":"OL6FSQASYSCNYHPP","created_at":"2026-07-05T08:54:48.576658+00:00"},{"alias_kind":"pith_short_8","alias_value":"OL6FSQAS","created_at":"2026-07-05T08:54:48.576658+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.02361","citing_title":"Chiral Anomalous Magnetohydrodynamics in action: effective field theory and holography","ref_index":13,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OL6FSQASYSCNYHPPRPWKFFZSBU","json":"https://pith.science/pith/OL6FSQASYSCNYHPPRPWKFFZSBU.json","graph_json":"https://pith.science/api/pith-number/OL6FSQASYSCNYHPPRPWKFFZSBU/graph.json","events_json":"https://pith.science/api/pith-number/OL6FSQASYSCNYHPPRPWKFFZSBU/events.json","paper":"https://pith.science/paper/OL6FSQAS"},"agent_actions":{"view_html":"https://pith.science/pith/OL6FSQASYSCNYHPPRPWKFFZSBU","download_json":"https://pith.science/pith/OL6FSQASYSCNYHPPRPWKFFZSBU.json","view_paper":"https://pith.science/paper/OL6FSQAS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.16957&json=true","fetch_graph":"https://pith.science/api/pith-number/OL6FSQASYSCNYHPPRPWKFFZSBU/graph.json","fetch_events":"https://pith.science/api/pith-number/OL6FSQASYSCNYHPPRPWKFFZSBU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OL6FSQASYSCNYHPPRPWKFFZSBU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OL6FSQASYSCNYHPPRPWKFFZSBU/action/storage_attestation","attest_author":"https://pith.science/pith/OL6FSQASYSCNYHPPRPWKFFZSBU/action/author_attestation","sign_citation":"https://pith.science/pith/OL6FSQASYSCNYHPPRPWKFFZSBU/action/citation_signature","submit_replication":"https://pith.science/pith/OL6FSQASYSCNYHPPRPWKFFZSBU/action/replication_record"}},"created_at":"2026-07-05T08:54:48.576658+00:00","updated_at":"2026-07-05T08:54:48.576658+00:00"}