{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:QL4XUQGKIKOHDH3RFHFVQPBQM5","short_pith_number":"pith:QL4XUQGK","schema_version":"1.0","canonical_sha256":"82f97a40ca429c719f7129cb583c30675f5a40119106ddb246f18c4c4a8b5ac5","source":{"kind":"arxiv","id":"2011.01606","version":1},"attestation_state":"computed","paper":{"title":"Relativistic non-resistive viscous magnetohydrodynamics from the kinetic theory:a relaxation time approach","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","physics.flu-dyn","physics.plasm-ph"],"primary_cat":"nucl-th","authors_text":"Ankit Kumar Panda, Ashutosh Dash, Rajesh Biswas, Victor Roy","submitted_at":"2020-11-03T10:20:44Z","abstract_excerpt":"We derive the relativistic non-resistive, viscous second-order magnetohydrodynamic equations for the dissipative quantities using the relaxation time approximation. The Boltzmann equation is solved for a system of particles and antiparticles using Chapman-Enskog like gradient expansion of the single-particle distribution function truncated at second order. In the first order, the transport coefficients are independent of the magnetic field. In the second-order, new transport coefficients that couple magnetic field and the dissipative quantities appear which are different from those obtained in"},"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":"2011.01606","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2020-11-03T10:20:44Z","cross_cats_sorted":["hep-ph","physics.flu-dyn","physics.plasm-ph"],"title_canon_sha256":"3f6a42ddcd9d89e1ab4c75e25546975bbb8db21cadded792681e1b1e62a574a9","abstract_canon_sha256":"0fb965feb4b7a217788969f8e9ea3e6ac3c397a479a1a9193b7743cb0a24613a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:29:34.567384Z","signature_b64":"y7OlptnzacL99X0doZZFooralqrwyrZeZvN7R+1iu5N0+kFowTLC1rSugW1MQUEiLsR30oLuMrtVZvfU+rs9Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"82f97a40ca429c719f7129cb583c30675f5a40119106ddb246f18c4c4a8b5ac5","last_reissued_at":"2026-07-05T02:29:34.566927Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:29:34.566927Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Relativistic non-resistive viscous magnetohydrodynamics from the kinetic theory:a relaxation time approach","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","physics.flu-dyn","physics.plasm-ph"],"primary_cat":"nucl-th","authors_text":"Ankit Kumar Panda, Ashutosh Dash, Rajesh Biswas, Victor Roy","submitted_at":"2020-11-03T10:20:44Z","abstract_excerpt":"We derive the relativistic non-resistive, viscous second-order magnetohydrodynamic equations for the dissipative quantities using the relaxation time approximation. The Boltzmann equation is solved for a system of particles and antiparticles using Chapman-Enskog like gradient expansion of the single-particle distribution function truncated at second order. In the first order, the transport coefficients are independent of the magnetic field. In the second-order, new transport coefficients that couple magnetic field and the dissipative quantities appear which are different from those obtained in"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2011.01606","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/2011.01606/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":"2011.01606","created_at":"2026-07-05T02:29:34.566982+00:00"},{"alias_kind":"arxiv_version","alias_value":"2011.01606v1","created_at":"2026-07-05T02:29:34.566982+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2011.01606","created_at":"2026-07-05T02:29:34.566982+00:00"},{"alias_kind":"pith_short_12","alias_value":"QL4XUQGKIKOH","created_at":"2026-07-05T02:29:34.566982+00:00"},{"alias_kind":"pith_short_16","alias_value":"QL4XUQGKIKOHDH3R","created_at":"2026-07-05T02:29:34.566982+00:00"},{"alias_kind":"pith_short_8","alias_value":"QL4XUQGK","created_at":"2026-07-05T02:29:34.566982+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2508.17543","citing_title":"Validity of relativistic hydrodynamics beyond local equilibrium","ref_index":46,"is_internal_anchor":false},{"citing_arxiv_id":"2605.01807","citing_title":"Relativistic BDNK MHD Evolution in a Boost-Invariant Medium and Its Impact on Dilepton Production","ref_index":64,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QL4XUQGKIKOHDH3RFHFVQPBQM5","json":"https://pith.science/pith/QL4XUQGKIKOHDH3RFHFVQPBQM5.json","graph_json":"https://pith.science/api/pith-number/QL4XUQGKIKOHDH3RFHFVQPBQM5/graph.json","events_json":"https://pith.science/api/pith-number/QL4XUQGKIKOHDH3RFHFVQPBQM5/events.json","paper":"https://pith.science/paper/QL4XUQGK"},"agent_actions":{"view_html":"https://pith.science/pith/QL4XUQGKIKOHDH3RFHFVQPBQM5","download_json":"https://pith.science/pith/QL4XUQGKIKOHDH3RFHFVQPBQM5.json","view_paper":"https://pith.science/paper/QL4XUQGK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2011.01606&json=true","fetch_graph":"https://pith.science/api/pith-number/QL4XUQGKIKOHDH3RFHFVQPBQM5/graph.json","fetch_events":"https://pith.science/api/pith-number/QL4XUQGKIKOHDH3RFHFVQPBQM5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QL4XUQGKIKOHDH3RFHFVQPBQM5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QL4XUQGKIKOHDH3RFHFVQPBQM5/action/storage_attestation","attest_author":"https://pith.science/pith/QL4XUQGKIKOHDH3RFHFVQPBQM5/action/author_attestation","sign_citation":"https://pith.science/pith/QL4XUQGKIKOHDH3RFHFVQPBQM5/action/citation_signature","submit_replication":"https://pith.science/pith/QL4XUQGKIKOHDH3RFHFVQPBQM5/action/replication_record"}},"created_at":"2026-07-05T02:29:34.566982+00:00","updated_at":"2026-07-05T02:29:34.566982+00:00"}