{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1996:BN2ZSR77Y2XOFTTEQ6M44IOHRH","short_pith_number":"pith:BN2ZSR77","schema_version":"1.0","canonical_sha256":"0b759947ffc6aee2ce648799ce21c789dbb68af99e02234e9bf17708d6bf63fa","source":{"kind":"arxiv","id":"hep-ph/9608271","version":1},"attestation_state":"computed","paper":{"title":"Hard thermal loops in a magnetic field and the chiral anomaly","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Per Elmfors","submitted_at":"1996-08-08T16:50:56Z","abstract_excerpt":"The fermionic dispersion relation in the presence of a background magnetic field and a high temperature QED plasma is calculated exactly in the external field, using the Hard Thermal Loop effective action. As the field strength increases there is a smooth transition from the weak-field ($qB\\ll q^2T^2$) thermal dispersion relations to the vacuum Landau levels when the background field is much stronger than any thermal effects ($qB\\gg q^2T^2$). The self-energy at finite field strength acquires an imaginary part. The spectral width becomes important for critical field strengths ($qB \\sim q^2T^2$)"},"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":"hep-ph/9608271","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"1996-08-08T16:50:56Z","cross_cats_sorted":[],"title_canon_sha256":"42944ac967a44bb73438921b9140dcce22661472d1bb853a29fee643996e5c68","abstract_canon_sha256":"ae722da7317f3bb2e0a980f9ec049b5690b33d6477f8d6329a7e7af84e97c6c3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:01:39.166274Z","signature_b64":"ESW2aO007GWlNP7o7SIO81o3kJfUJ21rJlLHC5RYhRfW9rx0gDcVuKE1GmzIaL+xx6acv+fakSgg0Xg+RrFOAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0b759947ffc6aee2ce648799ce21c789dbb68af99e02234e9bf17708d6bf63fa","last_reissued_at":"2026-07-04T16:01:39.165911Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:01:39.165911Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Hard thermal loops in a magnetic field and the chiral anomaly","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Per Elmfors","submitted_at":"1996-08-08T16:50:56Z","abstract_excerpt":"The fermionic dispersion relation in the presence of a background magnetic field and a high temperature QED plasma is calculated exactly in the external field, using the Hard Thermal Loop effective action. As the field strength increases there is a smooth transition from the weak-field ($qB\\ll q^2T^2$) thermal dispersion relations to the vacuum Landau levels when the background field is much stronger than any thermal effects ($qB\\gg q^2T^2$). The self-energy at finite field strength acquires an imaginary part. The spectral width becomes important for critical field strengths ($qB \\sim q^2T^2$)"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9608271","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/hep-ph/9608271/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":"hep-ph/9608271","created_at":"2026-07-04T16:01:39.165976+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/9608271v1","created_at":"2026-07-04T16:01:39.165976+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/9608271","created_at":"2026-07-04T16:01:39.165976+00:00"},{"alias_kind":"pith_short_12","alias_value":"BN2ZSR77Y2XO","created_at":"2026-07-04T16:01:39.165976+00:00"},{"alias_kind":"pith_short_16","alias_value":"BN2ZSR77Y2XOFTTE","created_at":"2026-07-04T16:01:39.165976+00:00"},{"alias_kind":"pith_short_8","alias_value":"BN2ZSR77","created_at":"2026-07-04T16:01:39.165976+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.17090","citing_title":"Non-extensive Hard Thermal Loop Resummation and Its Applications: Analysis in Zero and Finite Magnetic Fields","ref_index":11,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BN2ZSR77Y2XOFTTEQ6M44IOHRH","json":"https://pith.science/pith/BN2ZSR77Y2XOFTTEQ6M44IOHRH.json","graph_json":"https://pith.science/api/pith-number/BN2ZSR77Y2XOFTTEQ6M44IOHRH/graph.json","events_json":"https://pith.science/api/pith-number/BN2ZSR77Y2XOFTTEQ6M44IOHRH/events.json","paper":"https://pith.science/paper/BN2ZSR77"},"agent_actions":{"view_html":"https://pith.science/pith/BN2ZSR77Y2XOFTTEQ6M44IOHRH","download_json":"https://pith.science/pith/BN2ZSR77Y2XOFTTEQ6M44IOHRH.json","view_paper":"https://pith.science/paper/BN2ZSR77","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/9608271&json=true","fetch_graph":"https://pith.science/api/pith-number/BN2ZSR77Y2XOFTTEQ6M44IOHRH/graph.json","fetch_events":"https://pith.science/api/pith-number/BN2ZSR77Y2XOFTTEQ6M44IOHRH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BN2ZSR77Y2XOFTTEQ6M44IOHRH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BN2ZSR77Y2XOFTTEQ6M44IOHRH/action/storage_attestation","attest_author":"https://pith.science/pith/BN2ZSR77Y2XOFTTEQ6M44IOHRH/action/author_attestation","sign_citation":"https://pith.science/pith/BN2ZSR77Y2XOFTTEQ6M44IOHRH/action/citation_signature","submit_replication":"https://pith.science/pith/BN2ZSR77Y2XOFTTEQ6M44IOHRH/action/replication_record"}},"created_at":"2026-07-04T16:01:39.165976+00:00","updated_at":"2026-07-04T16:01:39.165976+00:00"}