{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:LMT3YJW3YYG25LPA5Z53EYI5WO","short_pith_number":"pith:LMT3YJW3","schema_version":"1.0","canonical_sha256":"5b27bc26dbc60daeade0ee7bb2611db38c338492beff2cf17dcf013b7ad5df47","source":{"kind":"arxiv","id":"1209.3276","version":5},"attestation_state":"computed","paper":{"title":"Bulk Properties of a Fermi Gas in a Magnetic Field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.SR","hep-ph"],"primary_cat":"nucl-th","authors_text":"Debora P. Menezes, Michael Strickland, Veronica Dexheimer","submitted_at":"2012-09-14T18:41:18Z","abstract_excerpt":"We calculate the number density, energy density, transverse pressure, longitudinal pressure, and magnetization of an ensemble of spin one-half particles in the presence of a homogenous background magnetic field. The magnetic field direction breaks spherical symmetry causing the pressure transverse to the magnetic field direction to be different than the pressure parallel to it. We present explicit formulae appropriate at zero and finite temperature for both charged and uncharged particles including the effect of the anomalous magnetic moment. We demonstrate that the resulting expressions satis"},"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":"1209.3276","kind":"arxiv","version":5},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2012-09-14T18:41:18Z","cross_cats_sorted":["astro-ph.HE","astro-ph.SR","hep-ph"],"title_canon_sha256":"d789db9de4cf28841cd0f8780e90ae79f8dfc58d227773625e2ea6be41675c71","abstract_canon_sha256":"110b2cf82af6073a15b55cf469751649d68189e63529ef93c8f2fcc7bed866e5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:25:04.201403Z","signature_b64":"YhnloPH1BjWwc/Iup4lj94WA0VrILYyTZTCTNyq1AXboHLRxLXNI32oiCVr99W/nBmCpRJSKGmOOWRTwRmXvCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5b27bc26dbc60daeade0ee7bb2611db38c338492beff2cf17dcf013b7ad5df47","last_reissued_at":"2026-05-18T03:25:04.200767Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:25:04.200767Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Bulk Properties of a Fermi Gas in a Magnetic Field","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.SR","hep-ph"],"primary_cat":"nucl-th","authors_text":"Debora P. Menezes, Michael Strickland, Veronica Dexheimer","submitted_at":"2012-09-14T18:41:18Z","abstract_excerpt":"We calculate the number density, energy density, transverse pressure, longitudinal pressure, and magnetization of an ensemble of spin one-half particles in the presence of a homogenous background magnetic field. The magnetic field direction breaks spherical symmetry causing the pressure transverse to the magnetic field direction to be different than the pressure parallel to it. We present explicit formulae appropriate at zero and finite temperature for both charged and uncharged particles including the effect of the anomalous magnetic moment. We demonstrate that the resulting expressions satis"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1209.3276","kind":"arxiv","version":5},"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":"1209.3276","created_at":"2026-05-18T03:25:04.200871+00:00"},{"alias_kind":"arxiv_version","alias_value":"1209.3276v5","created_at":"2026-05-18T03:25:04.200871+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1209.3276","created_at":"2026-05-18T03:25:04.200871+00:00"},{"alias_kind":"pith_short_12","alias_value":"LMT3YJW3YYG2","created_at":"2026-05-18T12:27:14.488303+00:00"},{"alias_kind":"pith_short_16","alias_value":"LMT3YJW3YYG25LPA","created_at":"2026-05-18T12:27:14.488303+00:00"},{"alias_kind":"pith_short_8","alias_value":"LMT3YJW3","created_at":"2026-05-18T12:27:14.488303+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"1907.03990","citing_title":"Effect of anomalous magnetic moment of quarks on the phase structure and mesonic properties in the NJL model","ref_index":60,"is_internal_anchor":true},{"citing_arxiv_id":"2507.14015","citing_title":"Anomalous-magnetic-moment-enhanced Casimir effect","ref_index":106,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LMT3YJW3YYG25LPA5Z53EYI5WO","json":"https://pith.science/pith/LMT3YJW3YYG25LPA5Z53EYI5WO.json","graph_json":"https://pith.science/api/pith-number/LMT3YJW3YYG25LPA5Z53EYI5WO/graph.json","events_json":"https://pith.science/api/pith-number/LMT3YJW3YYG25LPA5Z53EYI5WO/events.json","paper":"https://pith.science/paper/LMT3YJW3"},"agent_actions":{"view_html":"https://pith.science/pith/LMT3YJW3YYG25LPA5Z53EYI5WO","download_json":"https://pith.science/pith/LMT3YJW3YYG25LPA5Z53EYI5WO.json","view_paper":"https://pith.science/paper/LMT3YJW3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1209.3276&json=true","fetch_graph":"https://pith.science/api/pith-number/LMT3YJW3YYG25LPA5Z53EYI5WO/graph.json","fetch_events":"https://pith.science/api/pith-number/LMT3YJW3YYG25LPA5Z53EYI5WO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LMT3YJW3YYG25LPA5Z53EYI5WO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LMT3YJW3YYG25LPA5Z53EYI5WO/action/storage_attestation","attest_author":"https://pith.science/pith/LMT3YJW3YYG25LPA5Z53EYI5WO/action/author_attestation","sign_citation":"https://pith.science/pith/LMT3YJW3YYG25LPA5Z53EYI5WO/action/citation_signature","submit_replication":"https://pith.science/pith/LMT3YJW3YYG25LPA5Z53EYI5WO/action/replication_record"}},"created_at":"2026-05-18T03:25:04.200871+00:00","updated_at":"2026-05-18T03:25:04.200871+00:00"}