{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:V6BTZH3E6ZRTAMODL37ITFLNP5","short_pith_number":"pith:V6BTZH3E","schema_version":"1.0","canonical_sha256":"af833c9f64f6633031c35efe89956d7f4ee7891abea9d8e35ea6bfb4cf76edc5","source":{"kind":"arxiv","id":"2102.03476","version":2},"attestation_state":"computed","paper":{"title":"Fermion propagator in a rotating environment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th","nucl-th"],"primary_cat":"hep-ph","authors_text":"Alejandro Ayala, K. Raya, L. A. Hern\\'andez, R. Zamora","submitted_at":"2021-02-06T02:16:28Z","abstract_excerpt":"We apply the exponential operator method to derive the propagator for a fermion immersed within a rigidly rotating environment with cylindrical geometry. Given that the rotation axis provides a preferred direction, Lorentz symmetry is lost and the general solution is not translationally invariant in the radial coordinate. However, under the approximation that the fermion is completely dragged by the vortical motion, valid for large angular velocities, translation invariance is recovered. The propagator can then be written in momentum space. The result is suited to be used applying ordinary Fey"},"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":"2102.03476","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2021-02-06T02:16:28Z","cross_cats_sorted":["hep-th","nucl-th"],"title_canon_sha256":"acb72db0dc1574571091ff508cdc77f9e376586a0097f6698c0194cdd8ae6f7e","abstract_canon_sha256":"a9d34b0d5e977a26cabce36f49589804de8d6a65a0a3a725200c8a4405b39d44"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:37:35.747577Z","signature_b64":"MXvjZkNDeK82EPioRBe2DlOZMX3xb/3vJAeSD6c6vp7RRh8hghCd99xg4vx8iMhTOz/OqQarVwPmZtMwW5EnAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"af833c9f64f6633031c35efe89956d7f4ee7891abea9d8e35ea6bfb4cf76edc5","last_reissued_at":"2026-07-05T02:37:35.747040Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:37:35.747040Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Fermion propagator in a rotating environment","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th","nucl-th"],"primary_cat":"hep-ph","authors_text":"Alejandro Ayala, K. Raya, L. A. Hern\\'andez, R. Zamora","submitted_at":"2021-02-06T02:16:28Z","abstract_excerpt":"We apply the exponential operator method to derive the propagator for a fermion immersed within a rigidly rotating environment with cylindrical geometry. Given that the rotation axis provides a preferred direction, Lorentz symmetry is lost and the general solution is not translationally invariant in the radial coordinate. However, under the approximation that the fermion is completely dragged by the vortical motion, valid for large angular velocities, translation invariance is recovered. The propagator can then be written in momentum space. The result is suited to be used applying ordinary Fey"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2102.03476","kind":"arxiv","version":2},"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/2102.03476/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":"2102.03476","created_at":"2026-07-05T02:37:35.747098+00:00"},{"alias_kind":"arxiv_version","alias_value":"2102.03476v2","created_at":"2026-07-05T02:37:35.747098+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2102.03476","created_at":"2026-07-05T02:37:35.747098+00:00"},{"alias_kind":"pith_short_12","alias_value":"V6BTZH3E6ZRT","created_at":"2026-07-05T02:37:35.747098+00:00"},{"alias_kind":"pith_short_16","alias_value":"V6BTZH3E6ZRTAMOD","created_at":"2026-07-05T02:37:35.747098+00:00"},{"alias_kind":"pith_short_8","alias_value":"V6BTZH3E","created_at":"2026-07-05T02:37:35.747098+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.07501","citing_title":"Excitation function for global \\Lambda polarization in relativistic heavy ion collisions with the Core Corona model","ref_index":51,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/V6BTZH3E6ZRTAMODL37ITFLNP5","json":"https://pith.science/pith/V6BTZH3E6ZRTAMODL37ITFLNP5.json","graph_json":"https://pith.science/api/pith-number/V6BTZH3E6ZRTAMODL37ITFLNP5/graph.json","events_json":"https://pith.science/api/pith-number/V6BTZH3E6ZRTAMODL37ITFLNP5/events.json","paper":"https://pith.science/paper/V6BTZH3E"},"agent_actions":{"view_html":"https://pith.science/pith/V6BTZH3E6ZRTAMODL37ITFLNP5","download_json":"https://pith.science/pith/V6BTZH3E6ZRTAMODL37ITFLNP5.json","view_paper":"https://pith.science/paper/V6BTZH3E","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2102.03476&json=true","fetch_graph":"https://pith.science/api/pith-number/V6BTZH3E6ZRTAMODL37ITFLNP5/graph.json","fetch_events":"https://pith.science/api/pith-number/V6BTZH3E6ZRTAMODL37ITFLNP5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/V6BTZH3E6ZRTAMODL37ITFLNP5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/V6BTZH3E6ZRTAMODL37ITFLNP5/action/storage_attestation","attest_author":"https://pith.science/pith/V6BTZH3E6ZRTAMODL37ITFLNP5/action/author_attestation","sign_citation":"https://pith.science/pith/V6BTZH3E6ZRTAMODL37ITFLNP5/action/citation_signature","submit_replication":"https://pith.science/pith/V6BTZH3E6ZRTAMODL37ITFLNP5/action/replication_record"}},"created_at":"2026-07-05T02:37:35.747098+00:00","updated_at":"2026-07-05T02:37:35.747098+00:00"}