{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:2YBGBIJX4KJYPFAWRLBHZX4QDA","short_pith_number":"pith:2YBGBIJX","schema_version":"1.0","canonical_sha256":"d60260a137e2938794168ac27cdf90182065ff85b58f7a96ffe3289954d54d50","source":{"kind":"arxiv","id":"2506.02111","version":1},"attestation_state":"computed","paper":{"title":"The particle spectra of parity-violating theories: A less radical approach and an upgrade of PSALTer","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Georgios K. Karananas, Haochen Tu, Will Barker","submitted_at":"2025-06-02T18:00:03Z","abstract_excerpt":"Due to computational barriers, the effects of parity violation have so far been grossly neglected in gravitational model-building, leading to a serious gap in the space of prior models. We present a new algorithm for efficiently computing the particle spectrum for any parity-violating tensorial field theory. It allows to extract conditions for the absence of massive ghosts without resorting to any manipulation of radicals in cases where the particle masses are irrational functions of the Lagrangian coupling coefficients. We test it against several examples, among which is the most general pari"},"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":"2506.02111","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2025-06-02T18:00:03Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"56290c5431c1bd2939d3f847915d26814217ad7e8c57c2e36333d938d46a847c","abstract_canon_sha256":"5bcbbd4c443f7d891881b7d3653acf002c035e3f8e118688771811ffcbac3c55"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:14:32.722648Z","signature_b64":"vYyecIK/Ax40rZPDmbFr5yevJN/57I9KB14NO1ZaXXO5UDybSDH4abE1iEZXEnqF7g5zdTso7GXJI27d1D9EAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d60260a137e2938794168ac27cdf90182065ff85b58f7a96ffe3289954d54d50","last_reissued_at":"2026-07-05T11:14:32.722166Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:14:32.722166Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The particle spectra of parity-violating theories: A less radical approach and an upgrade of PSALTer","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Georgios K. Karananas, Haochen Tu, Will Barker","submitted_at":"2025-06-02T18:00:03Z","abstract_excerpt":"Due to computational barriers, the effects of parity violation have so far been grossly neglected in gravitational model-building, leading to a serious gap in the space of prior models. We present a new algorithm for efficiently computing the particle spectrum for any parity-violating tensorial field theory. It allows to extract conditions for the absence of massive ghosts without resorting to any manipulation of radicals in cases where the particle masses are irrational functions of the Lagrangian coupling coefficients. We test it against several examples, among which is the most general pari"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.02111","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/2506.02111/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":"2506.02111","created_at":"2026-07-05T11:14:32.722225+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.02111v1","created_at":"2026-07-05T11:14:32.722225+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.02111","created_at":"2026-07-05T11:14:32.722225+00:00"},{"alias_kind":"pith_short_12","alias_value":"2YBGBIJX4KJY","created_at":"2026-07-05T11:14:32.722225+00:00"},{"alias_kind":"pith_short_16","alias_value":"2YBGBIJX4KJYPFAW","created_at":"2026-07-05T11:14:32.722225+00:00"},{"alias_kind":"pith_short_8","alias_value":"2YBGBIJX","created_at":"2026-07-05T11:14:32.722225+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.30785","citing_title":"Numerical polology: towards next-generation model-building for cosmology","ref_index":68,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/2YBGBIJX4KJYPFAWRLBHZX4QDA","json":"https://pith.science/pith/2YBGBIJX4KJYPFAWRLBHZX4QDA.json","graph_json":"https://pith.science/api/pith-number/2YBGBIJX4KJYPFAWRLBHZX4QDA/graph.json","events_json":"https://pith.science/api/pith-number/2YBGBIJX4KJYPFAWRLBHZX4QDA/events.json","paper":"https://pith.science/paper/2YBGBIJX"},"agent_actions":{"view_html":"https://pith.science/pith/2YBGBIJX4KJYPFAWRLBHZX4QDA","download_json":"https://pith.science/pith/2YBGBIJX4KJYPFAWRLBHZX4QDA.json","view_paper":"https://pith.science/paper/2YBGBIJX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.02111&json=true","fetch_graph":"https://pith.science/api/pith-number/2YBGBIJX4KJYPFAWRLBHZX4QDA/graph.json","fetch_events":"https://pith.science/api/pith-number/2YBGBIJX4KJYPFAWRLBHZX4QDA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/2YBGBIJX4KJYPFAWRLBHZX4QDA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/2YBGBIJX4KJYPFAWRLBHZX4QDA/action/storage_attestation","attest_author":"https://pith.science/pith/2YBGBIJX4KJYPFAWRLBHZX4QDA/action/author_attestation","sign_citation":"https://pith.science/pith/2YBGBIJX4KJYPFAWRLBHZX4QDA/action/citation_signature","submit_replication":"https://pith.science/pith/2YBGBIJX4KJYPFAWRLBHZX4QDA/action/replication_record"}},"created_at":"2026-07-05T11:14:32.722225+00:00","updated_at":"2026-07-05T11:14:32.722225+00:00"}