{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2000:JIYFZIQ5OK6NNHFFQLSG3NSESG","short_pith_number":"pith:JIYFZIQ5","schema_version":"1.0","canonical_sha256":"4a305ca21d72bcd69ca582e46db64491bdbbce6a9a10b62c628100e1ad344646","source":{"kind":"arxiv","id":"hep-ph/0009290","version":2},"attestation_state":"computed","paper":{"title":"Strong CP problem and mirror world: the Weinberg Wilczek axion revisited","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Leonida Gianfagna, Maurizio Giannotti, Zurab Berezhiani","submitted_at":"2000-09-25T21:28:40Z","abstract_excerpt":"A new possibility for solving the strong CP-problem is suggested,which assumes that apart of the ordinary world of observable particles described by standard model, there exits a mirror sector of particles and two sectors share the same Peccei-Quinn symmetry realized {\\it a l\\`a} Weinberg-Wilczek model. The mirror gauge group is completely analogous to that of the standard model for ordinary particles but having somewhat larger electroweak scale,which in turn implies the infrared scale $\\Lambda'$ of the mirror strong interactions has to be larger than the ordinary QCD scale $\\Lambda$. In this "},"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/0009290","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2000-09-25T21:28:40Z","cross_cats_sorted":[],"title_canon_sha256":"9dfa2214f653d0c7a14d1ffb424a230afdb6df0a2977ca83cffb0cb60d1385ed","abstract_canon_sha256":"9c2037a81e4f03e4d17894c5291f978777793a3496ff23f2bba294035d52adcb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:20:27.132922Z","signature_b64":"UQ/SMkVLmlfRqwVV0qod3PE1T/lyHpdeY5T/E4CPSskdjKHgRAvT29Cb4Cf0/5wiC6t16rpv1uHI1p2l+obCAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4a305ca21d72bcd69ca582e46db64491bdbbce6a9a10b62c628100e1ad344646","last_reissued_at":"2026-07-04T16:20:27.132503Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:20:27.132503Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Strong CP problem and mirror world: the Weinberg Wilczek axion revisited","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Leonida Gianfagna, Maurizio Giannotti, Zurab Berezhiani","submitted_at":"2000-09-25T21:28:40Z","abstract_excerpt":"A new possibility for solving the strong CP-problem is suggested,which assumes that apart of the ordinary world of observable particles described by standard model, there exits a mirror sector of particles and two sectors share the same Peccei-Quinn symmetry realized {\\it a l\\`a} Weinberg-Wilczek model. The mirror gauge group is completely analogous to that of the standard model for ordinary particles but having somewhat larger electroweak scale,which in turn implies the infrared scale $\\Lambda'$ of the mirror strong interactions has to be larger than the ordinary QCD scale $\\Lambda$. In this "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0009290","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/hep-ph/0009290/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/0009290","created_at":"2026-07-04T16:20:27.132571+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0009290v2","created_at":"2026-07-04T16:20:27.132571+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0009290","created_at":"2026-07-04T16:20:27.132571+00:00"},{"alias_kind":"pith_short_12","alias_value":"JIYFZIQ5OK6N","created_at":"2026-07-04T16:20:27.132571+00:00"},{"alias_kind":"pith_short_16","alias_value":"JIYFZIQ5OK6NNHFF","created_at":"2026-07-04T16:20:27.132571+00:00"},{"alias_kind":"pith_short_8","alias_value":"JIYFZIQ5","created_at":"2026-07-04T16:20:27.132571+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":8,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"2606.02728","citing_title":"Deconstructing the Extra-Dimensional Axion","ref_index":36,"is_internal_anchor":true},{"citing_arxiv_id":"2605.06787","citing_title":"The structure of multi-axion solutions to the strong CP problem","ref_index":48,"is_internal_anchor":true},{"citing_arxiv_id":"2305.15473","citing_title":"Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter","ref_index":94,"is_internal_anchor":true},{"citing_arxiv_id":"2509.14323","citing_title":"High-Quality Axion Dark Matter at Gravitational Wave Interferometers","ref_index":53,"is_internal_anchor":true},{"citing_arxiv_id":"2601.00068","citing_title":"Braking protons at the EIC: from invisible meson decay to new physics searches","ref_index":74,"is_internal_anchor":true},{"citing_arxiv_id":"2604.24849","citing_title":"Accidental Peccei-Quinn Symmetry from Chiral Gauge Symmetry and Mirror QCD","ref_index":36,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08667","citing_title":"On Exclusive Coherent Production of Bosons in Electron-Proton Collisions","ref_index":48,"is_internal_anchor":false},{"citing_arxiv_id":"2605.06787","citing_title":"The structure of multi-axion solutions to the strong CP problem","ref_index":48,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JIYFZIQ5OK6NNHFFQLSG3NSESG","json":"https://pith.science/pith/JIYFZIQ5OK6NNHFFQLSG3NSESG.json","graph_json":"https://pith.science/api/pith-number/JIYFZIQ5OK6NNHFFQLSG3NSESG/graph.json","events_json":"https://pith.science/api/pith-number/JIYFZIQ5OK6NNHFFQLSG3NSESG/events.json","paper":"https://pith.science/paper/JIYFZIQ5"},"agent_actions":{"view_html":"https://pith.science/pith/JIYFZIQ5OK6NNHFFQLSG3NSESG","download_json":"https://pith.science/pith/JIYFZIQ5OK6NNHFFQLSG3NSESG.json","view_paper":"https://pith.science/paper/JIYFZIQ5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0009290&json=true","fetch_graph":"https://pith.science/api/pith-number/JIYFZIQ5OK6NNHFFQLSG3NSESG/graph.json","fetch_events":"https://pith.science/api/pith-number/JIYFZIQ5OK6NNHFFQLSG3NSESG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JIYFZIQ5OK6NNHFFQLSG3NSESG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JIYFZIQ5OK6NNHFFQLSG3NSESG/action/storage_attestation","attest_author":"https://pith.science/pith/JIYFZIQ5OK6NNHFFQLSG3NSESG/action/author_attestation","sign_citation":"https://pith.science/pith/JIYFZIQ5OK6NNHFFQLSG3NSESG/action/citation_signature","submit_replication":"https://pith.science/pith/JIYFZIQ5OK6NNHFFQLSG3NSESG/action/replication_record"}},"created_at":"2026-07-04T16:20:27.132571+00:00","updated_at":"2026-07-04T16:20:27.132571+00:00"}