{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:GEYDNCSLR27HAVMWWYREHDNX4L","short_pith_number":"pith:GEYDNCSL","schema_version":"1.0","canonical_sha256":"3130368a4b8ebe705596b622438db7e2dfc1327a1bc945aa2be9c67ee8017f08","source":{"kind":"arxiv","id":"2601.03571","version":2},"attestation_state":"computed","paper":{"title":"Constraining Lorentz and parity violations in gravity with multiband gravitational wave observations","license":"http://creativecommons.org/licenses/by-sa/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Tao Zhu, Zhi-Xin Jia, Zhoujian Cao","submitted_at":"2026-01-07T04:31:04Z","abstract_excerpt":"This study evaluates the capability of future multi-band observations of gravitational waves emitted from binary black hole coalescences, utilizing joint third-generation ground-based (CE, ET) and space-based (LISA, Taiji, TianQin) detector networks, to constrain parity and Lorentz symmetry violations in the gravitational sector. We model these effects through a parameterized waveform framework that incorporates a set of parameters that quantify potential deviations from general relativity. The frequency-dependence of their effects is described by power-law indices $\\beta$ (i.e., $\\beta_{\\bar "},"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":"2601.03571","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by-sa/4.0/","primary_cat":"gr-qc","submitted_at":"2026-01-07T04:31:04Z","cross_cats_sorted":["astro-ph.IM"],"title_canon_sha256":"e8c9e694aa8d242936ab6f3a952f66ea1878949fefdd4220a34463d62262b990","abstract_canon_sha256":"6b6fe7b15186d7d40ff367c8dd1e241af285761bc79e30c12dce82491e5d1d44"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-23T01:12:00.036194Z","signature_b64":"fpSJHbJ+EUcDGsj5YX3rSKJyfsdix5ig3eMdR7KbcQVv0IvLaRkY3oAoQBtrlxwk8V+YxVvowqrMiu/Skg30Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3130368a4b8ebe705596b622438db7e2dfc1327a1bc945aa2be9c67ee8017f08","last_reissued_at":"2026-06-23T01:12:00.035698Z","signature_status":"signed_v1","first_computed_at":"2026-06-23T01:12:00.035698Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraining Lorentz and parity violations in gravity with multiband gravitational wave observations","license":"http://creativecommons.org/licenses/by-sa/4.0/","headline":"","cross_cats":["astro-ph.IM"],"primary_cat":"gr-qc","authors_text":"Tao Zhu, Zhi-Xin Jia, Zhoujian Cao","submitted_at":"2026-01-07T04:31:04Z","abstract_excerpt":"This study evaluates the capability of future multi-band observations of gravitational waves emitted from binary black hole coalescences, utilizing joint third-generation ground-based (CE, ET) and space-based (LISA, Taiji, TianQin) detector networks, to constrain parity and Lorentz symmetry violations in the gravitational sector. We model these effects through a parameterized waveform framework that incorporates a set of parameters that quantify potential deviations from general relativity. The frequency-dependence of their effects is described by power-law indices $\\beta$ (i.e., $\\beta_{\\bar "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2601.03571","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/2601.03571/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":"2601.03571","created_at":"2026-06-23T01:12:00.035763+00:00"},{"alias_kind":"arxiv_version","alias_value":"2601.03571v2","created_at":"2026-06-23T01:12:00.035763+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2601.03571","created_at":"2026-06-23T01:12:00.035763+00:00"},{"alias_kind":"pith_short_12","alias_value":"GEYDNCSLR27H","created_at":"2026-06-23T01:12:00.035763+00:00"},{"alias_kind":"pith_short_16","alias_value":"GEYDNCSLR27HAVMW","created_at":"2026-06-23T01:12:00.035763+00:00"},{"alias_kind":"pith_short_8","alias_value":"GEYDNCSL","created_at":"2026-06-23T01:12:00.035763+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GEYDNCSLR27HAVMWWYREHDNX4L","json":"https://pith.science/pith/GEYDNCSLR27HAVMWWYREHDNX4L.json","graph_json":"https://pith.science/api/pith-number/GEYDNCSLR27HAVMWWYREHDNX4L/graph.json","events_json":"https://pith.science/api/pith-number/GEYDNCSLR27HAVMWWYREHDNX4L/events.json","paper":"https://pith.science/paper/GEYDNCSL"},"agent_actions":{"view_html":"https://pith.science/pith/GEYDNCSLR27HAVMWWYREHDNX4L","download_json":"https://pith.science/pith/GEYDNCSLR27HAVMWWYREHDNX4L.json","view_paper":"https://pith.science/paper/GEYDNCSL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2601.03571&json=true","fetch_graph":"https://pith.science/api/pith-number/GEYDNCSLR27HAVMWWYREHDNX4L/graph.json","fetch_events":"https://pith.science/api/pith-number/GEYDNCSLR27HAVMWWYREHDNX4L/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GEYDNCSLR27HAVMWWYREHDNX4L/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GEYDNCSLR27HAVMWWYREHDNX4L/action/storage_attestation","attest_author":"https://pith.science/pith/GEYDNCSLR27HAVMWWYREHDNX4L/action/author_attestation","sign_citation":"https://pith.science/pith/GEYDNCSLR27HAVMWWYREHDNX4L/action/citation_signature","submit_replication":"https://pith.science/pith/GEYDNCSLR27HAVMWWYREHDNX4L/action/replication_record"}},"created_at":"2026-06-23T01:12:00.035763+00:00","updated_at":"2026-06-23T01:12:00.035763+00:00"}