{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:BHNUTKHYZFSD7M5A3WBBE6HZIJ","short_pith_number":"pith:BHNUTKHY","schema_version":"1.0","canonical_sha256":"09db49a8f8c9643fb3a0dd821278f942500fccb207bb53b069a284c21025e1ed","source":{"kind":"arxiv","id":"1905.13460","version":2},"attestation_state":"computed","paper":{"title":"Bounding Alternative Theories of Gravity with Multi-Band GW Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Andrea Maselli, Giuseppe Gnocchi, Michela Mapelli, Nicola Giacobbo, Tiziano Abdelsalhin","submitted_at":"2019-05-31T08:20:51Z","abstract_excerpt":"We study the constraints on alternative theories of gravity that can be determined by multi-band observations of gravitational wave signals emitted from binary black hole coalescences. We focus on three types of General Relativity modifications induced by a generalised Brans-Dicke theory, and two classes of quadratic gravity, Einstein-dilaton-Gauss-Bonnet and dynamical Chern-Simons. Considering a network of space and ground-based detectors, supplied by a population of spinning binaries black hole, we show how the multi-band analysis improves the existing bounds on the theory's parameters by se"},"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":"1905.13460","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-05-31T08:20:51Z","cross_cats_sorted":[],"title_canon_sha256":"fd2805f012204558eec20a27720e04d7a4a747a285e8a8c78986954a645af0f9","abstract_canon_sha256":"65fd9f6a99e3fdc929de11e85ec68bceadfee05ea51ad160846ba4585d33fd82"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:05:10.935898Z","signature_b64":"5GEkKSDzgkr5TcWX8UlUCqThGQEs5RSuF58/JjCXA1Kr/CJFCfRQSXg97HHqG+cokVTdRm21hwApDst3bwuyDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"09db49a8f8c9643fb3a0dd821278f942500fccb207bb53b069a284c21025e1ed","last_reissued_at":"2026-07-05T00:05:10.935475Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:05:10.935475Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Bounding Alternative Theories of Gravity with Multi-Band GW Observations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Andrea Maselli, Giuseppe Gnocchi, Michela Mapelli, Nicola Giacobbo, Tiziano Abdelsalhin","submitted_at":"2019-05-31T08:20:51Z","abstract_excerpt":"We study the constraints on alternative theories of gravity that can be determined by multi-band observations of gravitational wave signals emitted from binary black hole coalescences. We focus on three types of General Relativity modifications induced by a generalised Brans-Dicke theory, and two classes of quadratic gravity, Einstein-dilaton-Gauss-Bonnet and dynamical Chern-Simons. Considering a network of space and ground-based detectors, supplied by a population of spinning binaries black hole, we show how the multi-band analysis improves the existing bounds on the theory's parameters by se"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1905.13460","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/1905.13460/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":"1905.13460","created_at":"2026-07-05T00:05:10.935531+00:00"},{"alias_kind":"arxiv_version","alias_value":"1905.13460v2","created_at":"2026-07-05T00:05:10.935531+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1905.13460","created_at":"2026-07-05T00:05:10.935531+00:00"},{"alias_kind":"pith_short_12","alias_value":"BHNUTKHYZFSD","created_at":"2026-07-05T00:05:10.935531+00:00"},{"alias_kind":"pith_short_16","alias_value":"BHNUTKHYZFSD7M5A","created_at":"2026-07-05T00:05:10.935531+00:00"},{"alias_kind":"pith_short_8","alias_value":"BHNUTKHY","created_at":"2026-07-05T00:05:10.935531+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.04216","citing_title":"Shape of U: Measuring the Curvature of the Universe with Gravitational Waves","ref_index":74,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BHNUTKHYZFSD7M5A3WBBE6HZIJ","json":"https://pith.science/pith/BHNUTKHYZFSD7M5A3WBBE6HZIJ.json","graph_json":"https://pith.science/api/pith-number/BHNUTKHYZFSD7M5A3WBBE6HZIJ/graph.json","events_json":"https://pith.science/api/pith-number/BHNUTKHYZFSD7M5A3WBBE6HZIJ/events.json","paper":"https://pith.science/paper/BHNUTKHY"},"agent_actions":{"view_html":"https://pith.science/pith/BHNUTKHYZFSD7M5A3WBBE6HZIJ","download_json":"https://pith.science/pith/BHNUTKHYZFSD7M5A3WBBE6HZIJ.json","view_paper":"https://pith.science/paper/BHNUTKHY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1905.13460&json=true","fetch_graph":"https://pith.science/api/pith-number/BHNUTKHYZFSD7M5A3WBBE6HZIJ/graph.json","fetch_events":"https://pith.science/api/pith-number/BHNUTKHYZFSD7M5A3WBBE6HZIJ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BHNUTKHYZFSD7M5A3WBBE6HZIJ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BHNUTKHYZFSD7M5A3WBBE6HZIJ/action/storage_attestation","attest_author":"https://pith.science/pith/BHNUTKHYZFSD7M5A3WBBE6HZIJ/action/author_attestation","sign_citation":"https://pith.science/pith/BHNUTKHYZFSD7M5A3WBBE6HZIJ/action/citation_signature","submit_replication":"https://pith.science/pith/BHNUTKHYZFSD7M5A3WBBE6HZIJ/action/replication_record"}},"created_at":"2026-07-05T00:05:10.935531+00:00","updated_at":"2026-07-05T00:05:10.935531+00:00"}