{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:BINYRMAMO327AJNYP4CFVI4K5F","short_pith_number":"pith:BINYRMAM","schema_version":"1.0","canonical_sha256":"0a1b88b00c76f5f025b87f045aa38ae95fc8a2c9f89a29bb96225face494e1e9","source":{"kind":"arxiv","id":"2110.02997","version":2},"attestation_state":"computed","paper":{"title":"Tidal Deformabilities of Neutron Stars in scalar-Gauss-Bonnet Gravity and Their Applications to Multimessenger Tests of Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alexander Saffer, Kent Yagi","submitted_at":"2021-10-06T18:12:37Z","abstract_excerpt":"The spacetime surrounding compact objects such as neutron stars and black holes provides an excellent place to study gravity in the strong, non-linear, dynamical regime. Here, the effects of strong curvature can leave their imprint on observables which we may use to study gravity. Recently, NICER provided a mass and radius measurement of an isolated neutron star using x-rays, while LIGO/Virgo measured the tidal deformability of neutron stars through gravitational waves. These measurements can be used to test the relation between the tidal deformability and compactness of neutron stars that are"},"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":"2110.02997","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2021-10-06T18:12:37Z","cross_cats_sorted":[],"title_canon_sha256":"4097d1f095cb95079d0b386154688cf248e23a0f0f820fdeb19aa9bfcfc27233","abstract_canon_sha256":"d7c5592954a8106f52e9f75ea675efbd5e9d3c210a5e879d9659a098b57f314b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:45:48.486998Z","signature_b64":"FmU8MQjbtd15TjnYFVjLzzW1+LRxFhwkHRToePXeTCQV/QJ9FHnhMYbVDPqdfB7XMrQA4SHwPiRz4mqJzBvKAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0a1b88b00c76f5f025b87f045aa38ae95fc8a2c9f89a29bb96225face494e1e9","last_reissued_at":"2026-07-05T03:45:48.486577Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:45:48.486577Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Tidal Deformabilities of Neutron Stars in scalar-Gauss-Bonnet Gravity and Their Applications to Multimessenger Tests of Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Alexander Saffer, Kent Yagi","submitted_at":"2021-10-06T18:12:37Z","abstract_excerpt":"The spacetime surrounding compact objects such as neutron stars and black holes provides an excellent place to study gravity in the strong, non-linear, dynamical regime. Here, the effects of strong curvature can leave their imprint on observables which we may use to study gravity. Recently, NICER provided a mass and radius measurement of an isolated neutron star using x-rays, while LIGO/Virgo measured the tidal deformability of neutron stars through gravitational waves. These measurements can be used to test the relation between the tidal deformability and compactness of neutron stars that are"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2110.02997","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/2110.02997/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":"2110.02997","created_at":"2026-07-05T03:45:48.486633+00:00"},{"alias_kind":"arxiv_version","alias_value":"2110.02997v2","created_at":"2026-07-05T03:45:48.486633+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2110.02997","created_at":"2026-07-05T03:45:48.486633+00:00"},{"alias_kind":"pith_short_12","alias_value":"BINYRMAMO327","created_at":"2026-07-05T03:45:48.486633+00:00"},{"alias_kind":"pith_short_16","alias_value":"BINYRMAMO327AJNY","created_at":"2026-07-05T03:45:48.486633+00:00"},{"alias_kind":"pith_short_8","alias_value":"BINYRMAM","created_at":"2026-07-05T03:45:48.486633+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.27429","citing_title":"Massive scalar fields in eccentric regime: Detectability and constraints from LISA observations of extreme mass-ratio inspirals","ref_index":82,"is_internal_anchor":false},{"citing_arxiv_id":"2406.03568","citing_title":"Tests of General Relativity with GW230529: a neutron star merging with a lower mass-gap compact object","ref_index":120,"is_internal_anchor":false},{"citing_arxiv_id":"2510.22137","citing_title":"Inferring neutron-star Love-Q relations from gravitational waves in the hierarchical Bayesian framework","ref_index":106,"is_internal_anchor":false},{"citing_arxiv_id":"2511.12580","citing_title":"Dynamical Tidal Response of Non-rotating Black Holes: Connecting the MST Formalism and Worldline EFT","ref_index":50,"is_internal_anchor":false},{"citing_arxiv_id":"2605.02633","citing_title":"Axial tidal Love numbers of black holes in matter environments","ref_index":56,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BINYRMAMO327AJNYP4CFVI4K5F","json":"https://pith.science/pith/BINYRMAMO327AJNYP4CFVI4K5F.json","graph_json":"https://pith.science/api/pith-number/BINYRMAMO327AJNYP4CFVI4K5F/graph.json","events_json":"https://pith.science/api/pith-number/BINYRMAMO327AJNYP4CFVI4K5F/events.json","paper":"https://pith.science/paper/BINYRMAM"},"agent_actions":{"view_html":"https://pith.science/pith/BINYRMAMO327AJNYP4CFVI4K5F","download_json":"https://pith.science/pith/BINYRMAMO327AJNYP4CFVI4K5F.json","view_paper":"https://pith.science/paper/BINYRMAM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2110.02997&json=true","fetch_graph":"https://pith.science/api/pith-number/BINYRMAMO327AJNYP4CFVI4K5F/graph.json","fetch_events":"https://pith.science/api/pith-number/BINYRMAMO327AJNYP4CFVI4K5F/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BINYRMAMO327AJNYP4CFVI4K5F/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BINYRMAMO327AJNYP4CFVI4K5F/action/storage_attestation","attest_author":"https://pith.science/pith/BINYRMAMO327AJNYP4CFVI4K5F/action/author_attestation","sign_citation":"https://pith.science/pith/BINYRMAMO327AJNYP4CFVI4K5F/action/citation_signature","submit_replication":"https://pith.science/pith/BINYRMAMO327AJNYP4CFVI4K5F/action/replication_record"}},"created_at":"2026-07-05T03:45:48.486633+00:00","updated_at":"2026-07-05T03:45:48.486633+00:00"}