{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:LQHF7VW6LQTN5T7OJZ65WPKSXF","short_pith_number":"pith:LQHF7VW6","schema_version":"1.0","canonical_sha256":"5c0e5fd6de5c26decfee4e7ddb3d52b94a34cdaf8f130eb2a99c673608293951","source":{"kind":"arxiv","id":"1703.10612","version":4},"attestation_state":"computed","paper":{"title":"Probing Planckian corrections at the horizon scale with LISA binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Andrea Maselli, Leonardo Gualtieri, Paolo Pani, Tiziano Abdelsalhin, Valeria Ferrari, Vitor Cardoso","submitted_at":"2017-03-30T18:00:11Z","abstract_excerpt":"Several quantum-gravity models of compact objects predict microscopic or even Planckian corrections at the horizon scale. We explore the possibility of measuring two model-independent, smoking-gun effects of these corrections in the gravitational waveform of a compact binary, namely the absence of tidal heating and the presence of tidal deformability. For events detectable by the future space-based interferometer LISA, we show that the effect of tidal heating dominates and allows one to constrain putative corrections down to the Planck scale. The measurement of the tidal Love numbers with LISA"},"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":"1703.10612","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2017-03-30T18:00:11Z","cross_cats_sorted":["astro-ph.HE","hep-ph","hep-th"],"title_canon_sha256":"9e2653951ff2aad0a1c9593e44a036a5a559eabf3904ca9b1c1fa77af7ff301f","abstract_canon_sha256":"43da842729ee76d3f1af04a1dab38ca7b3429948f922967f3c26adc1195e038b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:22:11.063995Z","signature_b64":"pManzLHOKmzCXnpOgqsBUsJvGGKUKYi9eQp04zXw5gkYTYLOGvytuikg9KGZJZc98ZokS3s0K/eTHq3dpfwRDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5c0e5fd6de5c26decfee4e7ddb3d52b94a34cdaf8f130eb2a99c673608293951","last_reissued_at":"2026-05-18T00:22:11.063341Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:22:11.063341Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing Planckian corrections at the horizon scale with LISA binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Andrea Maselli, Leonardo Gualtieri, Paolo Pani, Tiziano Abdelsalhin, Valeria Ferrari, Vitor Cardoso","submitted_at":"2017-03-30T18:00:11Z","abstract_excerpt":"Several quantum-gravity models of compact objects predict microscopic or even Planckian corrections at the horizon scale. We explore the possibility of measuring two model-independent, smoking-gun effects of these corrections in the gravitational waveform of a compact binary, namely the absence of tidal heating and the presence of tidal deformability. For events detectable by the future space-based interferometer LISA, we show that the effect of tidal heating dominates and allows one to constrain putative corrections down to the Planck scale. The measurement of the tidal Love numbers with LISA"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.10612","kind":"arxiv","version":4},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"1703.10612","created_at":"2026-05-18T00:22:11.063445+00:00"},{"alias_kind":"arxiv_version","alias_value":"1703.10612v4","created_at":"2026-05-18T00:22:11.063445+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.10612","created_at":"2026-05-18T00:22:11.063445+00:00"},{"alias_kind":"pith_short_12","alias_value":"LQHF7VW6LQTN","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_16","alias_value":"LQHF7VW6LQTN5T7O","created_at":"2026-05-18T12:31:28.150371+00:00"},{"alias_kind":"pith_short_8","alias_value":"LQHF7VW6","created_at":"2026-05-18T12:31:28.150371+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":8,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"2605.19731","citing_title":"Neutron stars more compact than black holes in quasi-topological gravity: Equilibrium configurations and radial stability","ref_index":63,"is_internal_anchor":true},{"citing_arxiv_id":"2506.22363","citing_title":"Binary black holes in the heat of merger","ref_index":14,"is_internal_anchor":true},{"citing_arxiv_id":"2511.12580","citing_title":"Dynamical Tidal Response of Non-rotating Black Holes: Connecting the MST Formalism and Worldline EFT","ref_index":67,"is_internal_anchor":true},{"citing_arxiv_id":"2512.05767","citing_title":"Tidal Love numbers for regular black holes","ref_index":51,"is_internal_anchor":true},{"citing_arxiv_id":"2010.14529","citing_title":"Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog","ref_index":189,"is_internal_anchor":true},{"citing_arxiv_id":"1904.05363","citing_title":"Testing the nature of dark compact objects: a status report","ref_index":138,"is_internal_anchor":false},{"citing_arxiv_id":"2112.06861","citing_title":"Tests of General Relativity with GWTC-3","ref_index":231,"is_internal_anchor":false},{"citing_arxiv_id":"2605.02633","citing_title":"Axial tidal Love numbers of black holes in matter environments","ref_index":52,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LQHF7VW6LQTN5T7OJZ65WPKSXF","json":"https://pith.science/pith/LQHF7VW6LQTN5T7OJZ65WPKSXF.json","graph_json":"https://pith.science/api/pith-number/LQHF7VW6LQTN5T7OJZ65WPKSXF/graph.json","events_json":"https://pith.science/api/pith-number/LQHF7VW6LQTN5T7OJZ65WPKSXF/events.json","paper":"https://pith.science/paper/LQHF7VW6"},"agent_actions":{"view_html":"https://pith.science/pith/LQHF7VW6LQTN5T7OJZ65WPKSXF","download_json":"https://pith.science/pith/LQHF7VW6LQTN5T7OJZ65WPKSXF.json","view_paper":"https://pith.science/paper/LQHF7VW6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1703.10612&json=true","fetch_graph":"https://pith.science/api/pith-number/LQHF7VW6LQTN5T7OJZ65WPKSXF/graph.json","fetch_events":"https://pith.science/api/pith-number/LQHF7VW6LQTN5T7OJZ65WPKSXF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LQHF7VW6LQTN5T7OJZ65WPKSXF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LQHF7VW6LQTN5T7OJZ65WPKSXF/action/storage_attestation","attest_author":"https://pith.science/pith/LQHF7VW6LQTN5T7OJZ65WPKSXF/action/author_attestation","sign_citation":"https://pith.science/pith/LQHF7VW6LQTN5T7OJZ65WPKSXF/action/citation_signature","submit_replication":"https://pith.science/pith/LQHF7VW6LQTN5T7OJZ65WPKSXF/action/replication_record"}},"created_at":"2026-05-18T00:22:11.063445+00:00","updated_at":"2026-05-18T00:22:11.063445+00:00"}