{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:LLEC636SQBJ2CGJBYYHU372AYV","short_pith_number":"pith:LLEC636S","schema_version":"1.0","canonical_sha256":"5ac82f6fd28053a11921c60f4dff40c5544515b20aaa3cbdc23f4b4413400701","source":{"kind":"arxiv","id":"1811.03689","version":2},"attestation_state":"computed","paper":{"title":"From micro to macro and back: probing near-horizon quantum structures with gravitational waves","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph"],"primary_cat":"gr-qc","authors_text":"Andrea Maselli, Leonardo Gualtieri, Paolo Pani, Tiziano Abdelsalhin, Valeria Ferrari, Vitor Cardoso","submitted_at":"2018-11-08T21:51:29Z","abstract_excerpt":"Supermassive binaries detectable by the future space gravitational-wave interferometer LISA might allow to distinguish black holes from ultracompact horizonless objects, even when the latter are motivated by quantum-gravity considerations. We show that a measurement of very small tidal Love numbers at the level of $10\\%$ accuracy (as achievable with \"golden binaries\") may also allow to distinguish between different models of these exotic compact objects, even when taking into account an intrinsic uncertainty in the object radius putatively due to quantum mechanics. We argue that there is no co"},"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":"1811.03689","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-11-08T21:51:29Z","cross_cats_sorted":["astro-ph.HE","hep-ph"],"title_canon_sha256":"88e760a6993a8fc469cf501e981a9a9a42c27ccaffcc5eb856162c48dc083ab0","abstract_canon_sha256":"d78ada1278ae127fe134da94bcbb43fd11c16d26e93513308eed97fc17adfef9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:39:41.582152Z","signature_b64":"SmA6yflcOcHs8CSbNYKG/d8Un3d9ASP1u5Qd68e2/Xh0YInQjmQYMU6Y7vDOztfYrGIeX4r3EW03qqmWgubcAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5ac82f6fd28053a11921c60f4dff40c5544515b20aaa3cbdc23f4b4413400701","last_reissued_at":"2026-05-17T23:39:41.581484Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:39:41.581484Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"From micro to macro and back: probing near-horizon quantum structures with gravitational waves","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph"],"primary_cat":"gr-qc","authors_text":"Andrea Maselli, Leonardo Gualtieri, Paolo Pani, Tiziano Abdelsalhin, Valeria Ferrari, Vitor Cardoso","submitted_at":"2018-11-08T21:51:29Z","abstract_excerpt":"Supermassive binaries detectable by the future space gravitational-wave interferometer LISA might allow to distinguish black holes from ultracompact horizonless objects, even when the latter are motivated by quantum-gravity considerations. We show that a measurement of very small tidal Love numbers at the level of $10\\%$ accuracy (as achievable with \"golden binaries\") may also allow to distinguish between different models of these exotic compact objects, even when taking into account an intrinsic uncertainty in the object radius putatively due to quantum mechanics. We argue that there is no co"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.03689","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":""},"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":"1811.03689","created_at":"2026-05-17T23:39:41.581595+00:00"},{"alias_kind":"arxiv_version","alias_value":"1811.03689v2","created_at":"2026-05-17T23:39:41.581595+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1811.03689","created_at":"2026-05-17T23:39:41.581595+00:00"},{"alias_kind":"pith_short_12","alias_value":"LLEC636SQBJ2","created_at":"2026-05-18T12:32:37.024351+00:00"},{"alias_kind":"pith_short_16","alias_value":"LLEC636SQBJ2CGJB","created_at":"2026-05-18T12:32:37.024351+00:00"},{"alias_kind":"pith_short_8","alias_value":"LLEC636S","created_at":"2026-05-18T12:32:37.024351+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2511.12580","citing_title":"Dynamical Tidal Response of Non-rotating Black Holes: Connecting the MST Formalism and Worldline EFT","ref_index":69,"is_internal_anchor":true},{"citing_arxiv_id":"2605.00693","citing_title":"Dynamical tidal Love numbers of black holes under generic perturbations: Connecting black hole perturbation theory with effective field theory","ref_index":49,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18669","citing_title":"Hawking area law in quantum gravity","ref_index":63,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LLEC636SQBJ2CGJBYYHU372AYV","json":"https://pith.science/pith/LLEC636SQBJ2CGJBYYHU372AYV.json","graph_json":"https://pith.science/api/pith-number/LLEC636SQBJ2CGJBYYHU372AYV/graph.json","events_json":"https://pith.science/api/pith-number/LLEC636SQBJ2CGJBYYHU372AYV/events.json","paper":"https://pith.science/paper/LLEC636S"},"agent_actions":{"view_html":"https://pith.science/pith/LLEC636SQBJ2CGJBYYHU372AYV","download_json":"https://pith.science/pith/LLEC636SQBJ2CGJBYYHU372AYV.json","view_paper":"https://pith.science/paper/LLEC636S","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1811.03689&json=true","fetch_graph":"https://pith.science/api/pith-number/LLEC636SQBJ2CGJBYYHU372AYV/graph.json","fetch_events":"https://pith.science/api/pith-number/LLEC636SQBJ2CGJBYYHU372AYV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LLEC636SQBJ2CGJBYYHU372AYV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LLEC636SQBJ2CGJBYYHU372AYV/action/storage_attestation","attest_author":"https://pith.science/pith/LLEC636SQBJ2CGJBYYHU372AYV/action/author_attestation","sign_citation":"https://pith.science/pith/LLEC636SQBJ2CGJBYYHU372AYV/action/citation_signature","submit_replication":"https://pith.science/pith/LLEC636SQBJ2CGJBYYHU372AYV/action/replication_record"}},"created_at":"2026-05-17T23:39:41.581595+00:00","updated_at":"2026-05-17T23:39:41.581595+00:00"}