{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:KN2VVBEV6GTCDPRJN3YCR7QFOI","short_pith_number":"pith:KN2VVBEV","schema_version":"1.0","canonical_sha256":"53755a8495f1a621be296ef028fe05722b12b08821937839db78b26cf0e0f39f","source":{"kind":"arxiv","id":"2303.16036","version":2},"attestation_state":"computed","paper":{"title":"Scalar Love numbers and Love symmetries of 5-dimensional Myers-Perry black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Mikhail M. Ivanov, Panagiotis Charalambous","submitted_at":"2023-03-28T15:07:56Z","abstract_excerpt":"The near-zone ``Love'' symmetry resolves the naturalness issue of black hole Love number vanishing with $\\text{SL}\\left(2,\\mathbb{R}\\right)$ representation theory. Here, we generalize this proposal to $5$-dimensional asymptotically flat and doubly spinning (Myers-Perry) black holes. We consider the scalar response of Myers-Perry black holes and extract its static scalar Love numbers. In agreement with the naturalness arguments, these Love numbers are, in general, non-zero and exhibit logarithmic running unless certain resonant conditions are met; these conditions include new cases with no prev"},"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":"2303.16036","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2023-03-28T15:07:56Z","cross_cats_sorted":["astro-ph.HE","gr-qc","hep-ph"],"title_canon_sha256":"f626786161980b12d01fc5592f435835fac05a33ce86240ddca9467e15a6a97d","abstract_canon_sha256":"ab442341e2e3fbaa5a6cf0895ad71afdad71521682afe56eee4c6bba7c9c34df"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:41:14.544130Z","signature_b64":"jgnwGEumKgzqO1TXRpT40q7Njopp24435UYMLl2YOPLA+eN24jGWLhV6fpOG5KsYbgJhb6Sd245Dbr2N6r9NBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"53755a8495f1a621be296ef028fe05722b12b08821937839db78b26cf0e0f39f","last_reissued_at":"2026-07-05T06:41:14.543698Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:41:14.543698Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Scalar Love numbers and Love symmetries of 5-dimensional Myers-Perry black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Mikhail M. Ivanov, Panagiotis Charalambous","submitted_at":"2023-03-28T15:07:56Z","abstract_excerpt":"The near-zone ``Love'' symmetry resolves the naturalness issue of black hole Love number vanishing with $\\text{SL}\\left(2,\\mathbb{R}\\right)$ representation theory. Here, we generalize this proposal to $5$-dimensional asymptotically flat and doubly spinning (Myers-Perry) black holes. We consider the scalar response of Myers-Perry black holes and extract its static scalar Love numbers. In agreement with the naturalness arguments, these Love numbers are, in general, non-zero and exhibit logarithmic running unless certain resonant conditions are met; these conditions include new cases with no prev"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2303.16036","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/2303.16036/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":"2303.16036","created_at":"2026-07-05T06:41:14.543751+00:00"},{"alias_kind":"arxiv_version","alias_value":"2303.16036v2","created_at":"2026-07-05T06:41:14.543751+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2303.16036","created_at":"2026-07-05T06:41:14.543751+00:00"},{"alias_kind":"pith_short_12","alias_value":"KN2VVBEV6GTC","created_at":"2026-07-05T06:41:14.543751+00:00"},{"alias_kind":"pith_short_16","alias_value":"KN2VVBEV6GTCDPRJ","created_at":"2026-07-05T06:41:14.543751+00:00"},{"alias_kind":"pith_short_8","alias_value":"KN2VVBEV","created_at":"2026-07-05T06:41:14.543751+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.19446","citing_title":"Dynamical Tidal Response of Neutron Stars: from Effective Field Theory to Gravitational Waveforms","ref_index":66,"is_internal_anchor":false},{"citing_arxiv_id":"2504.07862","citing_title":"Resummation of Universal Tails in Gravitational Waveforms","ref_index":85,"is_internal_anchor":false},{"citing_arxiv_id":"2605.16792","citing_title":"Static electromagnetic Love tensors of 5-dimensional Myers-Perry black holes","ref_index":12,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03025","citing_title":"Can wormholes have vanishing Love numbers?","ref_index":33,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08653","citing_title":"Love numbers of black holes and compact objects","ref_index":105,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KN2VVBEV6GTCDPRJN3YCR7QFOI","json":"https://pith.science/pith/KN2VVBEV6GTCDPRJN3YCR7QFOI.json","graph_json":"https://pith.science/api/pith-number/KN2VVBEV6GTCDPRJN3YCR7QFOI/graph.json","events_json":"https://pith.science/api/pith-number/KN2VVBEV6GTCDPRJN3YCR7QFOI/events.json","paper":"https://pith.science/paper/KN2VVBEV"},"agent_actions":{"view_html":"https://pith.science/pith/KN2VVBEV6GTCDPRJN3YCR7QFOI","download_json":"https://pith.science/pith/KN2VVBEV6GTCDPRJN3YCR7QFOI.json","view_paper":"https://pith.science/paper/KN2VVBEV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2303.16036&json=true","fetch_graph":"https://pith.science/api/pith-number/KN2VVBEV6GTCDPRJN3YCR7QFOI/graph.json","fetch_events":"https://pith.science/api/pith-number/KN2VVBEV6GTCDPRJN3YCR7QFOI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KN2VVBEV6GTCDPRJN3YCR7QFOI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KN2VVBEV6GTCDPRJN3YCR7QFOI/action/storage_attestation","attest_author":"https://pith.science/pith/KN2VVBEV6GTCDPRJN3YCR7QFOI/action/author_attestation","sign_citation":"https://pith.science/pith/KN2VVBEV6GTCDPRJN3YCR7QFOI/action/citation_signature","submit_replication":"https://pith.science/pith/KN2VVBEV6GTCDPRJN3YCR7QFOI/action/replication_record"}},"created_at":"2026-07-05T06:41:14.543751+00:00","updated_at":"2026-07-05T06:41:14.543751+00:00"}