{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:AC55NK2YHHDSI4CFOY4F7MZYUH","short_pith_number":"pith:AC55NK2Y","schema_version":"1.0","canonical_sha256":"00bbd6ab5839c724704576385fb338a1eec7c3c8be21dd9afc6f41448632c9b3","source":{"kind":"arxiv","id":"2502.02694","version":1},"attestation_state":"computed","paper":{"title":"Love numbers of black p-branes: fine tuning, Love symmetries, and their geometrization","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Mikhail M. Ivanov, Panagiotis Charalambous, Sergei Dubovsky","submitted_at":"2025-02-04T20:20:08Z","abstract_excerpt":"We compute scalar static response coefficients (Love numbers) of non-dilatonic black $p$-brane solutions in higher dimensional supergravity. This calculation revels a fine-tuning behavior similar to that of higher dimensional black holes, which we explain by ``hidden'' near-zone Love symmetries. In general, these symmetries act on equations for perturbations but they are not background isometries. The Love symmetry of charged $p=0$ branes is described by the usual $SL(2,\\mathbb{R})$ algebra. For $p=1$ the Love symmetry has an algebraic structure $SL(2,\\mathbb{R})\\times SL(2,\\mathbb{R})$. The $"},"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":"2502.02694","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2025-02-04T20:20:08Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"18b08ac1d4612ec6a0c2d2185ed96698b100a81d597e9331f80264d764d75d84","abstract_canon_sha256":"04bc1f202580ede84614e4399fc29b68052ed418014546e575a60675c6bb9282"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:09:53.632215Z","signature_b64":"OZokREdjtON8pLxKImeQ4FU2k2uDHeFJ0WrMzuV0SiTmvPaEA0f4RmMjEKP0Y3/5sl3rljefVufrLTNl2G+3Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"00bbd6ab5839c724704576385fb338a1eec7c3c8be21dd9afc6f41448632c9b3","last_reissued_at":"2026-07-05T10:09:53.631834Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:09:53.631834Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Love numbers of black p-branes: fine tuning, Love symmetries, and their geometrization","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Mikhail M. Ivanov, Panagiotis Charalambous, Sergei Dubovsky","submitted_at":"2025-02-04T20:20:08Z","abstract_excerpt":"We compute scalar static response coefficients (Love numbers) of non-dilatonic black $p$-brane solutions in higher dimensional supergravity. This calculation revels a fine-tuning behavior similar to that of higher dimensional black holes, which we explain by ``hidden'' near-zone Love symmetries. In general, these symmetries act on equations for perturbations but they are not background isometries. The Love symmetry of charged $p=0$ branes is described by the usual $SL(2,\\mathbb{R})$ algebra. For $p=1$ the Love symmetry has an algebraic structure $SL(2,\\mathbb{R})\\times SL(2,\\mathbb{R})$. The $"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.02694","kind":"arxiv","version":1},"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/2502.02694/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":"2502.02694","created_at":"2026-07-05T10:09:53.631885+00:00"},{"alias_kind":"arxiv_version","alias_value":"2502.02694v1","created_at":"2026-07-05T10:09:53.631885+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.02694","created_at":"2026-07-05T10:09:53.631885+00:00"},{"alias_kind":"pith_short_12","alias_value":"AC55NK2YHHDS","created_at":"2026-07-05T10:09:53.631885+00:00"},{"alias_kind":"pith_short_16","alias_value":"AC55NK2YHHDSI4CF","created_at":"2026-07-05T10:09:53.631885+00:00"},{"alias_kind":"pith_short_8","alias_value":"AC55NK2Y","created_at":"2026-07-05T10:09:53.631885+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.19281","citing_title":"Universal Closed Form for Dynamical Love Numbers of Black Holes","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2605.16792","citing_title":"Static electromagnetic Love tensors of 5-dimensional Myers-Perry black holes","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2505.21489","citing_title":"5-Dimensional Gravitational Raman Scattering: Scalar Wave Perturbations in Schwarzschild-Tangherlini Spacetime","ref_index":59,"is_internal_anchor":false},{"citing_arxiv_id":"2604.27046","citing_title":"Tidal Response and Thermodynamics of Black Holes","ref_index":26,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AC55NK2YHHDSI4CFOY4F7MZYUH","json":"https://pith.science/pith/AC55NK2YHHDSI4CFOY4F7MZYUH.json","graph_json":"https://pith.science/api/pith-number/AC55NK2YHHDSI4CFOY4F7MZYUH/graph.json","events_json":"https://pith.science/api/pith-number/AC55NK2YHHDSI4CFOY4F7MZYUH/events.json","paper":"https://pith.science/paper/AC55NK2Y"},"agent_actions":{"view_html":"https://pith.science/pith/AC55NK2YHHDSI4CFOY4F7MZYUH","download_json":"https://pith.science/pith/AC55NK2YHHDSI4CFOY4F7MZYUH.json","view_paper":"https://pith.science/paper/AC55NK2Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2502.02694&json=true","fetch_graph":"https://pith.science/api/pith-number/AC55NK2YHHDSI4CFOY4F7MZYUH/graph.json","fetch_events":"https://pith.science/api/pith-number/AC55NK2YHHDSI4CFOY4F7MZYUH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AC55NK2YHHDSI4CFOY4F7MZYUH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AC55NK2YHHDSI4CFOY4F7MZYUH/action/storage_attestation","attest_author":"https://pith.science/pith/AC55NK2YHHDSI4CFOY4F7MZYUH/action/author_attestation","sign_citation":"https://pith.science/pith/AC55NK2YHHDSI4CFOY4F7MZYUH/action/citation_signature","submit_replication":"https://pith.science/pith/AC55NK2YHHDSI4CFOY4F7MZYUH/action/replication_record"}},"created_at":"2026-07-05T10:09:53.631885+00:00","updated_at":"2026-07-05T10:09:53.631885+00:00"}