{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:7CXVFUBX5HJJC4JDNMINT5VR4V","short_pith_number":"pith:7CXVFUBX","schema_version":"1.0","canonical_sha256":"f8af52d037e9d29171236b10d9f6b1e56c17c0ce3a0fe3c0238893a5cc3d2d47","source":{"kind":"arxiv","id":"1711.10769","version":1},"attestation_state":"computed","paper":{"title":"On the motion of hairy black holes in Einstein-Maxwell-dilaton theories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"F\\'elix-Louis Juli\\'e","submitted_at":"2017-11-29T11:00:43Z","abstract_excerpt":"Starting from the static, spherically symmetric black hole solutions in massless Einstein-Maxwell-dilaton (EMD) theories, we build a \"skeleton\" action, that is, we phenomenologically replace black holes by an appropriate effective point particle action, which is well suited to the formal treatment of the many-body problem in EMD theories. We find that, depending crucially on the value of their scalar cosmological environment, black holes can undergo steep \"scalarization\" transitions, inducing large deviations to the general relativistic two-body dynamics, as shown, for example, when computing "},"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":"1711.10769","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2017-11-29T11:00:43Z","cross_cats_sorted":[],"title_canon_sha256":"62fd0aa6d4527e5df684c30018511c2f357475404e371a568d1a1ee8b068ee9d","abstract_canon_sha256":"e26bd66dafa854246bbad75d66424292c6e891f3eeff8d3509b517d616643c62"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:24:48.033868Z","signature_b64":"nAkxfkWDjkOFq7nZibPHiPjWKTPji9si3nGPE21N7EcPB4x5jn+QMu35OIuY36UmAI/M7W8/PrjpXpayGIU6DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f8af52d037e9d29171236b10d9f6b1e56c17c0ce3a0fe3c0238893a5cc3d2d47","last_reissued_at":"2026-05-18T00:24:48.033338Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:24:48.033338Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the motion of hairy black holes in Einstein-Maxwell-dilaton theories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"F\\'elix-Louis Juli\\'e","submitted_at":"2017-11-29T11:00:43Z","abstract_excerpt":"Starting from the static, spherically symmetric black hole solutions in massless Einstein-Maxwell-dilaton (EMD) theories, we build a \"skeleton\" action, that is, we phenomenologically replace black holes by an appropriate effective point particle action, which is well suited to the formal treatment of the many-body problem in EMD theories. We find that, depending crucially on the value of their scalar cosmological environment, black holes can undergo steep \"scalarization\" transitions, inducing large deviations to the general relativistic two-body dynamics, as shown, for example, when computing "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.10769","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":""},"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":"1711.10769","created_at":"2026-05-18T00:24:48.033427+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.10769v1","created_at":"2026-05-18T00:24:48.033427+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.10769","created_at":"2026-05-18T00:24:48.033427+00:00"},{"alias_kind":"pith_short_12","alias_value":"7CXVFUBX5HJJ","created_at":"2026-05-18T12:31:03.183658+00:00"},{"alias_kind":"pith_short_16","alias_value":"7CXVFUBX5HJJC4JD","created_at":"2026-05-18T12:31:03.183658+00:00"},{"alias_kind":"pith_short_8","alias_value":"7CXVFUBX","created_at":"2026-05-18T12:31:03.183658+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2606.24215","citing_title":"Nonlinear Stability of Kerr-Sen Black Holes in Merging Binaries","ref_index":43,"is_internal_anchor":true},{"citing_arxiv_id":"2310.19679","citing_title":"Tidal effects up to next-to-next-to leading post-Newtonian order in massless scalar-tensor theories","ref_index":26,"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":46,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7CXVFUBX5HJJC4JDNMINT5VR4V","json":"https://pith.science/pith/7CXVFUBX5HJJC4JDNMINT5VR4V.json","graph_json":"https://pith.science/api/pith-number/7CXVFUBX5HJJC4JDNMINT5VR4V/graph.json","events_json":"https://pith.science/api/pith-number/7CXVFUBX5HJJC4JDNMINT5VR4V/events.json","paper":"https://pith.science/paper/7CXVFUBX"},"agent_actions":{"view_html":"https://pith.science/pith/7CXVFUBX5HJJC4JDNMINT5VR4V","download_json":"https://pith.science/pith/7CXVFUBX5HJJC4JDNMINT5VR4V.json","view_paper":"https://pith.science/paper/7CXVFUBX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.10769&json=true","fetch_graph":"https://pith.science/api/pith-number/7CXVFUBX5HJJC4JDNMINT5VR4V/graph.json","fetch_events":"https://pith.science/api/pith-number/7CXVFUBX5HJJC4JDNMINT5VR4V/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7CXVFUBX5HJJC4JDNMINT5VR4V/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7CXVFUBX5HJJC4JDNMINT5VR4V/action/storage_attestation","attest_author":"https://pith.science/pith/7CXVFUBX5HJJC4JDNMINT5VR4V/action/author_attestation","sign_citation":"https://pith.science/pith/7CXVFUBX5HJJC4JDNMINT5VR4V/action/citation_signature","submit_replication":"https://pith.science/pith/7CXVFUBX5HJJC4JDNMINT5VR4V/action/replication_record"}},"created_at":"2026-05-18T00:24:48.033427+00:00","updated_at":"2026-05-18T00:24:48.033427+00:00"}