{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1996:Z2AWM37MCGOYREFVNX46OHWICT","short_pith_number":"pith:Z2AWM37M","schema_version":"1.0","canonical_sha256":"ce81666fec119d8890b56df9e71ec814de4dd318b47a369c2ed3ca53c379f30f","source":{"kind":"arxiv","id":"gr-qc/9602056","version":1},"attestation_state":"computed","paper":{"title":"Tensor-scalar gravity and binary-pulsar experiments","license":"","headline":"","cross_cats":["astro-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Gilles Esposito-Farese, Thibault Damour","submitted_at":"1996-02-27T21:41:54Z","abstract_excerpt":"Some recently discovered nonperturbative strong-field effects in tensor-scalar theories of gravitation are interpreted as a scalar analog of ferromagnetism: \"spontaneous scalarization\". This phenomenon leads to very significant deviations from general relativity in conditions involving strong gravitational fields, notably binary-pulsar experiments. Contrary to solar-system experiments, these deviations do not necessarily vanish when the weak-field scalar coupling tends to zero. We compute the scalar \"form factors\" measuring these deviations, and notably a parameter entering the pulsar timing o"},"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":"gr-qc/9602056","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"1996-02-27T21:41:54Z","cross_cats_sorted":["astro-ph","hep-th"],"title_canon_sha256":"f354c55aae4b30b1b9ef530bf0393005954869c201050bf354cfa4ad648e784c","abstract_canon_sha256":"f70eb03c25afda8e1be943ad9613bc4e294a5d1722d03b14e04382ed86b720b3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:08:07.963228Z","signature_b64":"VHY0mHTa4qkvMbRfZSZiAdmDWMvwmEzu8ObURBhjAA3Cmw8qzvAectG6p9EHB5RfczIW/v2urh9cSvQPON8UAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ce81666fec119d8890b56df9e71ec814de4dd318b47a369c2ed3ca53c379f30f","last_reissued_at":"2026-05-18T01:08:07.962811Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:08:07.962811Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Tensor-scalar gravity and binary-pulsar experiments","license":"","headline":"","cross_cats":["astro-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Gilles Esposito-Farese, Thibault Damour","submitted_at":"1996-02-27T21:41:54Z","abstract_excerpt":"Some recently discovered nonperturbative strong-field effects in tensor-scalar theories of gravitation are interpreted as a scalar analog of ferromagnetism: \"spontaneous scalarization\". This phenomenon leads to very significant deviations from general relativity in conditions involving strong gravitational fields, notably binary-pulsar experiments. Contrary to solar-system experiments, these deviations do not necessarily vanish when the weak-field scalar coupling tends to zero. We compute the scalar \"form factors\" measuring these deviations, and notably a parameter entering the pulsar timing o"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/9602056","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":"gr-qc/9602056","created_at":"2026-05-18T01:08:07.962873+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/9602056v1","created_at":"2026-05-18T01:08:07.962873+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/9602056","created_at":"2026-05-18T01:08:07.962873+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z2AWM37MCGOY","created_at":"2026-05-18T12:25:48.327863+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z2AWM37MCGOYREFV","created_at":"2026-05-18T12:25:48.327863+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z2AWM37M","created_at":"2026-05-18T12:25:48.327863+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":9,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2505.20919","citing_title":"Scalarization and superradiant instability of black hole induced by dark matter halo in the scalar-tensor theory of gravity","ref_index":49,"is_internal_anchor":true},{"citing_arxiv_id":"1202.5809","citing_title":"Dynamical Boson Stars","ref_index":147,"is_internal_anchor":true},{"citing_arxiv_id":"1501.07274","citing_title":"Testing General Relativity with Present and Future Astrophysical Observations","ref_index":116,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25100","citing_title":"Thermodynamic Phase Transitions in Einstein-Maxwell-Scalar-Gauss-Bonnet Gravity","ref_index":43,"is_internal_anchor":false},{"citing_arxiv_id":"2604.24867","citing_title":"Underlying mechanisms of phase transitions in scalar-tensor theories","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2605.01436","citing_title":"Constraints on Einstein-aether gravity from the precision timing of PSR J1738+0333","ref_index":40,"is_internal_anchor":false},{"citing_arxiv_id":"2604.21298","citing_title":"Phase transition structure of scalarized neutron stars: the effect of rotation and linear coupling","ref_index":10,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13614","citing_title":"Scalarizations of magnetized Reissner-Nordstr\\\"om black holes induced by parity-violating and parity-preserving interactions","ref_index":4,"is_internal_anchor":false},{"citing_arxiv_id":"2503.12263","citing_title":"The Science of the Einstein Telescope","ref_index":194,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Z2AWM37MCGOYREFVNX46OHWICT","json":"https://pith.science/pith/Z2AWM37MCGOYREFVNX46OHWICT.json","graph_json":"https://pith.science/api/pith-number/Z2AWM37MCGOYREFVNX46OHWICT/graph.json","events_json":"https://pith.science/api/pith-number/Z2AWM37MCGOYREFVNX46OHWICT/events.json","paper":"https://pith.science/paper/Z2AWM37M"},"agent_actions":{"view_html":"https://pith.science/pith/Z2AWM37MCGOYREFVNX46OHWICT","download_json":"https://pith.science/pith/Z2AWM37MCGOYREFVNX46OHWICT.json","view_paper":"https://pith.science/paper/Z2AWM37M","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/9602056&json=true","fetch_graph":"https://pith.science/api/pith-number/Z2AWM37MCGOYREFVNX46OHWICT/graph.json","fetch_events":"https://pith.science/api/pith-number/Z2AWM37MCGOYREFVNX46OHWICT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z2AWM37MCGOYREFVNX46OHWICT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z2AWM37MCGOYREFVNX46OHWICT/action/storage_attestation","attest_author":"https://pith.science/pith/Z2AWM37MCGOYREFVNX46OHWICT/action/author_attestation","sign_citation":"https://pith.science/pith/Z2AWM37MCGOYREFVNX46OHWICT/action/citation_signature","submit_replication":"https://pith.science/pith/Z2AWM37MCGOYREFVNX46OHWICT/action/replication_record"}},"created_at":"2026-05-18T01:08:07.962873+00:00","updated_at":"2026-05-18T01:08:07.962873+00:00"}