{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:3EG53AIGYEHDEAWPKCM3QMNPK4","short_pith_number":"pith:3EG53AIG","schema_version":"1.0","canonical_sha256":"d90ddd8106c10e3202cf5099b831af572ebe40b2dd91f40944f2babb56c02bae","source":{"kind":"arxiv","id":"1903.11591","version":2},"attestation_state":"computed","paper":{"title":"Vainshtein regime in Scalar-Tensor gravity: constraints on DHOST theories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Filippo Vernizzi, Marco Crisostomi, Matthew Lewandowski","submitted_at":"2019-03-27T17:58:19Z","abstract_excerpt":"We study the screening mechanism in the most general scalar-tensor theories that leave gravitational waves unaffected and are thus compatible with recent LIGO/Virgo observations. Using the effective field theory of dark energy approach, we consider the general action for perturbations beyond linear order, focussing on the quasi-static limit. When restricting to the subclass of theories that satisfy the gravitational wave constraints, the fully nonlinear effective Lagrangian contains only three independent parameters. One of these, $\\beta_1$, is uniquely present in degenerate higher-order theor"},"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":"1903.11591","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-03-27T17:58:19Z","cross_cats_sorted":["astro-ph.CO","hep-ph","hep-th"],"title_canon_sha256":"d36d4fd67b4915011dcac23bb306d039411b2561b40dbf3ce07fa088a9f569ed","abstract_canon_sha256":"d4ef2a026c5adbcce5a94332fd84cf4c6f34e27554c420912f79038f9adfd73a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:39:44.525420Z","signature_b64":"iAclGZupGl6E8fMIaJA844w8jBGRY6/GYrr8n1SY2mixnz1RyNtEJl5GDolKc5XpqNPmOs61FdxchEhkWBAyDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d90ddd8106c10e3202cf5099b831af572ebe40b2dd91f40944f2babb56c02bae","last_reissued_at":"2026-05-17T23:39:44.524680Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:39:44.524680Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Vainshtein regime in Scalar-Tensor gravity: constraints on DHOST theories","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Filippo Vernizzi, Marco Crisostomi, Matthew Lewandowski","submitted_at":"2019-03-27T17:58:19Z","abstract_excerpt":"We study the screening mechanism in the most general scalar-tensor theories that leave gravitational waves unaffected and are thus compatible with recent LIGO/Virgo observations. Using the effective field theory of dark energy approach, we consider the general action for perturbations beyond linear order, focussing on the quasi-static limit. When restricting to the subclass of theories that satisfy the gravitational wave constraints, the fully nonlinear effective Lagrangian contains only three independent parameters. One of these, $\\beta_1$, is uniquely present in degenerate higher-order theor"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1903.11591","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":"1903.11591","created_at":"2026-05-17T23:39:44.524807+00:00"},{"alias_kind":"arxiv_version","alias_value":"1903.11591v2","created_at":"2026-05-17T23:39:44.524807+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1903.11591","created_at":"2026-05-17T23:39:44.524807+00:00"},{"alias_kind":"pith_short_12","alias_value":"3EG53AIGYEHD","created_at":"2026-05-18T12:33:07.085635+00:00"},{"alias_kind":"pith_short_16","alias_value":"3EG53AIGYEHDEAWP","created_at":"2026-05-18T12:33:07.085635+00:00"},{"alias_kind":"pith_short_8","alias_value":"3EG53AIG","created_at":"2026-05-18T12:33:07.085635+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3EG53AIGYEHDEAWPKCM3QMNPK4","json":"https://pith.science/pith/3EG53AIGYEHDEAWPKCM3QMNPK4.json","graph_json":"https://pith.science/api/pith-number/3EG53AIGYEHDEAWPKCM3QMNPK4/graph.json","events_json":"https://pith.science/api/pith-number/3EG53AIGYEHDEAWPKCM3QMNPK4/events.json","paper":"https://pith.science/paper/3EG53AIG"},"agent_actions":{"view_html":"https://pith.science/pith/3EG53AIGYEHDEAWPKCM3QMNPK4","download_json":"https://pith.science/pith/3EG53AIGYEHDEAWPKCM3QMNPK4.json","view_paper":"https://pith.science/paper/3EG53AIG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1903.11591&json=true","fetch_graph":"https://pith.science/api/pith-number/3EG53AIGYEHDEAWPKCM3QMNPK4/graph.json","fetch_events":"https://pith.science/api/pith-number/3EG53AIGYEHDEAWPKCM3QMNPK4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3EG53AIGYEHDEAWPKCM3QMNPK4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3EG53AIGYEHDEAWPKCM3QMNPK4/action/storage_attestation","attest_author":"https://pith.science/pith/3EG53AIGYEHDEAWPKCM3QMNPK4/action/author_attestation","sign_citation":"https://pith.science/pith/3EG53AIGYEHDEAWPKCM3QMNPK4/action/citation_signature","submit_replication":"https://pith.science/pith/3EG53AIGYEHDEAWPKCM3QMNPK4/action/replication_record"}},"created_at":"2026-05-17T23:39:44.524807+00:00","updated_at":"2026-05-17T23:39:44.524807+00:00"}