{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:X3OONFST6KMG4E2XDSLRARQJ2C","short_pith_number":"pith:X3OONFST","schema_version":"1.0","canonical_sha256":"bedce69653f2986e13571c97104609d08eb2174ae562688797740d0545d3b9af","source":{"kind":"arxiv","id":"1807.04512","version":3},"attestation_state":"computed","paper":{"title":"Violation of the equivalence principle from light scalar dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","physics.atom-ph"],"primary_cat":"gr-qc","authors_text":"A. Hees, E. Savalle, O. Minazzoli, P. Wolf, Y. V. Stadnik","submitted_at":"2018-07-12T10:14:54Z","abstract_excerpt":"In this paper, we study the local observational consequences of a violation of the Einstein Equivalence Principle induced by models of light scalar Dark Matter (DM). We focus on two different models where the scalar field couples linearly or quadratically to the standard model of matter fields. For both these cases, we derive the solutions of the scalar field. We also derive from first principles the expressions for two types of observables: (i) the local comparison of two atomic sensors that are differently sensitive to the constants of Nature and (ii) the local differential acceleration betw"},"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":"1807.04512","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-07-12T10:14:54Z","cross_cats_sorted":["hep-ph","physics.atom-ph"],"title_canon_sha256":"1903af13c0db30fc1bc0a063757466e0d8f3e1874a9673bb1449e0168a44da32","abstract_canon_sha256":"82fea28ee518a820c3cc877f8b9cbab58bbab7cc65e7292643bba010b65e339f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:04:16.593635Z","signature_b64":"ieSH/BbKcH0PRT6il3c+4vP5GExDnfaMgGD3k+ZYrEGvpIFaNwRELQl1tY1E6YWxj4R0RYNa9BLgg3uYKDAwAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bedce69653f2986e13571c97104609d08eb2174ae562688797740d0545d3b9af","last_reissued_at":"2026-05-18T00:04:16.592981Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:04:16.592981Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Violation of the equivalence principle from light scalar dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","physics.atom-ph"],"primary_cat":"gr-qc","authors_text":"A. Hees, E. Savalle, O. Minazzoli, P. Wolf, Y. V. Stadnik","submitted_at":"2018-07-12T10:14:54Z","abstract_excerpt":"In this paper, we study the local observational consequences of a violation of the Einstein Equivalence Principle induced by models of light scalar Dark Matter (DM). We focus on two different models where the scalar field couples linearly or quadratically to the standard model of matter fields. For both these cases, we derive the solutions of the scalar field. We also derive from first principles the expressions for two types of observables: (i) the local comparison of two atomic sensors that are differently sensitive to the constants of Nature and (ii) the local differential acceleration betw"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1807.04512","kind":"arxiv","version":3},"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":"1807.04512","created_at":"2026-05-18T00:04:16.593062+00:00"},{"alias_kind":"arxiv_version","alias_value":"1807.04512v3","created_at":"2026-05-18T00:04:16.593062+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1807.04512","created_at":"2026-05-18T00:04:16.593062+00:00"},{"alias_kind":"pith_short_12","alias_value":"X3OONFST6KMG","created_at":"2026-05-18T12:33:01.666342+00:00"},{"alias_kind":"pith_short_16","alias_value":"X3OONFST6KMG4E2X","created_at":"2026-05-18T12:33:01.666342+00:00"},{"alias_kind":"pith_short_8","alias_value":"X3OONFST","created_at":"2026-05-18T12:33:01.666342+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2405.06744","citing_title":"Nelson-Barr ultralight dark matter","ref_index":30,"is_internal_anchor":true},{"citing_arxiv_id":"2509.25305","citing_title":"$\\phi$-Dwarfs: White Dwarfs probe Quadratically Coupled Scalars","ref_index":27,"is_internal_anchor":true},{"citing_arxiv_id":"2512.13816","citing_title":"Stellar Superradiance and Low-Energy Absorption in Dense Nuclear Media","ref_index":106,"is_internal_anchor":true},{"citing_arxiv_id":"2605.03477","citing_title":"Self-Interaction Bounds on Ultralight Dark Matter Couplings to Matter","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2604.23879","citing_title":"Searching for ultralight bosons with Josephson junction interferometry","ref_index":53,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/X3OONFST6KMG4E2XDSLRARQJ2C","json":"https://pith.science/pith/X3OONFST6KMG4E2XDSLRARQJ2C.json","graph_json":"https://pith.science/api/pith-number/X3OONFST6KMG4E2XDSLRARQJ2C/graph.json","events_json":"https://pith.science/api/pith-number/X3OONFST6KMG4E2XDSLRARQJ2C/events.json","paper":"https://pith.science/paper/X3OONFST"},"agent_actions":{"view_html":"https://pith.science/pith/X3OONFST6KMG4E2XDSLRARQJ2C","download_json":"https://pith.science/pith/X3OONFST6KMG4E2XDSLRARQJ2C.json","view_paper":"https://pith.science/paper/X3OONFST","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1807.04512&json=true","fetch_graph":"https://pith.science/api/pith-number/X3OONFST6KMG4E2XDSLRARQJ2C/graph.json","fetch_events":"https://pith.science/api/pith-number/X3OONFST6KMG4E2XDSLRARQJ2C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/X3OONFST6KMG4E2XDSLRARQJ2C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/X3OONFST6KMG4E2XDSLRARQJ2C/action/storage_attestation","attest_author":"https://pith.science/pith/X3OONFST6KMG4E2XDSLRARQJ2C/action/author_attestation","sign_citation":"https://pith.science/pith/X3OONFST6KMG4E2XDSLRARQJ2C/action/citation_signature","submit_replication":"https://pith.science/pith/X3OONFST6KMG4E2XDSLRARQJ2C/action/replication_record"}},"created_at":"2026-05-18T00:04:16.593062+00:00","updated_at":"2026-05-18T00:04:16.593062+00:00"}