{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7","short_pith_number":"pith:7YNQHJ7W","schema_version":"1.0","canonical_sha256":"fe1b03a7f680db9d92c6576f9de5e647c74f7bd6bd777cf37e1667721e1325e3","source":{"kind":"arxiv","id":"2403.13894","version":2},"attestation_state":"computed","paper":{"title":"Background-Induced Forces from Dark Relics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Sergio Barbosa, Sylvain Fichet","submitted_at":"2024-03-20T18:05:57Z","abstract_excerpt":"Light particles quadratically coupled to nucleons induce macroscopic forces in matter. While a quantum effect always exists, an additional force occurs in the presence of a finite density of the light particles. We compute and classify such background-induced forces for particles of spin $0,\\frac{1}{2},1$ in the framework of effective field theory. We show that, at short distance, the background-induced forces exhibit a universal behavior that depends solely on the moments of the phase space distribution function of the light particles. We compute the forces in the case of dark particles densi"},"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":"2403.13894","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2024-03-20T18:05:57Z","cross_cats_sorted":[],"title_canon_sha256":"1d4b169f1bc084b23813910ccbac941b12f109ee77028efbb43838d5036c8517","abstract_canon_sha256":"0ea0e010807fdf70647244259e2da781de31c743019c76f8df38e29e825e375a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:57:19.822343Z","signature_b64":"6ueSnhrV07HUi7oXjgRa0ZMpzT6b0W1b09BCZIVdtwi6YjbU1Th1/meHRwy3pAXg0Ua3z3mSWXjY4D/BHiK1CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fe1b03a7f680db9d92c6576f9de5e647c74f7bd6bd777cf37e1667721e1325e3","last_reissued_at":"2026-07-05T09:57:19.821877Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:57:19.821877Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Background-Induced Forces from Dark Relics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Sergio Barbosa, Sylvain Fichet","submitted_at":"2024-03-20T18:05:57Z","abstract_excerpt":"Light particles quadratically coupled to nucleons induce macroscopic forces in matter. While a quantum effect always exists, an additional force occurs in the presence of a finite density of the light particles. We compute and classify such background-induced forces for particles of spin $0,\\frac{1}{2},1$ in the framework of effective field theory. We show that, at short distance, the background-induced forces exhibit a universal behavior that depends solely on the moments of the phase space distribution function of the light particles. We compute the forces in the case of dark particles densi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2403.13894","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2403.13894/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":"2403.13894","created_at":"2026-07-05T09:57:19.821934+00:00"},{"alias_kind":"arxiv_version","alias_value":"2403.13894v2","created_at":"2026-07-05T09:57:19.821934+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2403.13894","created_at":"2026-07-05T09:57:19.821934+00:00"},{"alias_kind":"pith_short_12","alias_value":"7YNQHJ7WQDNZ","created_at":"2026-07-05T09:57:19.821934+00:00"},{"alias_kind":"pith_short_16","alias_value":"7YNQHJ7WQDNZ3EWG","created_at":"2026-07-05T09:57:19.821934+00:00"},{"alias_kind":"pith_short_8","alias_value":"7YNQHJ7W","created_at":"2026-07-05T09:57:19.821934+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.07008","citing_title":"Macroscopic Quantum Interference in Dark Matter Wave Scattering with MICROSCOPE","ref_index":42,"is_internal_anchor":false},{"citing_arxiv_id":"2606.28491","citing_title":"A directional force template for quadratically coupled ultralight dark matter","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2606.28481","citing_title":"Background-Induced Forces from Quadratically Coupled Ultralight Dark Matter","ref_index":87,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7","json":"https://pith.science/pith/7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7.json","graph_json":"https://pith.science/api/pith-number/7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7/graph.json","events_json":"https://pith.science/api/pith-number/7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7/events.json","paper":"https://pith.science/paper/7YNQHJ7W"},"agent_actions":{"view_html":"https://pith.science/pith/7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7","download_json":"https://pith.science/pith/7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7.json","view_paper":"https://pith.science/paper/7YNQHJ7W","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2403.13894&json=true","fetch_graph":"https://pith.science/api/pith-number/7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7/graph.json","fetch_events":"https://pith.science/api/pith-number/7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7/action/storage_attestation","attest_author":"https://pith.science/pith/7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7/action/author_attestation","sign_citation":"https://pith.science/pith/7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7/action/citation_signature","submit_replication":"https://pith.science/pith/7YNQHJ7WQDNZ3EWGK5XZ3ZPGI7/action/replication_record"}},"created_at":"2026-07-05T09:57:19.821934+00:00","updated_at":"2026-07-05T09:57:19.821934+00:00"}