{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:GQQRULPCQZ4E46FFUQZQRKXYOS","short_pith_number":"pith:GQQRULPC","schema_version":"1.0","canonical_sha256":"34211a2de286784e78a5a43308aaf8748008b2bc47a85569488a2867a040a2d1","source":{"kind":"arxiv","id":"2501.15476","version":2},"attestation_state":"computed","paper":{"title":"Microscopic composite systems bound by strong gravity in extra dimensions as candidates for dark matter","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","nucl-th","physics.atom-ph"],"primary_cat":"hep-ph","authors_text":"V. V. Flambaum","submitted_at":"2025-01-26T10:42:53Z","abstract_excerpt":"In the Arkani-Hamed-Dimopoulos-Dvali (ADD) model with n extra compactified dimensions, the gravitational potential scales as 1/r^{n+1} and becomes significantly stronger at short distances. We investigate the possibility of forming small-sized composite systems of Standard Model particles bound by this potential. Such bound states, composed of quarks, neutrinos, axions, or other particles, exhibit a small cross-section-to-mass ratio, making them viable candidates for dark matter."},"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":"2501.15476","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2025-01-26T10:42:53Z","cross_cats_sorted":["astro-ph.CO","nucl-th","physics.atom-ph"],"title_canon_sha256":"e87408db57b57223a861bf6f8d74c8cf6608d8fdbd746aae61df0848d7888b84","abstract_canon_sha256":"e18ea8dda91ae56e190ed0376e6c64bfe769fa7017331a95a2518a26cf501d8d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:30:41.009149Z","signature_b64":"eyxYcVj00JY2C0Ntee+1rZsCvLwMAfMtPAqqZigsOSGDzVwDZli/ZlaW51IF1w2oI+ooWCBVlWTICpgwhjzuAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"34211a2de286784e78a5a43308aaf8748008b2bc47a85569488a2867a040a2d1","last_reissued_at":"2026-07-05T11:30:41.008633Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:30:41.008633Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Microscopic composite systems bound by strong gravity in extra dimensions as candidates for dark matter","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","nucl-th","physics.atom-ph"],"primary_cat":"hep-ph","authors_text":"V. V. Flambaum","submitted_at":"2025-01-26T10:42:53Z","abstract_excerpt":"In the Arkani-Hamed-Dimopoulos-Dvali (ADD) model with n extra compactified dimensions, the gravitational potential scales as 1/r^{n+1} and becomes significantly stronger at short distances. We investigate the possibility of forming small-sized composite systems of Standard Model particles bound by this potential. Such bound states, composed of quarks, neutrinos, axions, or other particles, exhibit a small cross-section-to-mass ratio, making them viable candidates for dark matter."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.15476","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/2501.15476/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":"2501.15476","created_at":"2026-07-05T11:30:41.008694+00:00"},{"alias_kind":"arxiv_version","alias_value":"2501.15476v2","created_at":"2026-07-05T11:30:41.008694+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2501.15476","created_at":"2026-07-05T11:30:41.008694+00:00"},{"alias_kind":"pith_short_12","alias_value":"GQQRULPCQZ4E","created_at":"2026-07-05T11:30:41.008694+00:00"},{"alias_kind":"pith_short_16","alias_value":"GQQRULPCQZ4E46FF","created_at":"2026-07-05T11:30:41.008694+00:00"},{"alias_kind":"pith_short_8","alias_value":"GQQRULPC","created_at":"2026-07-05T11:30:41.008694+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.23178","citing_title":"Signatures of gravity-mediated dark matter interaction in theories with large extra dimensions","ref_index":21,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GQQRULPCQZ4E46FFUQZQRKXYOS","json":"https://pith.science/pith/GQQRULPCQZ4E46FFUQZQRKXYOS.json","graph_json":"https://pith.science/api/pith-number/GQQRULPCQZ4E46FFUQZQRKXYOS/graph.json","events_json":"https://pith.science/api/pith-number/GQQRULPCQZ4E46FFUQZQRKXYOS/events.json","paper":"https://pith.science/paper/GQQRULPC"},"agent_actions":{"view_html":"https://pith.science/pith/GQQRULPCQZ4E46FFUQZQRKXYOS","download_json":"https://pith.science/pith/GQQRULPCQZ4E46FFUQZQRKXYOS.json","view_paper":"https://pith.science/paper/GQQRULPC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2501.15476&json=true","fetch_graph":"https://pith.science/api/pith-number/GQQRULPCQZ4E46FFUQZQRKXYOS/graph.json","fetch_events":"https://pith.science/api/pith-number/GQQRULPCQZ4E46FFUQZQRKXYOS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GQQRULPCQZ4E46FFUQZQRKXYOS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GQQRULPCQZ4E46FFUQZQRKXYOS/action/storage_attestation","attest_author":"https://pith.science/pith/GQQRULPCQZ4E46FFUQZQRKXYOS/action/author_attestation","sign_citation":"https://pith.science/pith/GQQRULPCQZ4E46FFUQZQRKXYOS/action/citation_signature","submit_replication":"https://pith.science/pith/GQQRULPCQZ4E46FFUQZQRKXYOS/action/replication_record"}},"created_at":"2026-07-05T11:30:41.008694+00:00","updated_at":"2026-07-05T11:30:41.008694+00:00"}