{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:HWHS6PBVSX66ZA5FUEGTJNHSVE","short_pith_number":"pith:HWHS6PBV","schema_version":"1.0","canonical_sha256":"3d8f2f3c3595fdec83a5a10d34b4f2a9194a540b2064fe04d2bcb20c200e2531","source":{"kind":"arxiv","id":"2210.03749","version":1},"attestation_state":"computed","paper":{"title":"New Constraints on Dark Matter and Cosmic Neutrino Profiles through Gravity","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-ex","hep-th"],"primary_cat":"hep-ph","authors_text":"Davide Farnocchia, Jason Arakawa, Joshua Eby, Marianna S. Safronova, Yu-Dai Tsai","submitted_at":"2022-10-07T18:00:00Z","abstract_excerpt":"We derive purely gravitational constraints on dark matter and cosmic neutrino profiles in the solar system using asteroid (101955) Bennu. We focus on Bennu because of its extensive tracking data and high-fidelity trajectory modeling resulting from the OSIRIS-REx mission. We find that the local density of dark matter is bound by $\\rho_{\\rm DM}\\lesssim 3.3\\times 10^{-15}\\;\\rm kg/m^3 \\simeq 6\\times10^6\\,\\bar{\\rho}_{\\rm DM}$, in the vicinity of $\\sim 1.1$ au (where $\\bar{\\rho}_{\\rm DM}\\simeq 0.3\\;\\rm GeV/cm^3$). We show that high-precision tracking data of solar system objects can constrain cosmic"},"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":"2210.03749","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","primary_cat":"hep-ph","submitted_at":"2022-10-07T18:00:00Z","cross_cats_sorted":["astro-ph.CO","gr-qc","hep-ex","hep-th"],"title_canon_sha256":"dcb815939197bead5b4a621846c08a23135f115309c991f2bbe9041eeb563bd8","abstract_canon_sha256":"892608d83f788863e109d9ae69927c5d747b983172d576e57ec50aaede51649d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:53:46.025121Z","signature_b64":"53x5750wbKy/42yLO6M8zWgd63oyJMdnP8vAsHL2gO4tZJMrD8yCTI7Ai6uqKqHmBe0se4LBnjEiE2yP1uoHAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3d8f2f3c3595fdec83a5a10d34b4f2a9194a540b2064fe04d2bcb20c200e2531","last_reissued_at":"2026-07-05T07:53:46.024521Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:53:46.024521Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"New Constraints on Dark Matter and Cosmic Neutrino Profiles through Gravity","license":"http://creativecommons.org/licenses/by-nc-sa/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-ex","hep-th"],"primary_cat":"hep-ph","authors_text":"Davide Farnocchia, Jason Arakawa, Joshua Eby, Marianna S. Safronova, Yu-Dai Tsai","submitted_at":"2022-10-07T18:00:00Z","abstract_excerpt":"We derive purely gravitational constraints on dark matter and cosmic neutrino profiles in the solar system using asteroid (101955) Bennu. We focus on Bennu because of its extensive tracking data and high-fidelity trajectory modeling resulting from the OSIRIS-REx mission. We find that the local density of dark matter is bound by $\\rho_{\\rm DM}\\lesssim 3.3\\times 10^{-15}\\;\\rm kg/m^3 \\simeq 6\\times10^6\\,\\bar{\\rho}_{\\rm DM}$, in the vicinity of $\\sim 1.1$ au (where $\\bar{\\rho}_{\\rm DM}\\simeq 0.3\\;\\rm GeV/cm^3$). We show that high-precision tracking data of solar system objects can constrain cosmic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2210.03749","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2210.03749/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":"2210.03749","created_at":"2026-07-05T07:53:46.024622+00:00"},{"alias_kind":"arxiv_version","alias_value":"2210.03749v1","created_at":"2026-07-05T07:53:46.024622+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2210.03749","created_at":"2026-07-05T07:53:46.024622+00:00"},{"alias_kind":"pith_short_12","alias_value":"HWHS6PBVSX66","created_at":"2026-07-05T07:53:46.024622+00:00"},{"alias_kind":"pith_short_16","alias_value":"HWHS6PBVSX66ZA5F","created_at":"2026-07-05T07:53:46.024622+00:00"},{"alias_kind":"pith_short_8","alias_value":"HWHS6PBV","created_at":"2026-07-05T07:53:46.024622+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2607.00072","citing_title":"Precision Solar System Dynamics for Ultralight Dark Matter Search","ref_index":28,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HWHS6PBVSX66ZA5FUEGTJNHSVE","json":"https://pith.science/pith/HWHS6PBVSX66ZA5FUEGTJNHSVE.json","graph_json":"https://pith.science/api/pith-number/HWHS6PBVSX66ZA5FUEGTJNHSVE/graph.json","events_json":"https://pith.science/api/pith-number/HWHS6PBVSX66ZA5FUEGTJNHSVE/events.json","paper":"https://pith.science/paper/HWHS6PBV"},"agent_actions":{"view_html":"https://pith.science/pith/HWHS6PBVSX66ZA5FUEGTJNHSVE","download_json":"https://pith.science/pith/HWHS6PBVSX66ZA5FUEGTJNHSVE.json","view_paper":"https://pith.science/paper/HWHS6PBV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2210.03749&json=true","fetch_graph":"https://pith.science/api/pith-number/HWHS6PBVSX66ZA5FUEGTJNHSVE/graph.json","fetch_events":"https://pith.science/api/pith-number/HWHS6PBVSX66ZA5FUEGTJNHSVE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HWHS6PBVSX66ZA5FUEGTJNHSVE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HWHS6PBVSX66ZA5FUEGTJNHSVE/action/storage_attestation","attest_author":"https://pith.science/pith/HWHS6PBVSX66ZA5FUEGTJNHSVE/action/author_attestation","sign_citation":"https://pith.science/pith/HWHS6PBVSX66ZA5FUEGTJNHSVE/action/citation_signature","submit_replication":"https://pith.science/pith/HWHS6PBVSX66ZA5FUEGTJNHSVE/action/replication_record"}},"created_at":"2026-07-05T07:53:46.024622+00:00","updated_at":"2026-07-05T07:53:46.024622+00:00"}