{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:I445VFMJVOETJIQ7MNFGPJXG4C","short_pith_number":"pith:I445VFMJ","schema_version":"1.0","canonical_sha256":"4739da9589ab8934a21f634a67a6e6e0988e40e8caacb9987d03a0031235d7e2","source":{"kind":"arxiv","id":"1909.00654","version":3},"attestation_state":"computed","paper":{"title":"Dark Matter Signals on a Laser Interferometer","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Masaki Mori, Nobuyuki Kanda, Satoshi Tsuchida, Yousuke Itoh","submitted_at":"2019-09-02T10:38:27Z","abstract_excerpt":"WIMPs are promising dark matter candidates. A WIMP occasionally collides with a mirror equipped with interferometric gravitational wave detectors such as LIGO, Virgo, KAGRA and the Einstein Telescope (ET). When WIMPs collide with a mirror of an interferometer, we expect that characteristic motions of the pendulum and mirror are excited, and those signals could be extracted by highly sophisticated sensors developed for gravitational wave detection. We analyze the motions of the pendulum and mirror, and estimate the detectability of these motions. For the \"Thin-ET\" detector, the signal-to-noise "},"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":"1909.00654","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-09-02T10:38:27Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"0c9625f84d2ec2e7f121ef50ba6a283c3c279c5488bcd4c6e3e7dc3e145d52c6","abstract_canon_sha256":"2043529a6934e555c1a1c0ced59847aeda3606e088e4d82933c4c1782db246a6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:46:32.239281Z","signature_b64":"rNmziv+Jj+JCkX0DGCjhIJsJEDN9jWIQJVcBQw6W6W0H5HiXJ8I/ITZV/Cf1xAfjY3HRXjRiA7Hg7xFL+oBPDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4739da9589ab8934a21f634a67a6e6e0988e40e8caacb9987d03a0031235d7e2","last_reissued_at":"2026-07-05T00:46:32.238826Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:46:32.238826Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark Matter Signals on a Laser Interferometer","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Masaki Mori, Nobuyuki Kanda, Satoshi Tsuchida, Yousuke Itoh","submitted_at":"2019-09-02T10:38:27Z","abstract_excerpt":"WIMPs are promising dark matter candidates. A WIMP occasionally collides with a mirror equipped with interferometric gravitational wave detectors such as LIGO, Virgo, KAGRA and the Einstein Telescope (ET). When WIMPs collide with a mirror of an interferometer, we expect that characteristic motions of the pendulum and mirror are excited, and those signals could be extracted by highly sophisticated sensors developed for gravitational wave detection. We analyze the motions of the pendulum and mirror, and estimate the detectability of these motions. For the \"Thin-ET\" detector, the signal-to-noise "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1909.00654","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1909.00654/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":"1909.00654","created_at":"2026-07-05T00:46:32.238887+00:00"},{"alias_kind":"arxiv_version","alias_value":"1909.00654v3","created_at":"2026-07-05T00:46:32.238887+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1909.00654","created_at":"2026-07-05T00:46:32.238887+00:00"},{"alias_kind":"pith_short_12","alias_value":"I445VFMJVOET","created_at":"2026-07-05T00:46:32.238887+00:00"},{"alias_kind":"pith_short_16","alias_value":"I445VFMJVOETJIQ7","created_at":"2026-07-05T00:46:32.238887+00:00"},{"alias_kind":"pith_short_8","alias_value":"I445VFMJ","created_at":"2026-07-05T00:46:32.238887+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.11144","citing_title":"Synchronization Induced by Ultralight Dark Matter","ref_index":8,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/I445VFMJVOETJIQ7MNFGPJXG4C","json":"https://pith.science/pith/I445VFMJVOETJIQ7MNFGPJXG4C.json","graph_json":"https://pith.science/api/pith-number/I445VFMJVOETJIQ7MNFGPJXG4C/graph.json","events_json":"https://pith.science/api/pith-number/I445VFMJVOETJIQ7MNFGPJXG4C/events.json","paper":"https://pith.science/paper/I445VFMJ"},"agent_actions":{"view_html":"https://pith.science/pith/I445VFMJVOETJIQ7MNFGPJXG4C","download_json":"https://pith.science/pith/I445VFMJVOETJIQ7MNFGPJXG4C.json","view_paper":"https://pith.science/paper/I445VFMJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1909.00654&json=true","fetch_graph":"https://pith.science/api/pith-number/I445VFMJVOETJIQ7MNFGPJXG4C/graph.json","fetch_events":"https://pith.science/api/pith-number/I445VFMJVOETJIQ7MNFGPJXG4C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I445VFMJVOETJIQ7MNFGPJXG4C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I445VFMJVOETJIQ7MNFGPJXG4C/action/storage_attestation","attest_author":"https://pith.science/pith/I445VFMJVOETJIQ7MNFGPJXG4C/action/author_attestation","sign_citation":"https://pith.science/pith/I445VFMJVOETJIQ7MNFGPJXG4C/action/citation_signature","submit_replication":"https://pith.science/pith/I445VFMJVOETJIQ7MNFGPJXG4C/action/replication_record"}},"created_at":"2026-07-05T00:46:32.238887+00:00","updated_at":"2026-07-05T00:46:32.238887+00:00"}