{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:UJRSEK77RNTCEBRUSULM6MR2OG","short_pith_number":"pith:UJRSEK77","schema_version":"1.0","canonical_sha256":"a263222bff8b662206349516cf323a718ed9f486a880e8fc67af645df749f40c","source":{"kind":"arxiv","id":"2012.13406","version":2},"attestation_state":"computed","paper":{"title":"Etching Plastic Searches for Dark Matter","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Amit Bhoonah, Brian Courtman, Joseph Bramante, Ningqiang Song","submitted_at":"2020-12-24T19:00:00Z","abstract_excerpt":"Large panels of etched plastic, situated aboard the Skylab Space Station and inside the Ohya quarry near Tokyo, have been used to set limits on fluxes of cosmogenic particles. These plastic particle track detectors also provide the best sensitivity for some heavy dark matter that interacts strongly with nuclei. We revisit prior dark matter bounds from Skylab, and incorporate geometry-dependent thresholds, a halo velocity distribution, and a complete accounting of observed through-going particle fluxes. These considerations reduce the Skylab bound's mass range by a few orders of magnitude. Howe"},"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":"2012.13406","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2020-12-24T19:00:00Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"fb8a5aa8170e18b7142e17cd77947ea5d6234d4890da12f78759659980296cda","abstract_canon_sha256":"8f4f21c2e3aedab13b583bc9d14e56ab144e6acc0136eeb9f1833f6b80b88333"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:41:30.525697Z","signature_b64":"AtH/RtJPG4vRbR+M3dlqCdUCYcTHAaj1rzIcyQCabAI9oA7BLpfc2G8387l4mJZGsHddF4Cf+MmSJroQkFegAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a263222bff8b662206349516cf323a718ed9f486a880e8fc67af645df749f40c","last_reissued_at":"2026-07-05T02:41:30.525138Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:41:30.525138Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Etching Plastic Searches for Dark Matter","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Amit Bhoonah, Brian Courtman, Joseph Bramante, Ningqiang Song","submitted_at":"2020-12-24T19:00:00Z","abstract_excerpt":"Large panels of etched plastic, situated aboard the Skylab Space Station and inside the Ohya quarry near Tokyo, have been used to set limits on fluxes of cosmogenic particles. These plastic particle track detectors also provide the best sensitivity for some heavy dark matter that interacts strongly with nuclei. We revisit prior dark matter bounds from Skylab, and incorporate geometry-dependent thresholds, a halo velocity distribution, and a complete accounting of observed through-going particle fluxes. These considerations reduce the Skylab bound's mass range by a few orders of magnitude. Howe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2012.13406","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/2012.13406/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":"2012.13406","created_at":"2026-07-05T02:41:30.525198+00:00"},{"alias_kind":"arxiv_version","alias_value":"2012.13406v2","created_at":"2026-07-05T02:41:30.525198+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2012.13406","created_at":"2026-07-05T02:41:30.525198+00:00"},{"alias_kind":"pith_short_12","alias_value":"UJRSEK77RNTC","created_at":"2026-07-05T02:41:30.525198+00:00"},{"alias_kind":"pith_short_16","alias_value":"UJRSEK77RNTCEBRU","created_at":"2026-07-05T02:41:30.525198+00:00"},{"alias_kind":"pith_short_8","alias_value":"UJRSEK77","created_at":"2026-07-05T02:41:30.525198+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.02579","citing_title":"New Windows on Heavy Dark Matter: Mineral Melt Modelling and X-Ray Readout for Muscovite Mica","ref_index":74,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UJRSEK77RNTCEBRUSULM6MR2OG","json":"https://pith.science/pith/UJRSEK77RNTCEBRUSULM6MR2OG.json","graph_json":"https://pith.science/api/pith-number/UJRSEK77RNTCEBRUSULM6MR2OG/graph.json","events_json":"https://pith.science/api/pith-number/UJRSEK77RNTCEBRUSULM6MR2OG/events.json","paper":"https://pith.science/paper/UJRSEK77"},"agent_actions":{"view_html":"https://pith.science/pith/UJRSEK77RNTCEBRUSULM6MR2OG","download_json":"https://pith.science/pith/UJRSEK77RNTCEBRUSULM6MR2OG.json","view_paper":"https://pith.science/paper/UJRSEK77","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2012.13406&json=true","fetch_graph":"https://pith.science/api/pith-number/UJRSEK77RNTCEBRUSULM6MR2OG/graph.json","fetch_events":"https://pith.science/api/pith-number/UJRSEK77RNTCEBRUSULM6MR2OG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UJRSEK77RNTCEBRUSULM6MR2OG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UJRSEK77RNTCEBRUSULM6MR2OG/action/storage_attestation","attest_author":"https://pith.science/pith/UJRSEK77RNTCEBRUSULM6MR2OG/action/author_attestation","sign_citation":"https://pith.science/pith/UJRSEK77RNTCEBRUSULM6MR2OG/action/citation_signature","submit_replication":"https://pith.science/pith/UJRSEK77RNTCEBRUSULM6MR2OG/action/replication_record"}},"created_at":"2026-07-05T02:41:30.525198+00:00","updated_at":"2026-07-05T02:41:30.525198+00:00"}