{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:3XPVS77DH3KSXXRB4LM3NM7OSI","short_pith_number":"pith:3XPVS77D","schema_version":"1.0","canonical_sha256":"dddf597fe33ed52bde21e2d9b6b3ee922556e96a871765b2c896b90e382dfd07","source":{"kind":"arxiv","id":"1712.04901","version":4},"attestation_state":"computed","paper":{"title":"Earth-Scattering of super-heavy Dark Matter: updated constraints from detectors old and new","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Bradley J. Kavanagh","submitted_at":"2017-12-13T18:14:00Z","abstract_excerpt":"Direct searches for Dark Matter (DM) are continuously improving, probing down to lower and lower DM-nucleon interaction cross sections. For strongly-interacting massive particle (SIMP) Dark Matter, however, the accessible cross section is bounded from above due to the stopping effect of the atmosphere, Earth and detector shielding. We present a careful calculation of the SIMP signal rate, focusing on super-heavy DM ($m_\\chi \\gtrsim 10^5 \\,\\,\\mathrm{GeV}$) for which the standard nuclear-stopping formalism is applicable, and provide code for implementing this calculation numerically. With recent"},"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":"1712.04901","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2017-12-13T18:14:00Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"b8b6c0b4cbd83c69b93c9b3a86475ac3eb9d9b984072ebdbdfb77ce53bf7a699","abstract_canon_sha256":"b4ead8ffc60f8e243f8e263b5caf1f23005adc4266d5eeb867275df58abb2614"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:11:57.673763Z","signature_b64":"KkOgZDQLp/mz/z6dkcpKFaNgdntMsR6Oi3nMOCk7VSUWkYRNtEnXKR6imsJzK5lwN/0O4BTSBGg7qAcShx8TDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"dddf597fe33ed52bde21e2d9b6b3ee922556e96a871765b2c896b90e382dfd07","last_reissued_at":"2026-05-18T00:11:57.673108Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:11:57.673108Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Earth-Scattering of super-heavy Dark Matter: updated constraints from detectors old and new","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Bradley J. Kavanagh","submitted_at":"2017-12-13T18:14:00Z","abstract_excerpt":"Direct searches for Dark Matter (DM) are continuously improving, probing down to lower and lower DM-nucleon interaction cross sections. For strongly-interacting massive particle (SIMP) Dark Matter, however, the accessible cross section is bounded from above due to the stopping effect of the atmosphere, Earth and detector shielding. We present a careful calculation of the SIMP signal rate, focusing on super-heavy DM ($m_\\chi \\gtrsim 10^5 \\,\\,\\mathrm{GeV}$) for which the standard nuclear-stopping formalism is applicable, and provide code for implementing this calculation numerically. With recent"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1712.04901","kind":"arxiv","version":4},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"1712.04901","created_at":"2026-05-18T00:11:57.673212+00:00"},{"alias_kind":"arxiv_version","alias_value":"1712.04901v4","created_at":"2026-05-18T00:11:57.673212+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1712.04901","created_at":"2026-05-18T00:11:57.673212+00:00"},{"alias_kind":"pith_short_12","alias_value":"3XPVS77DH3KS","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_16","alias_value":"3XPVS77DH3KSXXRB","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_8","alias_value":"3XPVS77D","created_at":"2026-05-18T12:30:58.224056+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2503.03683","citing_title":"First Limits on Light Dark Matter Interactions in a Low Threshold Two Channel Athermal Phonon Detector from the TESSERACT Collaboration","ref_index":42,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3XPVS77DH3KSXXRB4LM3NM7OSI","json":"https://pith.science/pith/3XPVS77DH3KSXXRB4LM3NM7OSI.json","graph_json":"https://pith.science/api/pith-number/3XPVS77DH3KSXXRB4LM3NM7OSI/graph.json","events_json":"https://pith.science/api/pith-number/3XPVS77DH3KSXXRB4LM3NM7OSI/events.json","paper":"https://pith.science/paper/3XPVS77D"},"agent_actions":{"view_html":"https://pith.science/pith/3XPVS77DH3KSXXRB4LM3NM7OSI","download_json":"https://pith.science/pith/3XPVS77DH3KSXXRB4LM3NM7OSI.json","view_paper":"https://pith.science/paper/3XPVS77D","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1712.04901&json=true","fetch_graph":"https://pith.science/api/pith-number/3XPVS77DH3KSXXRB4LM3NM7OSI/graph.json","fetch_events":"https://pith.science/api/pith-number/3XPVS77DH3KSXXRB4LM3NM7OSI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3XPVS77DH3KSXXRB4LM3NM7OSI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3XPVS77DH3KSXXRB4LM3NM7OSI/action/storage_attestation","attest_author":"https://pith.science/pith/3XPVS77DH3KSXXRB4LM3NM7OSI/action/author_attestation","sign_citation":"https://pith.science/pith/3XPVS77DH3KSXXRB4LM3NM7OSI/action/citation_signature","submit_replication":"https://pith.science/pith/3XPVS77DH3KSXXRB4LM3NM7OSI/action/replication_record"}},"created_at":"2026-05-18T00:11:57.673212+00:00","updated_at":"2026-05-18T00:11:57.673212+00:00"}