{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:BLJTVKDTL2JJ7PYSKKHF32XY63","short_pith_number":"pith:BLJTVKDT","schema_version":"1.0","canonical_sha256":"0ad33aa8735e929fbf12528e5deaf8f6e4889b9760e2a8f771bbb83cb46927ce","source":{"kind":"arxiv","id":"1904.09994","version":2},"attestation_state":"computed","paper":{"title":"Luminous Signals of Inelastic Dark Matter in Large Detectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Graham D. Kribs, Joshua Eby, Patrick J. Fox, Roni Harnik","submitted_at":"2019-04-22T18:00:02Z","abstract_excerpt":"We study luminous dark matter signals in models with inelastic scattering. Dark matter $\\chi_1$ that scatters inelastically off elements in the Earth is kicked into an excited state $\\chi_2$ that can subsequently decay into a monoenergetic photon inside a detector. The photon signal exhibits large sidereal-daily modulation due to the daily rotation of the Earth and anisotropies in the problem: the dark matter wind comes from the direction of Cygnus due to the Sun's motion relative to the galaxy, and the rock overburden is anisotropic, as is the dark matter scattering angle. This allows outstan"},"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":"1904.09994","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2019-04-22T18:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"e2a07eebe67478119294a1dc73f5e6e2ec9fbbb8e685e3eb365f8101a993ba76","abstract_canon_sha256":"3f6031dda6b26aac2f9a7109cc7c07580f7b8c3041bedeb0e43f66918a93844f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:13:44.993760Z","signature_b64":"bKRXwg1e/8jGCxShS9t34tBeugY5eB3v5XOUB5xOtDK0Mxuh6eQDMP1eITUHIuQCRPG/DmodSoVEZx7sG0keDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0ad33aa8735e929fbf12528e5deaf8f6e4889b9760e2a8f771bbb83cb46927ce","last_reissued_at":"2026-07-05T00:13:44.993336Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:13:44.993336Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Luminous Signals of Inelastic Dark Matter in Large Detectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Graham D. Kribs, Joshua Eby, Patrick J. Fox, Roni Harnik","submitted_at":"2019-04-22T18:00:02Z","abstract_excerpt":"We study luminous dark matter signals in models with inelastic scattering. Dark matter $\\chi_1$ that scatters inelastically off elements in the Earth is kicked into an excited state $\\chi_2$ that can subsequently decay into a monoenergetic photon inside a detector. The photon signal exhibits large sidereal-daily modulation due to the daily rotation of the Earth and anisotropies in the problem: the dark matter wind comes from the direction of Cygnus due to the Sun's motion relative to the galaxy, and the rock overburden is anisotropic, as is the dark matter scattering angle. This allows outstan"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1904.09994","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/1904.09994/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":"1904.09994","created_at":"2026-07-05T00:13:44.993394+00:00"},{"alias_kind":"arxiv_version","alias_value":"1904.09994v2","created_at":"2026-07-05T00:13:44.993394+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1904.09994","created_at":"2026-07-05T00:13:44.993394+00:00"},{"alias_kind":"pith_short_12","alias_value":"BLJTVKDTL2JJ","created_at":"2026-07-05T00:13:44.993394+00:00"},{"alias_kind":"pith_short_16","alias_value":"BLJTVKDTL2JJ7PYS","created_at":"2026-07-05T00:13:44.993394+00:00"},{"alias_kind":"pith_short_8","alias_value":"BLJTVKDT","created_at":"2026-07-05T00:13:44.993394+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.05299","citing_title":"Heavy-element paleodetectors for Higgsino dark matter","ref_index":28,"is_internal_anchor":false},{"citing_arxiv_id":"2606.30760","citing_title":"Rich Phenomenology from Simple Ingredients: A Review of Confining Dark Sectors","ref_index":285,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BLJTVKDTL2JJ7PYSKKHF32XY63","json":"https://pith.science/pith/BLJTVKDTL2JJ7PYSKKHF32XY63.json","graph_json":"https://pith.science/api/pith-number/BLJTVKDTL2JJ7PYSKKHF32XY63/graph.json","events_json":"https://pith.science/api/pith-number/BLJTVKDTL2JJ7PYSKKHF32XY63/events.json","paper":"https://pith.science/paper/BLJTVKDT"},"agent_actions":{"view_html":"https://pith.science/pith/BLJTVKDTL2JJ7PYSKKHF32XY63","download_json":"https://pith.science/pith/BLJTVKDTL2JJ7PYSKKHF32XY63.json","view_paper":"https://pith.science/paper/BLJTVKDT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1904.09994&json=true","fetch_graph":"https://pith.science/api/pith-number/BLJTVKDTL2JJ7PYSKKHF32XY63/graph.json","fetch_events":"https://pith.science/api/pith-number/BLJTVKDTL2JJ7PYSKKHF32XY63/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BLJTVKDTL2JJ7PYSKKHF32XY63/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BLJTVKDTL2JJ7PYSKKHF32XY63/action/storage_attestation","attest_author":"https://pith.science/pith/BLJTVKDTL2JJ7PYSKKHF32XY63/action/author_attestation","sign_citation":"https://pith.science/pith/BLJTVKDTL2JJ7PYSKKHF32XY63/action/citation_signature","submit_replication":"https://pith.science/pith/BLJTVKDTL2JJ7PYSKKHF32XY63/action/replication_record"}},"created_at":"2026-07-05T00:13:44.993394+00:00","updated_at":"2026-07-05T00:13:44.993394+00:00"}