{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:GFBF4NNPOYLSS76RZKTPL3AUDT","short_pith_number":"pith:GFBF4NNP","schema_version":"1.0","canonical_sha256":"31425e35af7617297fd1caa6f5ec141cc18ddde8fd230f43b097b9e762d40b5f","source":{"kind":"arxiv","id":"2501.11569","version":2},"attestation_state":"computed","paper":{"title":"Blazar Boosted ALP and vector portal Dark matter confronting light mediator searches","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Sk Jeesun","submitted_at":"2025-01-20T16:18:51Z","abstract_excerpt":"The trouble in detecting low mass dark matter due to its low kinetic energy can be ameliorated in the boosted dark matter framework, where a sub-population of galactic dark matter attains very high energy after being up-scattered by energetic standard model particles. However, in such a scenario the upper limits on the cross-section obtained hitherto are typically large. Hence in the minimal extension of standard model where new mediators act as a portal between the dark and visible sectors, the direct detection limits for sub-GeV dark matter might lie within the exclusion region of other grou"},"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":"2501.11569","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2025-01-20T16:18:51Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"02a93575aa752501963bcf9d92bfbc352425d6e407d8bfdd0f6a72e823e9c19d","abstract_canon_sha256":"3ac70bffe67aa15c4527f09a164e1c32d3ff083b8865deead1c80228d824e419"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:52:57.761441Z","signature_b64":"8PzbFG0OfPbSujuele7xpP1nCj1jO3rP5epwDIoDF8/r7UAi1L3+V5aJPHKz5AONGvvGpCPoyuis9DUL54GxBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"31425e35af7617297fd1caa6f5ec141cc18ddde8fd230f43b097b9e762d40b5f","last_reissued_at":"2026-07-05T10:52:57.760950Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:52:57.760950Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Blazar Boosted ALP and vector portal Dark matter confronting light mediator searches","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Sk Jeesun","submitted_at":"2025-01-20T16:18:51Z","abstract_excerpt":"The trouble in detecting low mass dark matter due to its low kinetic energy can be ameliorated in the boosted dark matter framework, where a sub-population of galactic dark matter attains very high energy after being up-scattered by energetic standard model particles. However, in such a scenario the upper limits on the cross-section obtained hitherto are typically large. Hence in the minimal extension of standard model where new mediators act as a portal between the dark and visible sectors, the direct detection limits for sub-GeV dark matter might lie within the exclusion region of other grou"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.11569","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/2501.11569/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":"2501.11569","created_at":"2026-07-05T10:52:57.761009+00:00"},{"alias_kind":"arxiv_version","alias_value":"2501.11569v2","created_at":"2026-07-05T10:52:57.761009+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2501.11569","created_at":"2026-07-05T10:52:57.761009+00:00"},{"alias_kind":"pith_short_12","alias_value":"GFBF4NNPOYLS","created_at":"2026-07-05T10:52:57.761009+00:00"},{"alias_kind":"pith_short_16","alias_value":"GFBF4NNPOYLSS76R","created_at":"2026-07-05T10:52:57.761009+00:00"},{"alias_kind":"pith_short_8","alias_value":"GFBF4NNP","created_at":"2026-07-05T10:52:57.761009+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2602.04858","citing_title":"Primordial black holes as cosmic accelerators of light dark matter: Novel direct detection constraints","ref_index":86,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GFBF4NNPOYLSS76RZKTPL3AUDT","json":"https://pith.science/pith/GFBF4NNPOYLSS76RZKTPL3AUDT.json","graph_json":"https://pith.science/api/pith-number/GFBF4NNPOYLSS76RZKTPL3AUDT/graph.json","events_json":"https://pith.science/api/pith-number/GFBF4NNPOYLSS76RZKTPL3AUDT/events.json","paper":"https://pith.science/paper/GFBF4NNP"},"agent_actions":{"view_html":"https://pith.science/pith/GFBF4NNPOYLSS76RZKTPL3AUDT","download_json":"https://pith.science/pith/GFBF4NNPOYLSS76RZKTPL3AUDT.json","view_paper":"https://pith.science/paper/GFBF4NNP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2501.11569&json=true","fetch_graph":"https://pith.science/api/pith-number/GFBF4NNPOYLSS76RZKTPL3AUDT/graph.json","fetch_events":"https://pith.science/api/pith-number/GFBF4NNPOYLSS76RZKTPL3AUDT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GFBF4NNPOYLSS76RZKTPL3AUDT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GFBF4NNPOYLSS76RZKTPL3AUDT/action/storage_attestation","attest_author":"https://pith.science/pith/GFBF4NNPOYLSS76RZKTPL3AUDT/action/author_attestation","sign_citation":"https://pith.science/pith/GFBF4NNPOYLSS76RZKTPL3AUDT/action/citation_signature","submit_replication":"https://pith.science/pith/GFBF4NNPOYLSS76RZKTPL3AUDT/action/replication_record"}},"created_at":"2026-07-05T10:52:57.761009+00:00","updated_at":"2026-07-05T10:52:57.761009+00:00"}