{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:QCADRRQPYDZXROYAT3AH5KHCUH","short_pith_number":"pith:QCADRRQP","schema_version":"1.0","canonical_sha256":"808038c60fc0f378bb009ec07ea8e2a1f552bb09ff07fac9dc24d01946d117c2","source":{"kind":"arxiv","id":"1208.5481","version":2},"attestation_state":"computed","paper":{"title":"Gamma Ray Signals from Dark Matter: Concepts, Status and Prospects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Christoph Weniger, Torsten Bringmann","submitted_at":"2012-08-27T20:00:00Z","abstract_excerpt":"Weakly interacting massive particles (WIMPs) remain a prime candidate for the cosmological dark matter (DM), even in the absence of current collider signals that would unambiguously point to new physics below the TeV scale. The self-annihilation of these particles in astronomical targets may leave observable imprints in cosmic rays of various kinds. In this review, we focus on gamma rays which we argue to play a pronounced role among the various possible messengers. We discuss the most promising spectral and spatial signatures to look for, give an update on the current state of gamma-ray searc"},"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":"1208.5481","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2012-08-27T20:00:00Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE"],"title_canon_sha256":"217812384e2a4d15084be916db87cdd4269104196a1d37255571e4b85796a8bd","abstract_canon_sha256":"8b4592965b915fe2de46a9888674adf86585fe6917da99a720b3b409c0c8de71"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:38:32.767973Z","signature_b64":"L2YQVtByXri0W92t2mJUDzjtULAzvl4d+BMftLjzzX6E5Q/3rkxBFNdJX0BCo+zCisLR2/svo8U9UvzFZs3NAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"808038c60fc0f378bb009ec07ea8e2a1f552bb09ff07fac9dc24d01946d117c2","last_reissued_at":"2026-05-18T03:38:32.767478Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:38:32.767478Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gamma Ray Signals from Dark Matter: Concepts, Status and Prospects","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Christoph Weniger, Torsten Bringmann","submitted_at":"2012-08-27T20:00:00Z","abstract_excerpt":"Weakly interacting massive particles (WIMPs) remain a prime candidate for the cosmological dark matter (DM), even in the absence of current collider signals that would unambiguously point to new physics below the TeV scale. The self-annihilation of these particles in astronomical targets may leave observable imprints in cosmic rays of various kinds. In this review, we focus on gamma rays which we argue to play a pronounced role among the various possible messengers. We discuss the most promising spectral and spatial signatures to look for, give an update on the current state of gamma-ray searc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1208.5481","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":""},"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":"1208.5481","created_at":"2026-05-18T03:38:32.767552+00:00"},{"alias_kind":"arxiv_version","alias_value":"1208.5481v2","created_at":"2026-05-18T03:38:32.767552+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1208.5481","created_at":"2026-05-18T03:38:32.767552+00:00"},{"alias_kind":"pith_short_12","alias_value":"QCADRRQPYDZX","created_at":"2026-05-18T12:27:18.751474+00:00"},{"alias_kind":"pith_short_16","alias_value":"QCADRRQPYDZXROYA","created_at":"2026-05-18T12:27:18.751474+00:00"},{"alias_kind":"pith_short_8","alias_value":"QCADRRQP","created_at":"2026-05-18T12:27:18.751474+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.26072","citing_title":"Caught in the Cosmic Web: Environmental Impacts on the Halo Substructure Boosts to Dark Matter Annihilation Signals","ref_index":7,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18674","citing_title":"Hunting Sterile Neutrino Dark Matter in the MeV Gap","ref_index":107,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QCADRRQPYDZXROYAT3AH5KHCUH","json":"https://pith.science/pith/QCADRRQPYDZXROYAT3AH5KHCUH.json","graph_json":"https://pith.science/api/pith-number/QCADRRQPYDZXROYAT3AH5KHCUH/graph.json","events_json":"https://pith.science/api/pith-number/QCADRRQPYDZXROYAT3AH5KHCUH/events.json","paper":"https://pith.science/paper/QCADRRQP"},"agent_actions":{"view_html":"https://pith.science/pith/QCADRRQPYDZXROYAT3AH5KHCUH","download_json":"https://pith.science/pith/QCADRRQPYDZXROYAT3AH5KHCUH.json","view_paper":"https://pith.science/paper/QCADRRQP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1208.5481&json=true","fetch_graph":"https://pith.science/api/pith-number/QCADRRQPYDZXROYAT3AH5KHCUH/graph.json","fetch_events":"https://pith.science/api/pith-number/QCADRRQPYDZXROYAT3AH5KHCUH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QCADRRQPYDZXROYAT3AH5KHCUH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QCADRRQPYDZXROYAT3AH5KHCUH/action/storage_attestation","attest_author":"https://pith.science/pith/QCADRRQPYDZXROYAT3AH5KHCUH/action/author_attestation","sign_citation":"https://pith.science/pith/QCADRRQPYDZXROYAT3AH5KHCUH/action/citation_signature","submit_replication":"https://pith.science/pith/QCADRRQPYDZXROYAT3AH5KHCUH/action/replication_record"}},"created_at":"2026-05-18T03:38:32.767552+00:00","updated_at":"2026-05-18T03:38:32.767552+00:00"}