{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:PUA2Q3TJ3VPKHOIPPX5ZOECB2T","short_pith_number":"pith:PUA2Q3TJ","schema_version":"1.0","canonical_sha256":"7d01a86e69dd5ea3b90f7dfb971041d4e3d17438714eb34c32446e2896bd1e0e","source":{"kind":"arxiv","id":"1704.08258","version":2},"attestation_state":"computed","paper":{"title":"Probing dark matter annihilation in the Galaxy with antiprotons and gamma rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Alessandro Cuoco, Jan Heisig, Michael Korsmeier, Michael Kr\\\"amer","submitted_at":"2017-04-26T18:00:01Z","abstract_excerpt":"A possible hint of dark matter annihilation has been found in Cuoco, Korsmeier and Kr\\\"amer (2017) from an analysis of recent cosmic-ray antiproton data from AMS-02 and taking into account cosmic-ray propagation uncertainties by fitting at the same time dark matter and propagation parameters. Here, we extend this analysis to a wider class of annihilation channels. We find consistent hints of a dark matter signal with an annihilation cross-section close to the thermal value and with masses in range between 40 and 130 GeV depending on the annihilation channel. Furthermore, we investigate in how "},"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":"1704.08258","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-04-26T18:00:01Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"aed6b70abed408afe650da58a9e09a24330849a159928d8044537494a073c341","abstract_canon_sha256":"c4dd28963b5ffb5400ed24ea6bf9d176a9fdee6aab8f5d760ae20cb50372f0cc"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:31:21.737858Z","signature_b64":"9w+y8LUTk14UoL40esZnMEk5E9d4476Jk3JAtLOmjToO2A2aZKHQTo8WD++qT69STgKQrRhGffkKLxKrYdXgDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7d01a86e69dd5ea3b90f7dfb971041d4e3d17438714eb34c32446e2896bd1e0e","last_reissued_at":"2026-05-18T00:31:21.737257Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:31:21.737257Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing dark matter annihilation in the Galaxy with antiprotons and gamma rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Alessandro Cuoco, Jan Heisig, Michael Korsmeier, Michael Kr\\\"amer","submitted_at":"2017-04-26T18:00:01Z","abstract_excerpt":"A possible hint of dark matter annihilation has been found in Cuoco, Korsmeier and Kr\\\"amer (2017) from an analysis of recent cosmic-ray antiproton data from AMS-02 and taking into account cosmic-ray propagation uncertainties by fitting at the same time dark matter and propagation parameters. Here, we extend this analysis to a wider class of annihilation channels. We find consistent hints of a dark matter signal with an annihilation cross-section close to the thermal value and with masses in range between 40 and 130 GeV depending on the annihilation channel. Furthermore, we investigate in how "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.08258","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":"1704.08258","created_at":"2026-05-18T00:31:21.737345+00:00"},{"alias_kind":"arxiv_version","alias_value":"1704.08258v2","created_at":"2026-05-18T00:31:21.737345+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.08258","created_at":"2026-05-18T00:31:21.737345+00:00"},{"alias_kind":"pith_short_12","alias_value":"PUA2Q3TJ3VPK","created_at":"2026-05-18T12:31:37.085036+00:00"},{"alias_kind":"pith_short_16","alias_value":"PUA2Q3TJ3VPKHOIP","created_at":"2026-05-18T12:31:37.085036+00:00"},{"alias_kind":"pith_short_8","alias_value":"PUA2Q3TJ","created_at":"2026-05-18T12:31:37.085036+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"1807.06209","citing_title":"Planck 2018 results. VI. Cosmological parameters","ref_index":89,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PUA2Q3TJ3VPKHOIPPX5ZOECB2T","json":"https://pith.science/pith/PUA2Q3TJ3VPKHOIPPX5ZOECB2T.json","graph_json":"https://pith.science/api/pith-number/PUA2Q3TJ3VPKHOIPPX5ZOECB2T/graph.json","events_json":"https://pith.science/api/pith-number/PUA2Q3TJ3VPKHOIPPX5ZOECB2T/events.json","paper":"https://pith.science/paper/PUA2Q3TJ"},"agent_actions":{"view_html":"https://pith.science/pith/PUA2Q3TJ3VPKHOIPPX5ZOECB2T","download_json":"https://pith.science/pith/PUA2Q3TJ3VPKHOIPPX5ZOECB2T.json","view_paper":"https://pith.science/paper/PUA2Q3TJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1704.08258&json=true","fetch_graph":"https://pith.science/api/pith-number/PUA2Q3TJ3VPKHOIPPX5ZOECB2T/graph.json","fetch_events":"https://pith.science/api/pith-number/PUA2Q3TJ3VPKHOIPPX5ZOECB2T/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PUA2Q3TJ3VPKHOIPPX5ZOECB2T/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PUA2Q3TJ3VPKHOIPPX5ZOECB2T/action/storage_attestation","attest_author":"https://pith.science/pith/PUA2Q3TJ3VPKHOIPPX5ZOECB2T/action/author_attestation","sign_citation":"https://pith.science/pith/PUA2Q3TJ3VPKHOIPPX5ZOECB2T/action/citation_signature","submit_replication":"https://pith.science/pith/PUA2Q3TJ3VPKHOIPPX5ZOECB2T/action/replication_record"}},"created_at":"2026-05-18T00:31:21.737345+00:00","updated_at":"2026-05-18T00:31:21.737345+00:00"}