{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:SGTZ6PAOOWD2UDW2FO7A3HUQ4U","short_pith_number":"pith:SGTZ6PAO","schema_version":"1.0","canonical_sha256":"91a79f3c0e7587aa0eda2bbe0d9e90e5384df97bce3e93944561ade3d1704534","source":{"kind":"arxiv","id":"1610.04612","version":2},"attestation_state":"computed","paper":{"title":"Dark Matter interpretation of low energy IceCube MESE excess","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"G. Miele, M. Chianese, S. Morisi","submitted_at":"2016-10-14T20:00:00Z","abstract_excerpt":"The 2-years MESE IceCube events show a slightly excess in the energy range 10-100 TeV with a maximum local statistical significance of 2.3$\\sigma$, once a hard astrophysical power-law is assumed. A spectral index smaller than 2.2 is indeed suggested by multi-messenger studies related to $p$-$p$ sources and by the recent IceCube analysis regarding 6-years up-going muon neutrinos. In the present paper, we propose a two-components scenario where the extraterrestrial neutrinos are explained in terms of an astrophysical power-law and a Dark Matter signal. We consider both decaying and annihilating "},"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":"1610.04612","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2016-10-14T20:00:00Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE"],"title_canon_sha256":"6ad2a5dd83c3995f3ac3ec79d79e178163eec3e3fe7107e957845b420eb22dbe","abstract_canon_sha256":"b3cc6a9b22d0ec12d9711bce2d194d070779c0ae597880aada3c60c20f2b2c0c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:53:29.907785Z","signature_b64":"2jkxC/HOONgKKlP7Tuuh8Ci7g3Ih9fo4IOZhbfclHdXHF75c66iRwv0+datXD1/lYBnuIEyNBuhkhDHHSHcHBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"91a79f3c0e7587aa0eda2bbe0d9e90e5384df97bce3e93944561ade3d1704534","last_reissued_at":"2026-05-18T00:53:29.907331Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:53:29.907331Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark Matter interpretation of low energy IceCube MESE excess","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"G. Miele, M. Chianese, S. Morisi","submitted_at":"2016-10-14T20:00:00Z","abstract_excerpt":"The 2-years MESE IceCube events show a slightly excess in the energy range 10-100 TeV with a maximum local statistical significance of 2.3$\\sigma$, once a hard astrophysical power-law is assumed. A spectral index smaller than 2.2 is indeed suggested by multi-messenger studies related to $p$-$p$ sources and by the recent IceCube analysis regarding 6-years up-going muon neutrinos. In the present paper, we propose a two-components scenario where the extraterrestrial neutrinos are explained in terms of an astrophysical power-law and a Dark Matter signal. We consider both decaying and annihilating "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.04612","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":"1610.04612","created_at":"2026-05-18T00:53:29.907395+00:00"},{"alias_kind":"arxiv_version","alias_value":"1610.04612v2","created_at":"2026-05-18T00:53:29.907395+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.04612","created_at":"2026-05-18T00:53:29.907395+00:00"},{"alias_kind":"pith_short_12","alias_value":"SGTZ6PAOOWD2","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_16","alias_value":"SGTZ6PAOOWD2UDW2","created_at":"2026-05-18T12:30:44.179134+00:00"},{"alias_kind":"pith_short_8","alias_value":"SGTZ6PAO","created_at":"2026-05-18T12:30:44.179134+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1907.11926","citing_title":"Potential Dark Matter Signals at Neutrino Telescopes","ref_index":26,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SGTZ6PAOOWD2UDW2FO7A3HUQ4U","json":"https://pith.science/pith/SGTZ6PAOOWD2UDW2FO7A3HUQ4U.json","graph_json":"https://pith.science/api/pith-number/SGTZ6PAOOWD2UDW2FO7A3HUQ4U/graph.json","events_json":"https://pith.science/api/pith-number/SGTZ6PAOOWD2UDW2FO7A3HUQ4U/events.json","paper":"https://pith.science/paper/SGTZ6PAO"},"agent_actions":{"view_html":"https://pith.science/pith/SGTZ6PAOOWD2UDW2FO7A3HUQ4U","download_json":"https://pith.science/pith/SGTZ6PAOOWD2UDW2FO7A3HUQ4U.json","view_paper":"https://pith.science/paper/SGTZ6PAO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1610.04612&json=true","fetch_graph":"https://pith.science/api/pith-number/SGTZ6PAOOWD2UDW2FO7A3HUQ4U/graph.json","fetch_events":"https://pith.science/api/pith-number/SGTZ6PAOOWD2UDW2FO7A3HUQ4U/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SGTZ6PAOOWD2UDW2FO7A3HUQ4U/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SGTZ6PAOOWD2UDW2FO7A3HUQ4U/action/storage_attestation","attest_author":"https://pith.science/pith/SGTZ6PAOOWD2UDW2FO7A3HUQ4U/action/author_attestation","sign_citation":"https://pith.science/pith/SGTZ6PAOOWD2UDW2FO7A3HUQ4U/action/citation_signature","submit_replication":"https://pith.science/pith/SGTZ6PAOOWD2UDW2FO7A3HUQ4U/action/replication_record"}},"created_at":"2026-05-18T00:53:29.907395+00:00","updated_at":"2026-05-18T00:53:29.907395+00:00"}