{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:ZHLBXD6KLL76FNAUQBIQKEONLO","short_pith_number":"pith:ZHLBXD6K","schema_version":"1.0","canonical_sha256":"c9d61b8fca5affe2b41480510511cd5b842416caf62ddb9803c8d79434f6ece0","source":{"kind":"arxiv","id":"1612.03110","version":1},"attestation_state":"computed","paper":{"title":"Indirect Signals from Solar Dark Matter Annihilation to Long-lived Right-handed Neutrinos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Bradley Knockel, Rouzbeh Allahverdi, Shashank Shalgar, Yu Gao","submitted_at":"2016-12-09T18:00:41Z","abstract_excerpt":"We study indirect detection signals from solar annihilation of dark matter (DM) particles into light right-handed (RH) neutrinos with a mass in a $1-5$ GeV range. These RH neutrinos can have a sufficiently long lifetime to allow them to decay outside the Sun and their delayed decays can result in a signal in gamma rays from the otherwise `dark' solar direction, and also a neutrino signal that is not suppressed by the interactions with solar medium. We find that the latest Fermi-LAT and IceCube results place limits on the gamma ray and neutrino signals, respectively. Combined photon and neutrin"},"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":"1612.03110","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2016-12-09T18:00:41Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"624ee45ebce3ee90e0d384ccb75180e15d5dd7611e6f00c4528aa03f2a83f091","abstract_canon_sha256":"809602168f50971a171813c2ffeea44cc1878f8d1865618731aef6df3d891257"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:46:38.592753Z","signature_b64":"7SJ8KO/1nL7U/1+Jou8NzYZdSdQrTYgM/c89uAVChVLGIqwRS1fu+Tlr4MEUJ84Zf1Jwc9456yWayNaKVvWOCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c9d61b8fca5affe2b41480510511cd5b842416caf62ddb9803c8d79434f6ece0","last_reissued_at":"2026-05-18T00:46:38.592179Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:46:38.592179Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Indirect Signals from Solar Dark Matter Annihilation to Long-lived Right-handed Neutrinos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Bradley Knockel, Rouzbeh Allahverdi, Shashank Shalgar, Yu Gao","submitted_at":"2016-12-09T18:00:41Z","abstract_excerpt":"We study indirect detection signals from solar annihilation of dark matter (DM) particles into light right-handed (RH) neutrinos with a mass in a $1-5$ GeV range. These RH neutrinos can have a sufficiently long lifetime to allow them to decay outside the Sun and their delayed decays can result in a signal in gamma rays from the otherwise `dark' solar direction, and also a neutrino signal that is not suppressed by the interactions with solar medium. We find that the latest Fermi-LAT and IceCube results place limits on the gamma ray and neutrino signals, respectively. Combined photon and neutrin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.03110","kind":"arxiv","version":1},"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":"1612.03110","created_at":"2026-05-18T00:46:38.592275+00:00"},{"alias_kind":"arxiv_version","alias_value":"1612.03110v1","created_at":"2026-05-18T00:46:38.592275+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.03110","created_at":"2026-05-18T00:46:38.592275+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZHLBXD6KLL76","created_at":"2026-05-18T12:30:53.716459+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZHLBXD6KLL76FNAU","created_at":"2026-05-18T12:30:53.716459+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZHLBXD6K","created_at":"2026-05-18T12:30:53.716459+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1908.09796","citing_title":"Structures of the Massive Vector Boson Propagators at Finite Temperature Illuminated by the Goldstone Equivalence Gauge","ref_index":36,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZHLBXD6KLL76FNAUQBIQKEONLO","json":"https://pith.science/pith/ZHLBXD6KLL76FNAUQBIQKEONLO.json","graph_json":"https://pith.science/api/pith-number/ZHLBXD6KLL76FNAUQBIQKEONLO/graph.json","events_json":"https://pith.science/api/pith-number/ZHLBXD6KLL76FNAUQBIQKEONLO/events.json","paper":"https://pith.science/paper/ZHLBXD6K"},"agent_actions":{"view_html":"https://pith.science/pith/ZHLBXD6KLL76FNAUQBIQKEONLO","download_json":"https://pith.science/pith/ZHLBXD6KLL76FNAUQBIQKEONLO.json","view_paper":"https://pith.science/paper/ZHLBXD6K","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1612.03110&json=true","fetch_graph":"https://pith.science/api/pith-number/ZHLBXD6KLL76FNAUQBIQKEONLO/graph.json","fetch_events":"https://pith.science/api/pith-number/ZHLBXD6KLL76FNAUQBIQKEONLO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZHLBXD6KLL76FNAUQBIQKEONLO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZHLBXD6KLL76FNAUQBIQKEONLO/action/storage_attestation","attest_author":"https://pith.science/pith/ZHLBXD6KLL76FNAUQBIQKEONLO/action/author_attestation","sign_citation":"https://pith.science/pith/ZHLBXD6KLL76FNAUQBIQKEONLO/action/citation_signature","submit_replication":"https://pith.science/pith/ZHLBXD6KLL76FNAUQBIQKEONLO/action/replication_record"}},"created_at":"2026-05-18T00:46:38.592275+00:00","updated_at":"2026-05-18T00:46:38.592275+00:00"}