{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:CIOWI2HHNBV7IVB4LXGK6XIJXC","short_pith_number":"pith:CIOWI2HH","schema_version":"1.0","canonical_sha256":"121d6468e7686bf4543c5dccaf5d09b8a47537fa655731b3606a31467289ded6","source":{"kind":"arxiv","id":"2211.05996","version":1},"attestation_state":"computed","paper":{"title":"Sterile Neutrinos from Dark Matter: A $\\nu$ Nightmare?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Bibhushan Shakya, Logan Morrison, Stefano Profumo","submitted_at":"2022-11-11T04:41:24Z","abstract_excerpt":"We provide a comprehensive study of observable spectra from dark matter pair-annihilation or decay into sterile (right-handed) neutrinos. This occurs, for instance, in neutrino portal dark matter models, where a sterile neutrino acts as the portal between dark matter and the Standard Model sector. The subsequent decays of right-handed neutrinos produce detectable Standard Model particles, notably photons, positrons, and neutrinos. We study the phenomenology of models where the right-handed neutrino masses are below the GeV scale, as well as models where they are at, or significantly heavier th"},"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":"2211.05996","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2022-11-11T04:41:24Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"b41bc3620849d5e760ee9fc9c5b835fac6118b802f231296ee063b494233c95f","abstract_canon_sha256":"363f5f75d781395e25cb0e7efa7de68f314c1f7792b8a8152f29c74a3619806f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:15:16.017393Z","signature_b64":"pZrvIP1dXKAKn9nHK2B2IkrKNtmIFeRix1ObMl0v8iVq2gSAWreidgWVRKST/zl59d/YtRShIOC3sGWaas0aCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"121d6468e7686bf4543c5dccaf5d09b8a47537fa655731b3606a31467289ded6","last_reissued_at":"2026-07-05T05:15:16.017018Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:15:16.017018Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Sterile Neutrinos from Dark Matter: A $\\nu$ Nightmare?","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Bibhushan Shakya, Logan Morrison, Stefano Profumo","submitted_at":"2022-11-11T04:41:24Z","abstract_excerpt":"We provide a comprehensive study of observable spectra from dark matter pair-annihilation or decay into sterile (right-handed) neutrinos. This occurs, for instance, in neutrino portal dark matter models, where a sterile neutrino acts as the portal between dark matter and the Standard Model sector. The subsequent decays of right-handed neutrinos produce detectable Standard Model particles, notably photons, positrons, and neutrinos. We study the phenomenology of models where the right-handed neutrino masses are below the GeV scale, as well as models where they are at, or significantly heavier th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2211.05996","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2211.05996/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":"2211.05996","created_at":"2026-07-05T05:15:16.017073+00:00"},{"alias_kind":"arxiv_version","alias_value":"2211.05996v1","created_at":"2026-07-05T05:15:16.017073+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2211.05996","created_at":"2026-07-05T05:15:16.017073+00:00"},{"alias_kind":"pith_short_12","alias_value":"CIOWI2HHNBV7","created_at":"2026-07-05T05:15:16.017073+00:00"},{"alias_kind":"pith_short_16","alias_value":"CIOWI2HHNBV7IVB4","created_at":"2026-07-05T05:15:16.017073+00:00"},{"alias_kind":"pith_short_8","alias_value":"CIOWI2HH","created_at":"2026-07-05T05:15:16.017073+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.18752","citing_title":"Cosmic Colliders: High Energy Physics with First-Order Phase Transitions","ref_index":44,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CIOWI2HHNBV7IVB4LXGK6XIJXC","json":"https://pith.science/pith/CIOWI2HHNBV7IVB4LXGK6XIJXC.json","graph_json":"https://pith.science/api/pith-number/CIOWI2HHNBV7IVB4LXGK6XIJXC/graph.json","events_json":"https://pith.science/api/pith-number/CIOWI2HHNBV7IVB4LXGK6XIJXC/events.json","paper":"https://pith.science/paper/CIOWI2HH"},"agent_actions":{"view_html":"https://pith.science/pith/CIOWI2HHNBV7IVB4LXGK6XIJXC","download_json":"https://pith.science/pith/CIOWI2HHNBV7IVB4LXGK6XIJXC.json","view_paper":"https://pith.science/paper/CIOWI2HH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2211.05996&json=true","fetch_graph":"https://pith.science/api/pith-number/CIOWI2HHNBV7IVB4LXGK6XIJXC/graph.json","fetch_events":"https://pith.science/api/pith-number/CIOWI2HHNBV7IVB4LXGK6XIJXC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CIOWI2HHNBV7IVB4LXGK6XIJXC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CIOWI2HHNBV7IVB4LXGK6XIJXC/action/storage_attestation","attest_author":"https://pith.science/pith/CIOWI2HHNBV7IVB4LXGK6XIJXC/action/author_attestation","sign_citation":"https://pith.science/pith/CIOWI2HHNBV7IVB4LXGK6XIJXC/action/citation_signature","submit_replication":"https://pith.science/pith/CIOWI2HHNBV7IVB4LXGK6XIJXC/action/replication_record"}},"created_at":"2026-07-05T05:15:16.017073+00:00","updated_at":"2026-07-05T05:15:16.017073+00:00"}