{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:DFDYOISY7OL35K4763YCQTFYJB","short_pith_number":"pith:DFDYOISY","schema_version":"1.0","canonical_sha256":"1947872258fb97beab9ff6f0284cb84864a6bafbf4ec49f32771e9def1fa37c3","source":{"kind":"arxiv","id":"2407.12104","version":3},"attestation_state":"computed","paper":{"title":"Freezing-in Cannibal Dark Sectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Andrzej Hryczuk, Esau Cervantes","submitted_at":"2024-07-16T18:14:21Z","abstract_excerpt":"Self-Interacting Dark Matter models can successfully explain dark matter (DM) production through interactions confined within the dark sector. However, they often lack measurable experimental signals due to their secluded nature. Including a feeble interaction with the visible sector through a Higgs portal leads not only to potential detection avenues and richer thermal production dynamics, but also to a possible explanation of the initial dark sector population through the freeze-in mechanism. In this work we study, by solving the full system of coupled Boltzmann equations for the number dens"},"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":"2407.12104","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2024-07-16T18:14:21Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"da890d3bd9b655588a7ce65ea7bf08152e4c70874cce5a3fad749781c781a364","abstract_canon_sha256":"c988037d7e283c3772376145142300fe9cf555a6e0579f0ef738105842cc9de3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:01:14.737366Z","signature_b64":"ltassg8ByqPJIvy/Oq5yIF9vOg2O/yCW5+XlyXLNPWs9usF2J7X1/g+M1TFhA4nDGWGoxjLZgQodhK6QJLwtCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1947872258fb97beab9ff6f0284cb84864a6bafbf4ec49f32771e9def1fa37c3","last_reissued_at":"2026-07-05T10:01:14.736869Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:01:14.736869Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Freezing-in Cannibal Dark Sectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Andrzej Hryczuk, Esau Cervantes","submitted_at":"2024-07-16T18:14:21Z","abstract_excerpt":"Self-Interacting Dark Matter models can successfully explain dark matter (DM) production through interactions confined within the dark sector. However, they often lack measurable experimental signals due to their secluded nature. Including a feeble interaction with the visible sector through a Higgs portal leads not only to potential detection avenues and richer thermal production dynamics, but also to a possible explanation of the initial dark sector population through the freeze-in mechanism. In this work we study, by solving the full system of coupled Boltzmann equations for the number dens"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.12104","kind":"arxiv","version":3},"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/2407.12104/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":"2407.12104","created_at":"2026-07-05T10:01:14.736926+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.12104v3","created_at":"2026-07-05T10:01:14.736926+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.12104","created_at":"2026-07-05T10:01:14.736926+00:00"},{"alias_kind":"pith_short_12","alias_value":"DFDYOISY7OL3","created_at":"2026-07-05T10:01:14.736926+00:00"},{"alias_kind":"pith_short_16","alias_value":"DFDYOISY7OL35K47","created_at":"2026-07-05T10:01:14.736926+00:00"},{"alias_kind":"pith_short_8","alias_value":"DFDYOISY","created_at":"2026-07-05T10:01:14.736926+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2607.00755","citing_title":"KineticXGPU: A Tensorized Collision Operator for Dark-Sector Self-Scattering","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2509.06892","citing_title":"Asymmetric Cannibal Dark Matter: Constraints from Neutron Star","ref_index":16,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DFDYOISY7OL35K4763YCQTFYJB","json":"https://pith.science/pith/DFDYOISY7OL35K4763YCQTFYJB.json","graph_json":"https://pith.science/api/pith-number/DFDYOISY7OL35K4763YCQTFYJB/graph.json","events_json":"https://pith.science/api/pith-number/DFDYOISY7OL35K4763YCQTFYJB/events.json","paper":"https://pith.science/paper/DFDYOISY"},"agent_actions":{"view_html":"https://pith.science/pith/DFDYOISY7OL35K4763YCQTFYJB","download_json":"https://pith.science/pith/DFDYOISY7OL35K4763YCQTFYJB.json","view_paper":"https://pith.science/paper/DFDYOISY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.12104&json=true","fetch_graph":"https://pith.science/api/pith-number/DFDYOISY7OL35K4763YCQTFYJB/graph.json","fetch_events":"https://pith.science/api/pith-number/DFDYOISY7OL35K4763YCQTFYJB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DFDYOISY7OL35K4763YCQTFYJB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DFDYOISY7OL35K4763YCQTFYJB/action/storage_attestation","attest_author":"https://pith.science/pith/DFDYOISY7OL35K4763YCQTFYJB/action/author_attestation","sign_citation":"https://pith.science/pith/DFDYOISY7OL35K4763YCQTFYJB/action/citation_signature","submit_replication":"https://pith.science/pith/DFDYOISY7OL35K4763YCQTFYJB/action/replication_record"}},"created_at":"2026-07-05T10:01:14.736926+00:00","updated_at":"2026-07-05T10:01:14.736926+00:00"}