{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:ZYP2ZCLWVRGKQVSVFF5XRKEYWR","short_pith_number":"pith:ZYP2ZCLW","schema_version":"1.0","canonical_sha256":"ce1fac8976ac4ca85655297b78a898b47903105e4ec695b0d7fd2a29adef096b","source":{"kind":"arxiv","id":"2305.09719","version":3},"attestation_state":"computed","paper":{"title":"Composite Dark Matter and Neutrino Masses from a Light Hidden Sector","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Aqeel Ahmed, Can Kilic, Niral Desai, Saereh Najjari, Sanket Doshi, Zackaria Chacko","submitted_at":"2023-05-16T18:00:02Z","abstract_excerpt":"We study a class of models in which the particle that constitutes dark matter arises as a composite state of a strongly coupled hidden sector. The hidden sector interacts with the Standard Model through the neutrino portal, allowing the relic abundance of dark matter to be set by annihilation into final states containing neutrinos. The coupling to the hidden sector also leads to the generation of neutrino masses through the inverse seesaw mechanism, with composite hidden sector states playing the role of the singlet neutrinos. We focus on the scenario in which the hidden sector is conformal in"},"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":"2305.09719","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2023-05-16T18:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"e65787779dae9b1885d8637f47cc5e2befdb8f1615fe0b040fc8b5e1447b124f","abstract_canon_sha256":"b0491854fc9871d141ed03d7f574e1c77e8a341ec608b6ccab0e57b095301eb1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:27:17.081696Z","signature_b64":"yNZJuHTkPyPWaK0F01peU9gUXjZZ6EA/UrnFOEJt8wnrDw6zI3fG5WJVf+3/aVaYzJKOG4/ohlvztfJkCgLpCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ce1fac8976ac4ca85655297b78a898b47903105e4ec695b0d7fd2a29adef096b","last_reissued_at":"2026-07-05T11:27:17.081206Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:27:17.081206Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Composite Dark Matter and Neutrino Masses from a Light Hidden Sector","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Aqeel Ahmed, Can Kilic, Niral Desai, Saereh Najjari, Sanket Doshi, Zackaria Chacko","submitted_at":"2023-05-16T18:00:02Z","abstract_excerpt":"We study a class of models in which the particle that constitutes dark matter arises as a composite state of a strongly coupled hidden sector. The hidden sector interacts with the Standard Model through the neutrino portal, allowing the relic abundance of dark matter to be set by annihilation into final states containing neutrinos. The coupling to the hidden sector also leads to the generation of neutrino masses through the inverse seesaw mechanism, with composite hidden sector states playing the role of the singlet neutrinos. We focus on the scenario in which the hidden sector is conformal in"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2305.09719","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/2305.09719/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":"2305.09719","created_at":"2026-07-05T11:27:17.081262+00:00"},{"alias_kind":"arxiv_version","alias_value":"2305.09719v3","created_at":"2026-07-05T11:27:17.081262+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2305.09719","created_at":"2026-07-05T11:27:17.081262+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZYP2ZCLWVRGK","created_at":"2026-07-05T11:27:17.081262+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZYP2ZCLWVRGKQVSV","created_at":"2026-07-05T11:27:17.081262+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZYP2ZCLW","created_at":"2026-07-05T11:27:17.081262+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.25014","citing_title":"Probing Confining Dark Sectors with Cosmological Perturbations","ref_index":35,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14282","citing_title":"Probing Neutrino Compositeness with Invisible and Displaced Signals","ref_index":7,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZYP2ZCLWVRGKQVSVFF5XRKEYWR","json":"https://pith.science/pith/ZYP2ZCLWVRGKQVSVFF5XRKEYWR.json","graph_json":"https://pith.science/api/pith-number/ZYP2ZCLWVRGKQVSVFF5XRKEYWR/graph.json","events_json":"https://pith.science/api/pith-number/ZYP2ZCLWVRGKQVSVFF5XRKEYWR/events.json","paper":"https://pith.science/paper/ZYP2ZCLW"},"agent_actions":{"view_html":"https://pith.science/pith/ZYP2ZCLWVRGKQVSVFF5XRKEYWR","download_json":"https://pith.science/pith/ZYP2ZCLWVRGKQVSVFF5XRKEYWR.json","view_paper":"https://pith.science/paper/ZYP2ZCLW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2305.09719&json=true","fetch_graph":"https://pith.science/api/pith-number/ZYP2ZCLWVRGKQVSVFF5XRKEYWR/graph.json","fetch_events":"https://pith.science/api/pith-number/ZYP2ZCLWVRGKQVSVFF5XRKEYWR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZYP2ZCLWVRGKQVSVFF5XRKEYWR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZYP2ZCLWVRGKQVSVFF5XRKEYWR/action/storage_attestation","attest_author":"https://pith.science/pith/ZYP2ZCLWVRGKQVSVFF5XRKEYWR/action/author_attestation","sign_citation":"https://pith.science/pith/ZYP2ZCLWVRGKQVSVFF5XRKEYWR/action/citation_signature","submit_replication":"https://pith.science/pith/ZYP2ZCLWVRGKQVSVFF5XRKEYWR/action/replication_record"}},"created_at":"2026-07-05T11:27:17.081262+00:00","updated_at":"2026-07-05T11:27:17.081262+00:00"}