{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:LE75RQVF2JPR2QTSID2362UKFV","short_pith_number":"pith:LE75RQVF","schema_version":"1.0","canonical_sha256":"593fd8c2a5d25f1d427240f5bf6a8a2d66115aef748fe2361c4c8dff332e6251","source":{"kind":"arxiv","id":"2406.00188","version":2},"attestation_state":"computed","paper":{"title":"Cutting the Scotogenic loop: Adding flavor to Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Newton Nath, Rahul Srivastava, Ranjeet Kumar","submitted_at":"2024-05-31T20:38:54Z","abstract_excerpt":"We introduce a framework for hybrid neutrino mass generation, wherein scotogenic dark sector particles, including dark matter, are charged non-trivially under the $A_4$ flavor symmetry. The spontaneous breaking of the $A_4$ group to residual $\\mathcal{Z}_2$ subgroup results in the ``cutting\" of the radiative loop. As a consequence the neutrinos acquire mass through the hybrid ``scoto-seesaw\" mass mechanism, combining aspects of both the tree-level seesaw and one-loop scotogenic mechanisms, with the residual $\\mathcal{Z}_2$ subgroup ensuring the stability of the dark matter. The flavor symmetry"},"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":"2406.00188","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2024-05-31T20:38:54Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"ce2fb12c44c337bc6a4076d9c929a7879cf8e4d92b781750707297b7b85e5422","abstract_canon_sha256":"b09fb3c43d6e3fe9ba54a9e5fe862ab3bcc1ac9611aff66ce6e65aa9853d45d2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:44:51.026797Z","signature_b64":"+BLDBP2B6AQ6XTPHjsXAmurXlknS0RuwK8dlKKI16QD1tkABiwtbv9tRskXHnrROkFDeY1341/CBy4ww0XV6Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"593fd8c2a5d25f1d427240f5bf6a8a2d66115aef748fe2361c4c8dff332e6251","last_reissued_at":"2026-07-05T09:44:51.024339Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:44:51.024339Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cutting the Scotogenic loop: Adding flavor to Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Newton Nath, Rahul Srivastava, Ranjeet Kumar","submitted_at":"2024-05-31T20:38:54Z","abstract_excerpt":"We introduce a framework for hybrid neutrino mass generation, wherein scotogenic dark sector particles, including dark matter, are charged non-trivially under the $A_4$ flavor symmetry. The spontaneous breaking of the $A_4$ group to residual $\\mathcal{Z}_2$ subgroup results in the ``cutting\" of the radiative loop. As a consequence the neutrinos acquire mass through the hybrid ``scoto-seesaw\" mass mechanism, combining aspects of both the tree-level seesaw and one-loop scotogenic mechanisms, with the residual $\\mathcal{Z}_2$ subgroup ensuring the stability of the dark matter. The flavor symmetry"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2406.00188","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2406.00188/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":"2406.00188","created_at":"2026-07-05T09:44:51.024403+00:00"},{"alias_kind":"arxiv_version","alias_value":"2406.00188v2","created_at":"2026-07-05T09:44:51.024403+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2406.00188","created_at":"2026-07-05T09:44:51.024403+00:00"},{"alias_kind":"pith_short_12","alias_value":"LE75RQVF2JPR","created_at":"2026-07-05T09:44:51.024403+00:00"},{"alias_kind":"pith_short_16","alias_value":"LE75RQVF2JPR2QTS","created_at":"2026-07-05T09:44:51.024403+00:00"},{"alias_kind":"pith_short_8","alias_value":"LE75RQVF","created_at":"2026-07-05T09:44:51.024403+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.20119","citing_title":"The Simplest Dirac Scoto-Seesaw Realization","ref_index":43,"is_internal_anchor":false},{"citing_arxiv_id":"2605.29031","citing_title":"Twilight of the WIMP: Comprehensive Phenomenology of Electroweak Triplet Dark Matter","ref_index":27,"is_internal_anchor":false},{"citing_arxiv_id":"2506.04370","citing_title":"Dark Matter Induced Proton Decays","ref_index":49,"is_internal_anchor":false},{"citing_arxiv_id":"2602.11277","citing_title":"Fate of $\\theta_{12}$ under $\\mu-\\tau$ Reflection Symmetry in Light of the First JUNO Results","ref_index":55,"is_internal_anchor":false},{"citing_arxiv_id":"2604.19122","citing_title":"Implications of the First JUNO Results for Dirac Neutrino Texture Zeros","ref_index":13,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LE75RQVF2JPR2QTSID2362UKFV","json":"https://pith.science/pith/LE75RQVF2JPR2QTSID2362UKFV.json","graph_json":"https://pith.science/api/pith-number/LE75RQVF2JPR2QTSID2362UKFV/graph.json","events_json":"https://pith.science/api/pith-number/LE75RQVF2JPR2QTSID2362UKFV/events.json","paper":"https://pith.science/paper/LE75RQVF"},"agent_actions":{"view_html":"https://pith.science/pith/LE75RQVF2JPR2QTSID2362UKFV","download_json":"https://pith.science/pith/LE75RQVF2JPR2QTSID2362UKFV.json","view_paper":"https://pith.science/paper/LE75RQVF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2406.00188&json=true","fetch_graph":"https://pith.science/api/pith-number/LE75RQVF2JPR2QTSID2362UKFV/graph.json","fetch_events":"https://pith.science/api/pith-number/LE75RQVF2JPR2QTSID2362UKFV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LE75RQVF2JPR2QTSID2362UKFV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LE75RQVF2JPR2QTSID2362UKFV/action/storage_attestation","attest_author":"https://pith.science/pith/LE75RQVF2JPR2QTSID2362UKFV/action/author_attestation","sign_citation":"https://pith.science/pith/LE75RQVF2JPR2QTSID2362UKFV/action/citation_signature","submit_replication":"https://pith.science/pith/LE75RQVF2JPR2QTSID2362UKFV/action/replication_record"}},"created_at":"2026-07-05T09:44:51.024403+00:00","updated_at":"2026-07-05T09:44:51.024403+00:00"}