{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:DL3SN4CTCZQYHNGX56KUCFYIWN","short_pith_number":"pith:DL3SN4CT","schema_version":"1.0","canonical_sha256":"1af726f053166183b4d7ef95411708b34ed4635fa41f3ee288b13d178c113d46","source":{"kind":"arxiv","id":"1102.4906","version":1},"attestation_state":"computed","paper":{"title":"Dark Matter in Inert Triplet Models","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"C. Q. Geng, Keiko I. Nagao, Takeshi Araki","submitted_at":"2011-02-24T05:37:07Z","abstract_excerpt":"We study the inert triplet models, in which the standard model (SM) is extended to have a new SU(2)L triplet scalar (Y=0 or 2) with an Z2 symmetry. We show that the neutral component of the triplet can be a good dark matter candidate. In particular, for the hypercharge Y=0 triplet model, the WMAP data favors the region where the dark matter mass is around 5.5 TeV, which is also consistent with the direct detection experiments. In contrast, for the Y=2 model, although dark matter with its mass around 2.8 TeV is allowed by WMAP, it is excluded by the direct detection experiments because the spin"},"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":"1102.4906","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2011-02-24T05:37:07Z","cross_cats_sorted":[],"title_canon_sha256":"3d7292c6749e22ec6212420c765dba8c307bf9ecc228f92bcaef4c3978b6a0be","abstract_canon_sha256":"14ba0e433c045ba374ea7f0b7d0cbcedfec9cebdffd5883987d9ca231d80daaf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:22:39.809269Z","signature_b64":"2BUu1CjW1lnXldNjIVDfjUrLk76pANfFhEfFkzE8+yNlgm2sm9DtPTlO2RP+VXxbBLrcAYnSkTCXNidiESHdBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1af726f053166183b4d7ef95411708b34ed4635fa41f3ee288b13d178c113d46","last_reissued_at":"2026-05-18T04:22:39.808908Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:22:39.808908Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark Matter in Inert Triplet Models","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"C. Q. Geng, Keiko I. Nagao, Takeshi Araki","submitted_at":"2011-02-24T05:37:07Z","abstract_excerpt":"We study the inert triplet models, in which the standard model (SM) is extended to have a new SU(2)L triplet scalar (Y=0 or 2) with an Z2 symmetry. We show that the neutral component of the triplet can be a good dark matter candidate. In particular, for the hypercharge Y=0 triplet model, the WMAP data favors the region where the dark matter mass is around 5.5 TeV, which is also consistent with the direct detection experiments. In contrast, for the Y=2 model, although dark matter with its mass around 2.8 TeV is allowed by WMAP, it is excluded by the direct detection experiments because the spin"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1102.4906","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":"1102.4906","created_at":"2026-05-18T04:22:39.808963+00:00"},{"alias_kind":"arxiv_version","alias_value":"1102.4906v1","created_at":"2026-05-18T04:22:39.808963+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1102.4906","created_at":"2026-05-18T04:22:39.808963+00:00"},{"alias_kind":"pith_short_12","alias_value":"DL3SN4CTCZQY","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_16","alias_value":"DL3SN4CTCZQYHNGX","created_at":"2026-05-18T12:26:26.731475+00:00"},{"alias_kind":"pith_short_8","alias_value":"DL3SN4CT","created_at":"2026-05-18T12:26:26.731475+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DL3SN4CTCZQYHNGX56KUCFYIWN","json":"https://pith.science/pith/DL3SN4CTCZQYHNGX56KUCFYIWN.json","graph_json":"https://pith.science/api/pith-number/DL3SN4CTCZQYHNGX56KUCFYIWN/graph.json","events_json":"https://pith.science/api/pith-number/DL3SN4CTCZQYHNGX56KUCFYIWN/events.json","paper":"https://pith.science/paper/DL3SN4CT"},"agent_actions":{"view_html":"https://pith.science/pith/DL3SN4CTCZQYHNGX56KUCFYIWN","download_json":"https://pith.science/pith/DL3SN4CTCZQYHNGX56KUCFYIWN.json","view_paper":"https://pith.science/paper/DL3SN4CT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1102.4906&json=true","fetch_graph":"https://pith.science/api/pith-number/DL3SN4CTCZQYHNGX56KUCFYIWN/graph.json","fetch_events":"https://pith.science/api/pith-number/DL3SN4CTCZQYHNGX56KUCFYIWN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DL3SN4CTCZQYHNGX56KUCFYIWN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DL3SN4CTCZQYHNGX56KUCFYIWN/action/storage_attestation","attest_author":"https://pith.science/pith/DL3SN4CTCZQYHNGX56KUCFYIWN/action/author_attestation","sign_citation":"https://pith.science/pith/DL3SN4CTCZQYHNGX56KUCFYIWN/action/citation_signature","submit_replication":"https://pith.science/pith/DL3SN4CTCZQYHNGX56KUCFYIWN/action/replication_record"}},"created_at":"2026-05-18T04:22:39.808963+00:00","updated_at":"2026-05-18T04:22:39.808963+00:00"}