{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:X346O2JAT6Y4ZUHEEDDEG63XX6","short_pith_number":"pith:X346O2JA","schema_version":"1.0","canonical_sha256":"bef9e769209fb1ccd0e420c6437b77bfb49e883bf0ff8f67c22f1b72bfdda894","source":{"kind":"arxiv","id":"1501.03700","version":2},"attestation_state":"computed","paper":{"title":"Dark matter, neutrino masses and high scale validity of an inert Higgs doublet model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Biswarup Mukhopadhyaya, Dilip Kumar Ghosh, Ipsita Saha, Nabarun Chakrabarty","submitted_at":"2015-01-15T14:48:47Z","abstract_excerpt":"We consider a two-Higgs doublet scenario containing three $SU(2)_L$ singlet heavy neutrinos with Majorana masses. The second scalar doublet as well as the neutrinos are odd under a $Z_2$ symmetry. This scenario not only generates Majorana masses for the light neutrinos radiatively but also makes the lighter of the neutral $Z_2$-odd scalars an eligible dark matter candidate, in addition to triggering leptogenesis at the scale of the heavy neutrino masses. Taking two representative values of this mass scale, we identify the allowed regions of the parameter space of the model, which are consisten"},"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":"1501.03700","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-01-15T14:48:47Z","cross_cats_sorted":[],"title_canon_sha256":"b2e908b17f0cd0ffd650348e8b01c08f55b6e4c58711f9fdd53914448c0a49cc","abstract_canon_sha256":"fcd1f93e6fd28535745ed8ab153ac92619ee0b363ee6d48aa5f522cde943d609"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:36:54.551639Z","signature_b64":"7Zix4HNe8N16lnr4/aD3wsDhexqksnQShgtsScs9TUlvhJooNARQTzeoK/XNlGiGel0CUC16eusjAyrMPHkFDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bef9e769209fb1ccd0e420c6437b77bfb49e883bf0ff8f67c22f1b72bfdda894","last_reissued_at":"2026-05-18T01:36:54.550918Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:36:54.550918Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark matter, neutrino masses and high scale validity of an inert Higgs doublet model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Biswarup Mukhopadhyaya, Dilip Kumar Ghosh, Ipsita Saha, Nabarun Chakrabarty","submitted_at":"2015-01-15T14:48:47Z","abstract_excerpt":"We consider a two-Higgs doublet scenario containing three $SU(2)_L$ singlet heavy neutrinos with Majorana masses. The second scalar doublet as well as the neutrinos are odd under a $Z_2$ symmetry. This scenario not only generates Majorana masses for the light neutrinos radiatively but also makes the lighter of the neutral $Z_2$-odd scalars an eligible dark matter candidate, in addition to triggering leptogenesis at the scale of the heavy neutrino masses. Taking two representative values of this mass scale, we identify the allowed regions of the parameter space of the model, which are consisten"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.03700","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":""},"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":"1501.03700","created_at":"2026-05-18T01:36:54.551030+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.03700v2","created_at":"2026-05-18T01:36:54.551030+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.03700","created_at":"2026-05-18T01:36:54.551030+00:00"},{"alias_kind":"pith_short_12","alias_value":"X346O2JAT6Y4","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_16","alias_value":"X346O2JAT6Y4ZUHE","created_at":"2026-05-18T12:29:47.479230+00:00"},{"alias_kind":"pith_short_8","alias_value":"X346O2JA","created_at":"2026-05-18T12:29:47.479230+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/X346O2JAT6Y4ZUHEEDDEG63XX6","json":"https://pith.science/pith/X346O2JAT6Y4ZUHEEDDEG63XX6.json","graph_json":"https://pith.science/api/pith-number/X346O2JAT6Y4ZUHEEDDEG63XX6/graph.json","events_json":"https://pith.science/api/pith-number/X346O2JAT6Y4ZUHEEDDEG63XX6/events.json","paper":"https://pith.science/paper/X346O2JA"},"agent_actions":{"view_html":"https://pith.science/pith/X346O2JAT6Y4ZUHEEDDEG63XX6","download_json":"https://pith.science/pith/X346O2JAT6Y4ZUHEEDDEG63XX6.json","view_paper":"https://pith.science/paper/X346O2JA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.03700&json=true","fetch_graph":"https://pith.science/api/pith-number/X346O2JAT6Y4ZUHEEDDEG63XX6/graph.json","fetch_events":"https://pith.science/api/pith-number/X346O2JAT6Y4ZUHEEDDEG63XX6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/X346O2JAT6Y4ZUHEEDDEG63XX6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/X346O2JAT6Y4ZUHEEDDEG63XX6/action/storage_attestation","attest_author":"https://pith.science/pith/X346O2JAT6Y4ZUHEEDDEG63XX6/action/author_attestation","sign_citation":"https://pith.science/pith/X346O2JAT6Y4ZUHEEDDEG63XX6/action/citation_signature","submit_replication":"https://pith.science/pith/X346O2JAT6Y4ZUHEEDDEG63XX6/action/replication_record"}},"created_at":"2026-05-18T01:36:54.551030+00:00","updated_at":"2026-05-18T01:36:54.551030+00:00"}