{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2008:7IYL4ZEAJG5R46O3FTSZYPAN5Q","short_pith_number":"pith:7IYL4ZEA","schema_version":"1.0","canonical_sha256":"fa30be648049bb1e79db2ce59c3c0dec328157c7ed4430624c6a08c51da85b5a","source":{"kind":"arxiv","id":"0810.3924","version":2},"attestation_state":"computed","paper":{"title":"Inert Doublet Model and LEP II Limits","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph"],"primary_cat":"hep-ph","authors_text":"Erik Lundstrom, Joakim Edsjo, Michael Gustafsson","submitted_at":"2008-10-21T20:33:35Z","abstract_excerpt":"The inert doublet model is a minimal extension of the standard model introducing an additional SU(2) doublet with new scalar particles that could be produced at accelerators. While there exists no LEP II analysis dedicated for these inert scalars, the absence of a signal within searches for supersymmetric neutralinos can be used to constrain the inert doublet model. This translation however requires some care because of the different properties of the inert scalars and the neutralinos. We investigate what restrictions an existing DELPHI collaboration study of neutralino pair production can put"},"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":"0810.3924","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2008-10-21T20:33:35Z","cross_cats_sorted":["astro-ph"],"title_canon_sha256":"677e9c89cce04f272f0c50304db72b6827bf4ec8c174d9b9b998b4d022943d73","abstract_canon_sha256":"d350d39dd473f8cdd9093b6afcbcdeb382621f873097ee25154e9d1aacdaa625"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:38:09.663556Z","signature_b64":"pQLTjFnpQYMWZkQoprE77G6ZWunrPWyk3eMVgiRirpbgncDysZ0msf3zg1J6C9ocLZR+uEdNyVxPmcLZ7XTyCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fa30be648049bb1e79db2ce59c3c0dec328157c7ed4430624c6a08c51da85b5a","last_reissued_at":"2026-07-04T15:38:09.663077Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:38:09.663077Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Inert Doublet Model and LEP II Limits","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph"],"primary_cat":"hep-ph","authors_text":"Erik Lundstrom, Joakim Edsjo, Michael Gustafsson","submitted_at":"2008-10-21T20:33:35Z","abstract_excerpt":"The inert doublet model is a minimal extension of the standard model introducing an additional SU(2) doublet with new scalar particles that could be produced at accelerators. While there exists no LEP II analysis dedicated for these inert scalars, the absence of a signal within searches for supersymmetric neutralinos can be used to constrain the inert doublet model. This translation however requires some care because of the different properties of the inert scalars and the neutralinos. We investigate what restrictions an existing DELPHI collaboration study of neutralino pair production can put"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0810.3924","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/0810.3924/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":"0810.3924","created_at":"2026-07-04T15:38:09.663141+00:00"},{"alias_kind":"arxiv_version","alias_value":"0810.3924v2","created_at":"2026-07-04T15:38:09.663141+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0810.3924","created_at":"2026-07-04T15:38:09.663141+00:00"},{"alias_kind":"pith_short_12","alias_value":"7IYL4ZEAJG5R","created_at":"2026-07-04T15:38:09.663141+00:00"},{"alias_kind":"pith_short_16","alias_value":"7IYL4ZEAJG5R46O3","created_at":"2026-07-04T15:38:09.663141+00:00"},{"alias_kind":"pith_short_8","alias_value":"7IYL4ZEA","created_at":"2026-07-04T15:38:09.663141+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2607.07853","citing_title":"Neutrino Masses and Dark Matter Stability in 3HDMs with Minimal Non-Abelian Discrete Symmetries","ref_index":28,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13614","citing_title":"Search for pair production of additional neutral scalars within the Inert Doublet Model in a final state with two electrons or two muons in proton-proton collisions at $\\sqrt{s}$ = 13 TeV and 13.6 TeV","ref_index":44,"is_internal_anchor":true},{"citing_arxiv_id":"2605.07616","citing_title":"Probing the Inert Doublet Dark Matter with Stellar-Mass Black Hole Mini-Spikes","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15425","citing_title":"The $Z_3$ soft breaking in the I(2+1)HDM and its cosmological probes","ref_index":16,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7IYL4ZEAJG5R46O3FTSZYPAN5Q","json":"https://pith.science/pith/7IYL4ZEAJG5R46O3FTSZYPAN5Q.json","graph_json":"https://pith.science/api/pith-number/7IYL4ZEAJG5R46O3FTSZYPAN5Q/graph.json","events_json":"https://pith.science/api/pith-number/7IYL4ZEAJG5R46O3FTSZYPAN5Q/events.json","paper":"https://pith.science/paper/7IYL4ZEA"},"agent_actions":{"view_html":"https://pith.science/pith/7IYL4ZEAJG5R46O3FTSZYPAN5Q","download_json":"https://pith.science/pith/7IYL4ZEAJG5R46O3FTSZYPAN5Q.json","view_paper":"https://pith.science/paper/7IYL4ZEA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0810.3924&json=true","fetch_graph":"https://pith.science/api/pith-number/7IYL4ZEAJG5R46O3FTSZYPAN5Q/graph.json","fetch_events":"https://pith.science/api/pith-number/7IYL4ZEAJG5R46O3FTSZYPAN5Q/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7IYL4ZEAJG5R46O3FTSZYPAN5Q/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7IYL4ZEAJG5R46O3FTSZYPAN5Q/action/storage_attestation","attest_author":"https://pith.science/pith/7IYL4ZEAJG5R46O3FTSZYPAN5Q/action/author_attestation","sign_citation":"https://pith.science/pith/7IYL4ZEAJG5R46O3FTSZYPAN5Q/action/citation_signature","submit_replication":"https://pith.science/pith/7IYL4ZEAJG5R46O3FTSZYPAN5Q/action/replication_record"}},"created_at":"2026-07-04T15:38:09.663141+00:00","updated_at":"2026-07-04T15:38:09.663141+00:00"}