{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:GIPGKHZNPV2LASDZW6PFF32TVO","short_pith_number":"pith:GIPGKHZN","schema_version":"1.0","canonical_sha256":"321e651f2d7d74b04879b79e52ef53abb2b068a9a251ef973ad0afbc063a6b91","source":{"kind":"arxiv","id":"1908.04659","version":1},"attestation_state":"computed","paper":{"title":"Inert Doublet Model Signatures at Future e+e- Colliders","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Aleksander Filip Zarnecki, Dorota Sokolowska, Jan Kalinowski, Jan Klamka, Pawel Sopicki, Tania Robens, Wojciech Kotlarski","submitted_at":"2019-08-13T14:30:11Z","abstract_excerpt":"The Inert Doublet Model is one of the simplest extensions of the Standard Model, providing a dark matter candidate. It is a two Higgs doublet model with a discrete $Z_2$ symmetry, that prevents the scalars of the second doublet (inert scalars) from coupling to the Standard Model fermions and makes the lightest of them stable. We study a large number of Inert Doublet Model scenarios, which are consistent with current constraints on direct detection, including the most recent bounds from the XENON1T experiment and relic density of dark matter, as well as collider and low-energy limits. We use a "},"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":"1908.04659","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2019-08-13T14:30:11Z","cross_cats_sorted":[],"title_canon_sha256":"fa592583e06779845e093fa931b64c59e1d61ff0b53314aa4504ac219ba751b3","abstract_canon_sha256":"37b438f0494a67fd0489256111bccabf7a60acf0955e22f307aa60cc91d2b2c1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T23:55:15.349126Z","signature_b64":"qMiZbJ6J6J9uoZykiuA1cjlkiNi+Y/Sl555msqI+wVSWBsAU+WloK5QCAUoPCJAw2bAyTF12psV4rsmSw8ptAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"321e651f2d7d74b04879b79e52ef53abb2b068a9a251ef973ad0afbc063a6b91","last_reissued_at":"2026-07-04T23:55:15.348740Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T23:55:15.348740Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Inert Doublet Model Signatures at Future e+e- Colliders","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Aleksander Filip Zarnecki, Dorota Sokolowska, Jan Kalinowski, Jan Klamka, Pawel Sopicki, Tania Robens, Wojciech Kotlarski","submitted_at":"2019-08-13T14:30:11Z","abstract_excerpt":"The Inert Doublet Model is one of the simplest extensions of the Standard Model, providing a dark matter candidate. It is a two Higgs doublet model with a discrete $Z_2$ symmetry, that prevents the scalars of the second doublet (inert scalars) from coupling to the Standard Model fermions and makes the lightest of them stable. We study a large number of Inert Doublet Model scenarios, which are consistent with current constraints on direct detection, including the most recent bounds from the XENON1T experiment and relic density of dark matter, as well as collider and low-energy limits. We use a "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1908.04659","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1908.04659/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":"1908.04659","created_at":"2026-07-04T23:55:15.348795+00:00"},{"alias_kind":"arxiv_version","alias_value":"1908.04659v1","created_at":"2026-07-04T23:55:15.348795+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1908.04659","created_at":"2026-07-04T23:55:15.348795+00:00"},{"alias_kind":"pith_short_12","alias_value":"GIPGKHZNPV2L","created_at":"2026-07-04T23:55:15.348795+00:00"},{"alias_kind":"pith_short_16","alias_value":"GIPGKHZNPV2LASDZ","created_at":"2026-07-04T23:55:15.348795+00:00"},{"alias_kind":"pith_short_8","alias_value":"GIPGKHZN","created_at":"2026-07-04T23:55:15.348795+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1908.10809","citing_title":"Investigating extended scalar sectors at current and future colliders","ref_index":61,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GIPGKHZNPV2LASDZW6PFF32TVO","json":"https://pith.science/pith/GIPGKHZNPV2LASDZW6PFF32TVO.json","graph_json":"https://pith.science/api/pith-number/GIPGKHZNPV2LASDZW6PFF32TVO/graph.json","events_json":"https://pith.science/api/pith-number/GIPGKHZNPV2LASDZW6PFF32TVO/events.json","paper":"https://pith.science/paper/GIPGKHZN"},"agent_actions":{"view_html":"https://pith.science/pith/GIPGKHZNPV2LASDZW6PFF32TVO","download_json":"https://pith.science/pith/GIPGKHZNPV2LASDZW6PFF32TVO.json","view_paper":"https://pith.science/paper/GIPGKHZN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1908.04659&json=true","fetch_graph":"https://pith.science/api/pith-number/GIPGKHZNPV2LASDZW6PFF32TVO/graph.json","fetch_events":"https://pith.science/api/pith-number/GIPGKHZNPV2LASDZW6PFF32TVO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GIPGKHZNPV2LASDZW6PFF32TVO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GIPGKHZNPV2LASDZW6PFF32TVO/action/storage_attestation","attest_author":"https://pith.science/pith/GIPGKHZNPV2LASDZW6PFF32TVO/action/author_attestation","sign_citation":"https://pith.science/pith/GIPGKHZNPV2LASDZW6PFF32TVO/action/citation_signature","submit_replication":"https://pith.science/pith/GIPGKHZNPV2LASDZW6PFF32TVO/action/replication_record"}},"created_at":"2026-07-04T23:55:15.348795+00:00","updated_at":"2026-07-04T23:55:15.348795+00:00"}