{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:SJYMR54FIANJ7HXSOXIVPY7UAF","short_pith_number":"pith:SJYMR54F","schema_version":"1.0","canonical_sha256":"9270c8f785401a9f9ef275d157e3f4014a6a4edeb782947493ed6195dbeab22b","source":{"kind":"arxiv","id":"1806.11281","version":2},"attestation_state":"computed","paper":{"title":"Impact of vacuum stability, perturbativity and XENON1T on global fits of $\\mathbb{Z}_2$ and $\\mathbb{Z}_3$ scalar singlet dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Felix Kahlhoefer, James McKay, Jonathan M. Cornell, Pat Scott, Peter Athron, Sebastian Wild","submitted_at":"2018-06-29T07:04:18Z","abstract_excerpt":"Scalar singlet dark matter is one of the simplest and most predictive realisations of the WIMP (weakly-interacting massive particle) idea. Although the model is constrained from all directions by the latest experimental data, it still has viable regions of parameter space. Another compelling aspect of scalar singlets is their ability to stabilise the electroweak vacuum. Indeed, models of scalar dark matter are not low-energy effective theories, but can be valid all the way to the Planck scale. Using the GAMBIT framework, we present the first global fit to include both the low-energy experiment"},"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":"1806.11281","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2018-06-29T07:04:18Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"20d6a932cc33d113f77df6201bf35913d52407da2ada3ea8dc037ad18485d4c3","abstract_canon_sha256":"a0d97ed7f2ab483a3bc96d6d669d68392c34d06f050da4adfc1e53ee9c8b1493"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:24:46.563646Z","signature_b64":"2J2fbTghb7vsLzSKi5n3Lic3U2ZuQSFPm3uk2VpMwsbxYzj0Nm8E1SPcS8kDpnHg/Uf3FSQNFF89SH5nFRFZAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9270c8f785401a9f9ef275d157e3f4014a6a4edeb782947493ed6195dbeab22b","last_reissued_at":"2026-07-05T01:24:46.563014Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:24:46.563014Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Impact of vacuum stability, perturbativity and XENON1T on global fits of $\\mathbb{Z}_2$ and $\\mathbb{Z}_3$ scalar singlet dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Felix Kahlhoefer, James McKay, Jonathan M. Cornell, Pat Scott, Peter Athron, Sebastian Wild","submitted_at":"2018-06-29T07:04:18Z","abstract_excerpt":"Scalar singlet dark matter is one of the simplest and most predictive realisations of the WIMP (weakly-interacting massive particle) idea. Although the model is constrained from all directions by the latest experimental data, it still has viable regions of parameter space. Another compelling aspect of scalar singlets is their ability to stabilise the electroweak vacuum. Indeed, models of scalar dark matter are not low-energy effective theories, but can be valid all the way to the Planck scale. Using the GAMBIT framework, we present the first global fit to include both the low-energy experiment"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.11281","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/1806.11281/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":"1806.11281","created_at":"2026-07-05T01:24:46.563080+00:00"},{"alias_kind":"arxiv_version","alias_value":"1806.11281v2","created_at":"2026-07-05T01:24:46.563080+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1806.11281","created_at":"2026-07-05T01:24:46.563080+00:00"},{"alias_kind":"pith_short_12","alias_value":"SJYMR54FIANJ","created_at":"2026-07-05T01:24:46.563080+00:00"},{"alias_kind":"pith_short_16","alias_value":"SJYMR54FIANJ7HXS","created_at":"2026-07-05T01:24:46.563080+00:00"},{"alias_kind":"pith_short_8","alias_value":"SJYMR54F","created_at":"2026-07-05T01:24:46.563080+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1908.10615","citing_title":"Probing the Symmetric Higgs Portal with Di-Higgs Boson Production","ref_index":16,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SJYMR54FIANJ7HXSOXIVPY7UAF","json":"https://pith.science/pith/SJYMR54FIANJ7HXSOXIVPY7UAF.json","graph_json":"https://pith.science/api/pith-number/SJYMR54FIANJ7HXSOXIVPY7UAF/graph.json","events_json":"https://pith.science/api/pith-number/SJYMR54FIANJ7HXSOXIVPY7UAF/events.json","paper":"https://pith.science/paper/SJYMR54F"},"agent_actions":{"view_html":"https://pith.science/pith/SJYMR54FIANJ7HXSOXIVPY7UAF","download_json":"https://pith.science/pith/SJYMR54FIANJ7HXSOXIVPY7UAF.json","view_paper":"https://pith.science/paper/SJYMR54F","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1806.11281&json=true","fetch_graph":"https://pith.science/api/pith-number/SJYMR54FIANJ7HXSOXIVPY7UAF/graph.json","fetch_events":"https://pith.science/api/pith-number/SJYMR54FIANJ7HXSOXIVPY7UAF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SJYMR54FIANJ7HXSOXIVPY7UAF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SJYMR54FIANJ7HXSOXIVPY7UAF/action/storage_attestation","attest_author":"https://pith.science/pith/SJYMR54FIANJ7HXSOXIVPY7UAF/action/author_attestation","sign_citation":"https://pith.science/pith/SJYMR54FIANJ7HXSOXIVPY7UAF/action/citation_signature","submit_replication":"https://pith.science/pith/SJYMR54FIANJ7HXSOXIVPY7UAF/action/replication_record"}},"created_at":"2026-07-05T01:24:46.563080+00:00","updated_at":"2026-07-05T01:24:46.563080+00:00"}