{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:E775TF267S42BIOF2GUOJKA6WG","short_pith_number":"pith:E775TF26","schema_version":"1.0","canonical_sha256":"27ffd9975efcb9a0a1c5d1a8e4a81eb18a54e1aa4dde51e9ff50866465817092","source":{"kind":"arxiv","id":"2009.11287","version":3},"attestation_state":"computed","paper":{"title":"WIMPs at High Energy Muon Colliders","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Lian-Tao Wang, Tao Han, Xing Wang, Zhen Liu","submitted_at":"2020-09-23T17:59:59Z","abstract_excerpt":"The Weakly Interacting Massive Particle (WIMP) paradigm is one of the most compelling scenarios for particle dark matter (DM). We show in this paper that a high energy muon collider can make decisive statements about the WIMP DM, and this should serve as one of its main physics driver cases. We demonstrate this by employing the DM as the lightest member of an electroweak (EW) multiplet, which is a simple, yet one of the most challenging WIMP scenarios given its minimal collider signature and high thermal target mass scale of 1 TeV$-$23 TeV. We perform a first study of the reach of high energy "},"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":"2009.11287","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2020-09-23T17:59:59Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"2dfc4d520841a7227abf6edbcb8db11937b1b846017c82ad9aec04a1358a6cfe","abstract_canon_sha256":"1c84d69cab176dead6c9c4a379c7c59d728e365c9a2f7e6ab91c65f7eefd1e0e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:54:29.154620Z","signature_b64":"T6U28KfzMdgcw7erB8DUnMOtQq8efUuQ0K5JbguokiMCZUM7YyFhRm6eGrwaN4b6XZ/nFUXUmald0Yt/yKr+Cw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"27ffd9975efcb9a0a1c5d1a8e4a81eb18a54e1aa4dde51e9ff50866465817092","last_reissued_at":"2026-07-05T02:54:29.154207Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:54:29.154207Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"WIMPs at High Energy Muon Colliders","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Lian-Tao Wang, Tao Han, Xing Wang, Zhen Liu","submitted_at":"2020-09-23T17:59:59Z","abstract_excerpt":"The Weakly Interacting Massive Particle (WIMP) paradigm is one of the most compelling scenarios for particle dark matter (DM). We show in this paper that a high energy muon collider can make decisive statements about the WIMP DM, and this should serve as one of its main physics driver cases. We demonstrate this by employing the DM as the lightest member of an electroweak (EW) multiplet, which is a simple, yet one of the most challenging WIMP scenarios given its minimal collider signature and high thermal target mass scale of 1 TeV$-$23 TeV. We perform a first study of the reach of high energy "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2009.11287","kind":"arxiv","version":3},"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/2009.11287/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":"2009.11287","created_at":"2026-07-05T02:54:29.154261+00:00"},{"alias_kind":"arxiv_version","alias_value":"2009.11287v3","created_at":"2026-07-05T02:54:29.154261+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2009.11287","created_at":"2026-07-05T02:54:29.154261+00:00"},{"alias_kind":"pith_short_12","alias_value":"E775TF267S42","created_at":"2026-07-05T02:54:29.154261+00:00"},{"alias_kind":"pith_short_16","alias_value":"E775TF267S42BIOF","created_at":"2026-07-05T02:54:29.154261+00:00"},{"alias_kind":"pith_short_8","alias_value":"E775TF26","created_at":"2026-07-05T02:54:29.154261+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2512.23159","citing_title":"Muonphilic asymmetric dark matter at a future muon collider","ref_index":29,"is_internal_anchor":false},{"citing_arxiv_id":"2605.13957","citing_title":"Heavy Vector Triplets at a Muon Collider","ref_index":21,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08688","citing_title":"Probing Higgs and Top Interactions through the Muon Lens at multi-TeV Muon Colliders","ref_index":32,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/E775TF267S42BIOF2GUOJKA6WG","json":"https://pith.science/pith/E775TF267S42BIOF2GUOJKA6WG.json","graph_json":"https://pith.science/api/pith-number/E775TF267S42BIOF2GUOJKA6WG/graph.json","events_json":"https://pith.science/api/pith-number/E775TF267S42BIOF2GUOJKA6WG/events.json","paper":"https://pith.science/paper/E775TF26"},"agent_actions":{"view_html":"https://pith.science/pith/E775TF267S42BIOF2GUOJKA6WG","download_json":"https://pith.science/pith/E775TF267S42BIOF2GUOJKA6WG.json","view_paper":"https://pith.science/paper/E775TF26","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2009.11287&json=true","fetch_graph":"https://pith.science/api/pith-number/E775TF267S42BIOF2GUOJKA6WG/graph.json","fetch_events":"https://pith.science/api/pith-number/E775TF267S42BIOF2GUOJKA6WG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/E775TF267S42BIOF2GUOJKA6WG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/E775TF267S42BIOF2GUOJKA6WG/action/storage_attestation","attest_author":"https://pith.science/pith/E775TF267S42BIOF2GUOJKA6WG/action/author_attestation","sign_citation":"https://pith.science/pith/E775TF267S42BIOF2GUOJKA6WG/action/citation_signature","submit_replication":"https://pith.science/pith/E775TF267S42BIOF2GUOJKA6WG/action/replication_record"}},"created_at":"2026-07-05T02:54:29.154261+00:00","updated_at":"2026-07-05T02:54:29.154261+00:00"}