{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:LXBQEE7MPDNGCU5DNMJNW3SWJG","short_pith_number":"pith:LXBQEE7M","schema_version":"1.0","canonical_sha256":"5dc30213ec78da6153a36b12db6e564988eea4a23773c1dba7720ca5ea7f29af","source":{"kind":"arxiv","id":"1009.3963","version":2},"attestation_state":"computed","paper":{"title":"Dark Light Higgs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"hep-ph","authors_text":"Carlos E.M. Wagner, Hao Zhang, Lian-Tao Wang, Patrick Draper, Tao Liu","submitted_at":"2010-09-20T23:02:06Z","abstract_excerpt":"We study a limit of the nearly-Peccei-Quinn-symmetric Next-to-Minimal Supersymmetric Standard Model possessing novel Higgs and dark matter (DM) properties. In this scenario, there naturally co-exist three light singlet-like particles: a scalar, a pseudoscalar, and a singlino-like DM candidate, all with masses of order 0.1-10 GeV. The decay of a Standard Model-like Higgs boson to pairs of the light scalars or pseudoscalars is generically suppressed, avoiding constraints from collider searches for these channels. For a certain parameter window annihilation into the light pseudoscalar and exchang"},"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":"1009.3963","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-09-20T23:02:06Z","cross_cats_sorted":["astro-ph.CO","hep-th"],"title_canon_sha256":"615b8151bbff56c6519c2ea93b78e9b151d5ffcf94b8738f35fcb7dfddc12370","abstract_canon_sha256":"ddbf7a7b19edffe30e624cb0590a897b2ffaf52fb7cc6614dbf8b30379d309f3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:08:33.610373Z","signature_b64":"V2TunySWjwKt4Hb/js5zTX3i9wpbdaVv+ox1fmT8FPniEnnDF8/ZRAsbYtLTy0OPLqe3S39bOLNyFI5LoRvOBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5dc30213ec78da6153a36b12db6e564988eea4a23773c1dba7720ca5ea7f29af","last_reissued_at":"2026-05-18T04:08:33.609771Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:08:33.609771Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark Light Higgs","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-th"],"primary_cat":"hep-ph","authors_text":"Carlos E.M. Wagner, Hao Zhang, Lian-Tao Wang, Patrick Draper, Tao Liu","submitted_at":"2010-09-20T23:02:06Z","abstract_excerpt":"We study a limit of the nearly-Peccei-Quinn-symmetric Next-to-Minimal Supersymmetric Standard Model possessing novel Higgs and dark matter (DM) properties. In this scenario, there naturally co-exist three light singlet-like particles: a scalar, a pseudoscalar, and a singlino-like DM candidate, all with masses of order 0.1-10 GeV. The decay of a Standard Model-like Higgs boson to pairs of the light scalars or pseudoscalars is generically suppressed, avoiding constraints from collider searches for these channels. For a certain parameter window annihilation into the light pseudoscalar and exchang"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1009.3963","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":"1009.3963","created_at":"2026-05-18T04:08:33.609887+00:00"},{"alias_kind":"arxiv_version","alias_value":"1009.3963v2","created_at":"2026-05-18T04:08:33.609887+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1009.3963","created_at":"2026-05-18T04:08:33.609887+00:00"},{"alias_kind":"pith_short_12","alias_value":"LXBQEE7MPDNG","created_at":"2026-05-18T12:26:10.704358+00:00"},{"alias_kind":"pith_short_16","alias_value":"LXBQEE7MPDNGCU5D","created_at":"2026-05-18T12:26:10.704358+00:00"},{"alias_kind":"pith_short_8","alias_value":"LXBQEE7M","created_at":"2026-05-18T12:26:10.704358+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2503.05463","citing_title":"Search for Higgs boson exotic decays into Lorentz-boosted light bosons in the four-$\\tau$ final state at $\\sqrt{s}=13$ TeV with the ATLAS detector","ref_index":13,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13336","citing_title":"Probing Boosted Light Scalars in the Type-I 2HDM","ref_index":6,"is_internal_anchor":true},{"citing_arxiv_id":"2604.06326","citing_title":"Exotic Higgs Decays at a Muon Collider","ref_index":103,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LXBQEE7MPDNGCU5DNMJNW3SWJG","json":"https://pith.science/pith/LXBQEE7MPDNGCU5DNMJNW3SWJG.json","graph_json":"https://pith.science/api/pith-number/LXBQEE7MPDNGCU5DNMJNW3SWJG/graph.json","events_json":"https://pith.science/api/pith-number/LXBQEE7MPDNGCU5DNMJNW3SWJG/events.json","paper":"https://pith.science/paper/LXBQEE7M"},"agent_actions":{"view_html":"https://pith.science/pith/LXBQEE7MPDNGCU5DNMJNW3SWJG","download_json":"https://pith.science/pith/LXBQEE7MPDNGCU5DNMJNW3SWJG.json","view_paper":"https://pith.science/paper/LXBQEE7M","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1009.3963&json=true","fetch_graph":"https://pith.science/api/pith-number/LXBQEE7MPDNGCU5DNMJNW3SWJG/graph.json","fetch_events":"https://pith.science/api/pith-number/LXBQEE7MPDNGCU5DNMJNW3SWJG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LXBQEE7MPDNGCU5DNMJNW3SWJG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LXBQEE7MPDNGCU5DNMJNW3SWJG/action/storage_attestation","attest_author":"https://pith.science/pith/LXBQEE7MPDNGCU5DNMJNW3SWJG/action/author_attestation","sign_citation":"https://pith.science/pith/LXBQEE7MPDNGCU5DNMJNW3SWJG/action/citation_signature","submit_replication":"https://pith.science/pith/LXBQEE7MPDNGCU5DNMJNW3SWJG/action/replication_record"}},"created_at":"2026-05-18T04:08:33.609887+00:00","updated_at":"2026-05-18T04:08:33.609887+00:00"}