{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:FE67GCQRILEOOKI7DJYPDJDQLS","short_pith_number":"pith:FE67GCQR","schema_version":"1.0","canonical_sha256":"293df30a1142c8e7291f1a70f1a4705c9a8ae77ab7e355f541713277aa0a1260","source":{"kind":"arxiv","id":"1412.0018","version":2},"attestation_state":"computed","paper":{"title":"Illuminating Dark Photons with High-Energy Colliders","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"David Curtin, Jessie Shelton, Rouven Essig, Stefania Gori","submitted_at":"2014-11-28T21:00:05Z","abstract_excerpt":"High-energy colliders offer a unique sensitivity to dark photons, the mediators of a broken dark U(1) gauge theory that kinetically mixes with the Standard Model (SM) hypercharge. Dark photons can be detected in the exotic decay of the 125 GeV Higgs boson, h -> Z Z_D -> 4l, and in Drell-Yan events, pp -> Z_D -> ll. If the dark U(1) is broken by a hidden-sector Higgs mechanism, then mixing between the dark and SM Higgs bosons also allows the exotic decay h -> Z_D Z_D -> 4l. We show that the 14 TeV LHC and a 100 TeV proton-proton collider provide powerful probes of both exotic Higgs decay channe"},"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":"1412.0018","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-11-28T21:00:05Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"d64f9cd23f00bffde3be42b004fc930c3efddb3c29b469c6238a03d320c2709b","abstract_canon_sha256":"54bef3bca112ce2692e65e5815534c4d6cedcf95bf8a289e8642e44b586eb390"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:41:24.951251Z","signature_b64":"qCuw5HFLTzxBiYYElngqwpbsAqTs4ifzbR+nIRUbUU/LEWV7NwNzBDBnRA8ogneCY5Vay74iz3tLtjpsoLd8AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"293df30a1142c8e7291f1a70f1a4705c9a8ae77ab7e355f541713277aa0a1260","last_reissued_at":"2026-05-18T01:41:24.950621Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:41:24.950621Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Illuminating Dark Photons with High-Energy Colliders","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"David Curtin, Jessie Shelton, Rouven Essig, Stefania Gori","submitted_at":"2014-11-28T21:00:05Z","abstract_excerpt":"High-energy colliders offer a unique sensitivity to dark photons, the mediators of a broken dark U(1) gauge theory that kinetically mixes with the Standard Model (SM) hypercharge. Dark photons can be detected in the exotic decay of the 125 GeV Higgs boson, h -> Z Z_D -> 4l, and in Drell-Yan events, pp -> Z_D -> ll. If the dark U(1) is broken by a hidden-sector Higgs mechanism, then mixing between the dark and SM Higgs bosons also allows the exotic decay h -> Z_D Z_D -> 4l. We show that the 14 TeV LHC and a 100 TeV proton-proton collider provide powerful probes of both exotic Higgs decay channe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1412.0018","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":"1412.0018","created_at":"2026-05-18T01:41:24.950745+00:00"},{"alias_kind":"arxiv_version","alias_value":"1412.0018v2","created_at":"2026-05-18T01:41:24.950745+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1412.0018","created_at":"2026-05-18T01:41:24.950745+00:00"},{"alias_kind":"pith_short_12","alias_value":"FE67GCQRILEO","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_16","alias_value":"FE67GCQRILEOOKI7","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_8","alias_value":"FE67GCQR","created_at":"2026-05-18T12:28:28.263976+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2507.11376","citing_title":"GeV-scale thermal dark matter from dark photons: tightly constrained, yet allowed","ref_index":58,"is_internal_anchor":true},{"citing_arxiv_id":"2508.08676","citing_title":"WIMP Dark Matter within the dark photon portal","ref_index":43,"is_internal_anchor":true},{"citing_arxiv_id":"2605.11630","citing_title":"Long-lived sterile neutrinos from axionlike particles at the Super Tau-Charm Facility","ref_index":29,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FE67GCQRILEOOKI7DJYPDJDQLS","json":"https://pith.science/pith/FE67GCQRILEOOKI7DJYPDJDQLS.json","graph_json":"https://pith.science/api/pith-number/FE67GCQRILEOOKI7DJYPDJDQLS/graph.json","events_json":"https://pith.science/api/pith-number/FE67GCQRILEOOKI7DJYPDJDQLS/events.json","paper":"https://pith.science/paper/FE67GCQR"},"agent_actions":{"view_html":"https://pith.science/pith/FE67GCQRILEOOKI7DJYPDJDQLS","download_json":"https://pith.science/pith/FE67GCQRILEOOKI7DJYPDJDQLS.json","view_paper":"https://pith.science/paper/FE67GCQR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1412.0018&json=true","fetch_graph":"https://pith.science/api/pith-number/FE67GCQRILEOOKI7DJYPDJDQLS/graph.json","fetch_events":"https://pith.science/api/pith-number/FE67GCQRILEOOKI7DJYPDJDQLS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FE67GCQRILEOOKI7DJYPDJDQLS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FE67GCQRILEOOKI7DJYPDJDQLS/action/storage_attestation","attest_author":"https://pith.science/pith/FE67GCQRILEOOKI7DJYPDJDQLS/action/author_attestation","sign_citation":"https://pith.science/pith/FE67GCQRILEOOKI7DJYPDJDQLS/action/citation_signature","submit_replication":"https://pith.science/pith/FE67GCQRILEOOKI7DJYPDJDQLS/action/replication_record"}},"created_at":"2026-05-18T01:41:24.950745+00:00","updated_at":"2026-05-18T01:41:24.950745+00:00"}