{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:KKFWBZNK7HZXGMFZPRUHLV4C4R","short_pith_number":"pith:KKFWBZNK","schema_version":"1.0","canonical_sha256":"528b60e5aaf9f37330b97c6875d782e468ab80b7da0a9f26b6f26c1a89f389e1","source":{"kind":"arxiv","id":"1503.07209","version":1},"attestation_state":"computed","paper":{"title":"Radiative Return Capabilities of a High-Energy, High-Luminosity $e^+e^-$ Collider","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Jonathan L. Rosner, Lian-Tao Wang, Marek Karliner, Matthew Low","submitted_at":"2015-03-24T21:25:38Z","abstract_excerpt":"An electron-positron collider operating at a center-of-mass energy $E_{CM}$ can collect events at all lower energies through initial-state radiation (ISR or radiative return). We explore the capabilities for radiative return studies by a proposed high-luminosity collider at $E_{CM}$ = 250 or 90 GeV, to fill in gaps left by lower-energy colliders such as PEP, PETRA, TRISTAN, and LEP. These capabilities are compared with those of the lower-energy $e^+e^-$ colliders as well as hadron colliders such as the Tevatron and the CERN Large Hadron Collider (LHC). Some examples of accessible questions in "},"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":"1503.07209","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2015-03-24T21:25:38Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"10eccd4ce6da117e01a9feae83cc401dbfa658ac5a95d888e576be19c78b9f61","abstract_canon_sha256":"585e1a7949c697aa45ebb94c6cd021e7dbacb64e3bc79761805d163dee60f2e3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:35:10.773436Z","signature_b64":"aec700zqbrezNo0IBlcj8iy0IXcsZyDIoKBri+TGwKX+XuUcOLHVUHxkOV2Ob2YdcROa5Mob0C2us9NJR8x9BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"528b60e5aaf9f37330b97c6875d782e468ab80b7da0a9f26b6f26c1a89f389e1","last_reissued_at":"2026-05-18T01:35:10.772820Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:35:10.772820Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Radiative Return Capabilities of a High-Energy, High-Luminosity $e^+e^-$ Collider","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Jonathan L. Rosner, Lian-Tao Wang, Marek Karliner, Matthew Low","submitted_at":"2015-03-24T21:25:38Z","abstract_excerpt":"An electron-positron collider operating at a center-of-mass energy $E_{CM}$ can collect events at all lower energies through initial-state radiation (ISR or radiative return). We explore the capabilities for radiative return studies by a proposed high-luminosity collider at $E_{CM}$ = 250 or 90 GeV, to fill in gaps left by lower-energy colliders such as PEP, PETRA, TRISTAN, and LEP. These capabilities are compared with those of the lower-energy $e^+e^-$ colliders as well as hadron colliders such as the Tevatron and the CERN Large Hadron Collider (LHC). Some examples of accessible questions in "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1503.07209","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":""},"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":"1503.07209","created_at":"2026-05-18T01:35:10.772910+00:00"},{"alias_kind":"arxiv_version","alias_value":"1503.07209v1","created_at":"2026-05-18T01:35:10.772910+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1503.07209","created_at":"2026-05-18T01:35:10.772910+00:00"},{"alias_kind":"pith_short_12","alias_value":"KKFWBZNK7HZX","created_at":"2026-05-18T12:29:29.992203+00:00"},{"alias_kind":"pith_short_16","alias_value":"KKFWBZNK7HZXGMFZ","created_at":"2026-05-18T12:29:29.992203+00:00"},{"alias_kind":"pith_short_8","alias_value":"KKFWBZNK","created_at":"2026-05-18T12:29:29.992203+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":4,"sample":[{"citing_arxiv_id":"2607.08082","citing_title":"$Z^\\prime$ Portal Dark Matter with Observable $\\Delta N_{\\rm eff}$","ref_index":106,"is_internal_anchor":true},{"citing_arxiv_id":"2606.07746","citing_title":"Dark Z' at a Muon Collider: Radiative Return versus Vector Boson Fusion","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2005.01515","citing_title":"The Dark Photon","ref_index":210,"is_internal_anchor":true},{"citing_arxiv_id":"2505.00272","citing_title":"Future Circular Collider Feasibility Study Report: Volume 1, Physics, Experiments, Detectors","ref_index":153,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/KKFWBZNK7HZXGMFZPRUHLV4C4R","json":"https://pith.science/pith/KKFWBZNK7HZXGMFZPRUHLV4C4R.json","graph_json":"https://pith.science/api/pith-number/KKFWBZNK7HZXGMFZPRUHLV4C4R/graph.json","events_json":"https://pith.science/api/pith-number/KKFWBZNK7HZXGMFZPRUHLV4C4R/events.json","paper":"https://pith.science/paper/KKFWBZNK"},"agent_actions":{"view_html":"https://pith.science/pith/KKFWBZNK7HZXGMFZPRUHLV4C4R","download_json":"https://pith.science/pith/KKFWBZNK7HZXGMFZPRUHLV4C4R.json","view_paper":"https://pith.science/paper/KKFWBZNK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1503.07209&json=true","fetch_graph":"https://pith.science/api/pith-number/KKFWBZNK7HZXGMFZPRUHLV4C4R/graph.json","fetch_events":"https://pith.science/api/pith-number/KKFWBZNK7HZXGMFZPRUHLV4C4R/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KKFWBZNK7HZXGMFZPRUHLV4C4R/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KKFWBZNK7HZXGMFZPRUHLV4C4R/action/storage_attestation","attest_author":"https://pith.science/pith/KKFWBZNK7HZXGMFZPRUHLV4C4R/action/author_attestation","sign_citation":"https://pith.science/pith/KKFWBZNK7HZXGMFZPRUHLV4C4R/action/citation_signature","submit_replication":"https://pith.science/pith/KKFWBZNK7HZXGMFZPRUHLV4C4R/action/replication_record"}},"created_at":"2026-05-18T01:35:10.772910+00:00","updated_at":"2026-05-18T01:35:10.772910+00:00"}