{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1996:IWN4FMSZM5JXN5WHWFJX76ATFQ","short_pith_number":"pith:IWN4FMSZ","schema_version":"1.0","canonical_sha256":"459bc2b259675376f6c7b1537ff8132c0b52d0a9700f6d83e28cb3ff4469099c","source":{"kind":"arxiv","id":"hep-ph/9601362","version":1},"attestation_state":"computed","paper":{"title":"Detecting a Light Gravitino at Linear Collider to Probe the SUSY Breaking Scale","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"C.-P. Yuan, Daniel R. Stump, Michael Wiest","submitted_at":"1996-01-29T22:26:47Z","abstract_excerpt":"If supersymmetry is dynamically broken at a low scale ($M_{susy}$), within a few orders of magnitude of the weak scale, then the lightest supersymmetric partner is the gravitino and the next to lightest supersymmetric partner is a neutralino $\\chi^0_1$ with mass $m_{\\chi^0_1}$, which can decay into a photon ($\\gamma$) plus a gravitino ($\\widetilde{G}$). We study the detection of $e^{-}e^{+}\\rightarrow \\chi^0_1 \\chi^0_1 \\rightarrow \\gamma\\widetilde{G}\\gamma\\widetilde{G}$ at the proposed Linear Collider, and find the range of the parameters $M_{susy}$ and $m_{\\chi^0_1}$ that can be accessible wi"},"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":"hep-ph/9601362","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"1996-01-29T22:26:47Z","cross_cats_sorted":[],"title_canon_sha256":"17f90f473908a8107a2e64cd6010677841d30dda0521a8505022db0ea3227abc","abstract_canon_sha256":"bbee260518a2d266f246a895668f91665e723ccb7c32a1156a579e6677904ab1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:01:28.122084Z","signature_b64":"znyft7tvYCdkig+NdMRVOOiksEVZ/5uHS5JySBBUUQNcIWlQg7EX3D6hgs6oIeTCGbEJFEeLCw31lqyx0KW1Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"459bc2b259675376f6c7b1537ff8132c0b52d0a9700f6d83e28cb3ff4469099c","last_reissued_at":"2026-07-04T16:01:28.121709Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:01:28.121709Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Detecting a Light Gravitino at Linear Collider to Probe the SUSY Breaking Scale","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"C.-P. Yuan, Daniel R. Stump, Michael Wiest","submitted_at":"1996-01-29T22:26:47Z","abstract_excerpt":"If supersymmetry is dynamically broken at a low scale ($M_{susy}$), within a few orders of magnitude of the weak scale, then the lightest supersymmetric partner is the gravitino and the next to lightest supersymmetric partner is a neutralino $\\chi^0_1$ with mass $m_{\\chi^0_1}$, which can decay into a photon ($\\gamma$) plus a gravitino ($\\widetilde{G}$). We study the detection of $e^{-}e^{+}\\rightarrow \\chi^0_1 \\chi^0_1 \\rightarrow \\gamma\\widetilde{G}\\gamma\\widetilde{G}$ at the proposed Linear Collider, and find the range of the parameters $M_{susy}$ and $m_{\\chi^0_1}$ that can be accessible wi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9601362","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/hep-ph/9601362/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":"hep-ph/9601362","created_at":"2026-07-04T16:01:28.121771+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/9601362v1","created_at":"2026-07-04T16:01:28.121771+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/9601362","created_at":"2026-07-04T16:01:28.121771+00:00"},{"alias_kind":"pith_short_12","alias_value":"IWN4FMSZM5JX","created_at":"2026-07-04T16:01:28.121771+00:00"},{"alias_kind":"pith_short_16","alias_value":"IWN4FMSZM5JXN5WH","created_at":"2026-07-04T16:01:28.121771+00:00"},{"alias_kind":"pith_short_8","alias_value":"IWN4FMSZ","created_at":"2026-07-04T16:01:28.121771+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.09650","citing_title":"Revisiting the LHC Constraints on Gauge-Mediated Supersymmetry Breaking Scenarios","ref_index":39,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IWN4FMSZM5JXN5WHWFJX76ATFQ","json":"https://pith.science/pith/IWN4FMSZM5JXN5WHWFJX76ATFQ.json","graph_json":"https://pith.science/api/pith-number/IWN4FMSZM5JXN5WHWFJX76ATFQ/graph.json","events_json":"https://pith.science/api/pith-number/IWN4FMSZM5JXN5WHWFJX76ATFQ/events.json","paper":"https://pith.science/paper/IWN4FMSZ"},"agent_actions":{"view_html":"https://pith.science/pith/IWN4FMSZM5JXN5WHWFJX76ATFQ","download_json":"https://pith.science/pith/IWN4FMSZM5JXN5WHWFJX76ATFQ.json","view_paper":"https://pith.science/paper/IWN4FMSZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/9601362&json=true","fetch_graph":"https://pith.science/api/pith-number/IWN4FMSZM5JXN5WHWFJX76ATFQ/graph.json","fetch_events":"https://pith.science/api/pith-number/IWN4FMSZM5JXN5WHWFJX76ATFQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IWN4FMSZM5JXN5WHWFJX76ATFQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IWN4FMSZM5JXN5WHWFJX76ATFQ/action/storage_attestation","attest_author":"https://pith.science/pith/IWN4FMSZM5JXN5WHWFJX76ATFQ/action/author_attestation","sign_citation":"https://pith.science/pith/IWN4FMSZM5JXN5WHWFJX76ATFQ/action/citation_signature","submit_replication":"https://pith.science/pith/IWN4FMSZM5JXN5WHWFJX76ATFQ/action/replication_record"}},"created_at":"2026-07-04T16:01:28.121771+00:00","updated_at":"2026-07-04T16:01:28.121771+00:00"}