{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:HQVV2424TLJOVCDDDUJQECCC72","short_pith_number":"pith:HQVV2424","schema_version":"1.0","canonical_sha256":"3c2b5d735c9ad2ea88631d13020842feb8a23e8815c6fd7d7534938f6d7bb52c","source":{"kind":"arxiv","id":"2507.10745","version":1},"attestation_state":"computed","paper":{"title":"Beyond standard model particles in the atmospheric flux: a long-lived stau example","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Atri Bhattacharya, Ina Sarcevic, Mary Hall Reno","submitted_at":"2025-07-14T19:11:17Z","abstract_excerpt":"We discuss fluxes of long-lived supersymmetric (SUSY) particles produced in the atmosphere from ultra-high energy cosmic-ray interactions with air nuclei. We consider long-lived particle production which proceeds first via the on-shell formation of heavier particles in the SUSY spectrum and then their decays. Specifically, we focus on the production of stau pairs from the decays of squarks produced in the initial cosmic ray-air collision under the purview of gauge-mediated symmetry breaking models that have the stau as the next-to-lightest SUSY particle. The calculation of the resulting stau f"},"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":"2507.10745","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2025-07-14T19:11:17Z","cross_cats_sorted":[],"title_canon_sha256":"363cffa18ba662b4542871ae22437150e530ea743b221f028ae4a19257cc0366","abstract_canon_sha256":"1a5840aec0e2aa17acd0bd39bfc5983ec6f434ce92b0b5660bfc58e928d59e89"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:36:59.368059Z","signature_b64":"9elYFKgEJ8R+et6GTzkpCWMzUht8IZxDadevAp1W+SQXYyLE1P1RLpEYP6mU/wabYFY4DUoYvJMk93yBXkMRCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3c2b5d735c9ad2ea88631d13020842feb8a23e8815c6fd7d7534938f6d7bb52c","last_reissued_at":"2026-07-05T11:36:59.367473Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:36:59.367473Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Beyond standard model particles in the atmospheric flux: a long-lived stau example","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Atri Bhattacharya, Ina Sarcevic, Mary Hall Reno","submitted_at":"2025-07-14T19:11:17Z","abstract_excerpt":"We discuss fluxes of long-lived supersymmetric (SUSY) particles produced in the atmosphere from ultra-high energy cosmic-ray interactions with air nuclei. We consider long-lived particle production which proceeds first via the on-shell formation of heavier particles in the SUSY spectrum and then their decays. Specifically, we focus on the production of stau pairs from the decays of squarks produced in the initial cosmic ray-air collision under the purview of gauge-mediated symmetry breaking models that have the stau as the next-to-lightest SUSY particle. The calculation of the resulting stau f"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2507.10745","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/2507.10745/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":"2507.10745","created_at":"2026-07-05T11:36:59.367541+00:00"},{"alias_kind":"arxiv_version","alias_value":"2507.10745v1","created_at":"2026-07-05T11:36:59.367541+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2507.10745","created_at":"2026-07-05T11:36:59.367541+00:00"},{"alias_kind":"pith_short_12","alias_value":"HQVV2424TLJO","created_at":"2026-07-05T11:36:59.367541+00:00"},{"alias_kind":"pith_short_16","alias_value":"HQVV2424TLJOVCDD","created_at":"2026-07-05T11:36:59.367541+00:00"},{"alias_kind":"pith_short_8","alias_value":"HQVV2424","created_at":"2026-07-05T11:36:59.367541+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HQVV2424TLJOVCDDDUJQECCC72","json":"https://pith.science/pith/HQVV2424TLJOVCDDDUJQECCC72.json","graph_json":"https://pith.science/api/pith-number/HQVV2424TLJOVCDDDUJQECCC72/graph.json","events_json":"https://pith.science/api/pith-number/HQVV2424TLJOVCDDDUJQECCC72/events.json","paper":"https://pith.science/paper/HQVV2424"},"agent_actions":{"view_html":"https://pith.science/pith/HQVV2424TLJOVCDDDUJQECCC72","download_json":"https://pith.science/pith/HQVV2424TLJOVCDDDUJQECCC72.json","view_paper":"https://pith.science/paper/HQVV2424","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2507.10745&json=true","fetch_graph":"https://pith.science/api/pith-number/HQVV2424TLJOVCDDDUJQECCC72/graph.json","fetch_events":"https://pith.science/api/pith-number/HQVV2424TLJOVCDDDUJQECCC72/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HQVV2424TLJOVCDDDUJQECCC72/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HQVV2424TLJOVCDDDUJQECCC72/action/storage_attestation","attest_author":"https://pith.science/pith/HQVV2424TLJOVCDDDUJQECCC72/action/author_attestation","sign_citation":"https://pith.science/pith/HQVV2424TLJOVCDDDUJQECCC72/action/citation_signature","submit_replication":"https://pith.science/pith/HQVV2424TLJOVCDDDUJQECCC72/action/replication_record"}},"created_at":"2026-07-05T11:36:59.367541+00:00","updated_at":"2026-07-05T11:36:59.367541+00:00"}