{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:27Z6IIHD6OF3AEAZ6VOA32YKAQ","short_pith_number":"pith:27Z6IIHD","schema_version":"1.0","canonical_sha256":"d7f3e420e3f38bb01019f55c0deb0a041e2b14fe3b88aa31e6beaccee429a899","source":{"kind":"arxiv","id":"2507.16246","version":1},"attestation_state":"computed","paper":{"title":"Split supersymmetry and hybrid inflation in light of Atacama Cosmology Telescope DR6 data","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Nobuchika Okada, Qaisar Shafi","submitted_at":"2025-07-22T05:39:31Z","abstract_excerpt":"Inspired by the recent measurement of the scalar spectral index, $n_s = 0.9743 \\pm 0.0034$, by the Atacama Cosmology Telescope (ACT) DR6 data, we present an update on the split supersymmetry hybrid inflation model, also known as $\\mu$-term hybrid inflation. The model employs a canonical K\\\"{a}hler potential but incorporates an additional renormalizable term in the superpotential $W$, which yields the MSSM $\\mu$-term following supersymmetry breaking. This additional term in $W$ is responsible for a high reheat temperature, $T_r \\gtrsim 10^{12}$ GeV, and consequently the necessity of split super"},"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":"2507.16246","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2025-07-22T05:39:31Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"e0aa289d05702f68f65eccfa01754fc36857f9d4c4b643cd6c5df15a630dc9b9","abstract_canon_sha256":"1c968e3c43007b355895b6655d617ad1bd0777bd72d60dd8ae64d0f462313409"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:41:06.272550Z","signature_b64":"vVdQEKn2JUBC87sNLyeJKbBNzbkIO7tzwksKh/UJx/W4V4talelE8khbpuXGWpHJu0+VIdanDQVrokYOy4CqBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d7f3e420e3f38bb01019f55c0deb0a041e2b14fe3b88aa31e6beaccee429a899","last_reissued_at":"2026-07-05T11:41:06.272096Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:41:06.272096Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Split supersymmetry and hybrid inflation in light of Atacama Cosmology Telescope DR6 data","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Nobuchika Okada, Qaisar Shafi","submitted_at":"2025-07-22T05:39:31Z","abstract_excerpt":"Inspired by the recent measurement of the scalar spectral index, $n_s = 0.9743 \\pm 0.0034$, by the Atacama Cosmology Telescope (ACT) DR6 data, we present an update on the split supersymmetry hybrid inflation model, also known as $\\mu$-term hybrid inflation. The model employs a canonical K\\\"{a}hler potential but incorporates an additional renormalizable term in the superpotential $W$, which yields the MSSM $\\mu$-term following supersymmetry breaking. This additional term in $W$ is responsible for a high reheat temperature, $T_r \\gtrsim 10^{12}$ GeV, and consequently the necessity of split super"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2507.16246","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/2507.16246/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":"2507.16246","created_at":"2026-07-05T11:41:06.272151+00:00"},{"alias_kind":"arxiv_version","alias_value":"2507.16246v1","created_at":"2026-07-05T11:41:06.272151+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2507.16246","created_at":"2026-07-05T11:41:06.272151+00:00"},{"alias_kind":"pith_short_12","alias_value":"27Z6IIHD6OF3","created_at":"2026-07-05T11:41:06.272151+00:00"},{"alias_kind":"pith_short_16","alias_value":"27Z6IIHD6OF3AEAZ","created_at":"2026-07-05T11:41:06.272151+00:00"},{"alias_kind":"pith_short_8","alias_value":"27Z6IIHD","created_at":"2026-07-05T11:41:06.272151+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2510.18320","citing_title":"The implications of inflation for the last ACT","ref_index":47,"is_internal_anchor":false},{"citing_arxiv_id":"2605.16884","citing_title":"Warm inflation in Weyl geometric gravity","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2602.05623","citing_title":"Induced-Gravity Palatini-Like Higgs Inflation in Supergravity Confronts ACT DR6","ref_index":42,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/27Z6IIHD6OF3AEAZ6VOA32YKAQ","json":"https://pith.science/pith/27Z6IIHD6OF3AEAZ6VOA32YKAQ.json","graph_json":"https://pith.science/api/pith-number/27Z6IIHD6OF3AEAZ6VOA32YKAQ/graph.json","events_json":"https://pith.science/api/pith-number/27Z6IIHD6OF3AEAZ6VOA32YKAQ/events.json","paper":"https://pith.science/paper/27Z6IIHD"},"agent_actions":{"view_html":"https://pith.science/pith/27Z6IIHD6OF3AEAZ6VOA32YKAQ","download_json":"https://pith.science/pith/27Z6IIHD6OF3AEAZ6VOA32YKAQ.json","view_paper":"https://pith.science/paper/27Z6IIHD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2507.16246&json=true","fetch_graph":"https://pith.science/api/pith-number/27Z6IIHD6OF3AEAZ6VOA32YKAQ/graph.json","fetch_events":"https://pith.science/api/pith-number/27Z6IIHD6OF3AEAZ6VOA32YKAQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/27Z6IIHD6OF3AEAZ6VOA32YKAQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/27Z6IIHD6OF3AEAZ6VOA32YKAQ/action/storage_attestation","attest_author":"https://pith.science/pith/27Z6IIHD6OF3AEAZ6VOA32YKAQ/action/author_attestation","sign_citation":"https://pith.science/pith/27Z6IIHD6OF3AEAZ6VOA32YKAQ/action/citation_signature","submit_replication":"https://pith.science/pith/27Z6IIHD6OF3AEAZ6VOA32YKAQ/action/replication_record"}},"created_at":"2026-07-05T11:41:06.272151+00:00","updated_at":"2026-07-05T11:41:06.272151+00:00"}