{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:NFAQO2PEOPDX2QOXLIPHJQVF7Z","short_pith_number":"pith:NFAQO2PE","schema_version":"1.0","canonical_sha256":"69410769e473c77d41d75a1e74c2a5fe48ea5a46674ceb30886b541e010309fb","source":{"kind":"arxiv","id":"2012.03266","version":2},"attestation_state":"computed","paper":{"title":"The Upper Bound of the Second Higgs Boson Mass in Minimal Gauge Mediation with the Gravitino Warm Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Gongjun Choi, Norimi Yokozaki, Tsutomu T. Yanagida","submitted_at":"2020-12-06T13:42:21Z","abstract_excerpt":"A keV-scale gravitino arsing from a minimal supersymmetric (SUSY) Standard Model (MSSM) is an interesting possibility since the small scale problems that $\\Lambda$CDM model encounters in the modern cosmology could be alleviated with the keV-scale gravitino serving as the warm dark matter (WDM). Such a light gravitino asks for a low scale supersymmetry (SUSY) breaking for which the gauge mediation (GM) is required as a consistent SUSY-breaking mediation mechanism. In this paper, we show upperbounds of the masses of the second CP-even Higgs boson $H$ and the CP-odd Higgs boson $A$, assuming the "},"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":"2012.03266","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2020-12-06T13:42:21Z","cross_cats_sorted":["astro-ph.CO","hep-ex"],"title_canon_sha256":"9fbbf4d66078dbd4fea4b6e471ccd141b263d6483668b73e10afaa4907e1ba85","abstract_canon_sha256":"67bd7c36d12aa57de5f826873d68af721ec660203a31b6a4c0fb54f20584fe5d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:29:56.289089Z","signature_b64":"NGub/j4W1+o83rvXw01XxmQoEwp2v097q8ieUHzxbrcWY2I+Rv5FMznhHbzSYhMEYB+REsiDx92rXmmPjYVpCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"69410769e473c77d41d75a1e74c2a5fe48ea5a46674ceb30886b541e010309fb","last_reissued_at":"2026-07-05T02:29:56.288668Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:29:56.288668Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Upper Bound of the Second Higgs Boson Mass in Minimal Gauge Mediation with the Gravitino Warm Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Gongjun Choi, Norimi Yokozaki, Tsutomu T. Yanagida","submitted_at":"2020-12-06T13:42:21Z","abstract_excerpt":"A keV-scale gravitino arsing from a minimal supersymmetric (SUSY) Standard Model (MSSM) is an interesting possibility since the small scale problems that $\\Lambda$CDM model encounters in the modern cosmology could be alleviated with the keV-scale gravitino serving as the warm dark matter (WDM). Such a light gravitino asks for a low scale supersymmetry (SUSY) breaking for which the gauge mediation (GM) is required as a consistent SUSY-breaking mediation mechanism. In this paper, we show upperbounds of the masses of the second CP-even Higgs boson $H$ and the CP-odd Higgs boson $A$, assuming the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2012.03266","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2012.03266/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":"2012.03266","created_at":"2026-07-05T02:29:56.288725+00:00"},{"alias_kind":"arxiv_version","alias_value":"2012.03266v2","created_at":"2026-07-05T02:29:56.288725+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2012.03266","created_at":"2026-07-05T02:29:56.288725+00:00"},{"alias_kind":"pith_short_12","alias_value":"NFAQO2PEOPDX","created_at":"2026-07-05T02:29:56.288725+00:00"},{"alias_kind":"pith_short_16","alias_value":"NFAQO2PEOPDX2QOX","created_at":"2026-07-05T02:29:56.288725+00:00"},{"alias_kind":"pith_short_8","alias_value":"NFAQO2PE","created_at":"2026-07-05T02:29:56.288725+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2502.07539","citing_title":"Neutralino dark matter in gauge mediation","ref_index":28,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NFAQO2PEOPDX2QOXLIPHJQVF7Z","json":"https://pith.science/pith/NFAQO2PEOPDX2QOXLIPHJQVF7Z.json","graph_json":"https://pith.science/api/pith-number/NFAQO2PEOPDX2QOXLIPHJQVF7Z/graph.json","events_json":"https://pith.science/api/pith-number/NFAQO2PEOPDX2QOXLIPHJQVF7Z/events.json","paper":"https://pith.science/paper/NFAQO2PE"},"agent_actions":{"view_html":"https://pith.science/pith/NFAQO2PEOPDX2QOXLIPHJQVF7Z","download_json":"https://pith.science/pith/NFAQO2PEOPDX2QOXLIPHJQVF7Z.json","view_paper":"https://pith.science/paper/NFAQO2PE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2012.03266&json=true","fetch_graph":"https://pith.science/api/pith-number/NFAQO2PEOPDX2QOXLIPHJQVF7Z/graph.json","fetch_events":"https://pith.science/api/pith-number/NFAQO2PEOPDX2QOXLIPHJQVF7Z/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NFAQO2PEOPDX2QOXLIPHJQVF7Z/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NFAQO2PEOPDX2QOXLIPHJQVF7Z/action/storage_attestation","attest_author":"https://pith.science/pith/NFAQO2PEOPDX2QOXLIPHJQVF7Z/action/author_attestation","sign_citation":"https://pith.science/pith/NFAQO2PEOPDX2QOXLIPHJQVF7Z/action/citation_signature","submit_replication":"https://pith.science/pith/NFAQO2PEOPDX2QOXLIPHJQVF7Z/action/replication_record"}},"created_at":"2026-07-05T02:29:56.288725+00:00","updated_at":"2026-07-05T02:29:56.288725+00:00"}