{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:EGBA4F7MWPZ35IE7V3OBQMCHRW","short_pith_number":"pith:EGBA4F7M","schema_version":"1.0","canonical_sha256":"21820e17ecb3f3bea09faedc1830478db5201f1656cd5fbc38d90b5f16b6f5a9","source":{"kind":"arxiv","id":"hep-ph/0410198","version":4},"attestation_state":"computed","paper":{"title":"How Long Could We Live?","license":"","headline":"","cross_cats":["hep-ex","hep-th"],"primary_cat":"hep-ph","authors_text":"Ilja Dorsner, Pavel Fileviez Perez","submitted_at":"2004-10-13T16:48:29Z","abstract_excerpt":"We investigate model independent upper bounds on total proton lifetime in the context of Grand Unified Theories with the Standard Model matter content. We find them to be $\\tau_p \\leq 1.5^{+0.5}_{-0.3} \\times 10^{39} \\ \\frac{(M_X/10^{16} \\textrm{GeV})^4}{\\alpha_{GUT}^2} (0.003 \\textrm{GeV}^3 / \\alpha)^2 \\textrm{years}$ and $\\tau_p \\leq 7.1^{+0.0}_{-0.0} \\times 10^{36} \\ \\frac{(M_X/10^{16} \\textrm{GeV})^4}{\\alpha_{GUT}^2} (0.003 \\textrm{GeV}^3 / \\alpha)^2 \\textrm{years}$ in the Majorana and Dirac neutrino case, respectively. These bounds, in conjunction with experimental limits, put lower limit"},"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/0410198","kind":"arxiv","version":4},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2004-10-13T16:48:29Z","cross_cats_sorted":["hep-ex","hep-th"],"title_canon_sha256":"9db50b7bd129ce5fa869f92188b67ae881560d97e0529a5053068d747543d213","abstract_canon_sha256":"af635f25528d9cec82768c69ce5214a3abd48624ffae793fd31de986310fc8ff"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:23:10.731190Z","signature_b64":"BRcDko99xfCIVFeaPgcgS3i7Yd9MFpEsmqaZ0roU2WXRF9EwEDwSsNckE2YY66n7+4hSA9bnkzL7DZ10we9HCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"21820e17ecb3f3bea09faedc1830478db5201f1656cd5fbc38d90b5f16b6f5a9","last_reissued_at":"2026-07-04T15:23:10.730773Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:23:10.730773Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"How Long Could We Live?","license":"","headline":"","cross_cats":["hep-ex","hep-th"],"primary_cat":"hep-ph","authors_text":"Ilja Dorsner, Pavel Fileviez Perez","submitted_at":"2004-10-13T16:48:29Z","abstract_excerpt":"We investigate model independent upper bounds on total proton lifetime in the context of Grand Unified Theories with the Standard Model matter content. We find them to be $\\tau_p \\leq 1.5^{+0.5}_{-0.3} \\times 10^{39} \\ \\frac{(M_X/10^{16} \\textrm{GeV})^4}{\\alpha_{GUT}^2} (0.003 \\textrm{GeV}^3 / \\alpha)^2 \\textrm{years}$ and $\\tau_p \\leq 7.1^{+0.0}_{-0.0} \\times 10^{36} \\ \\frac{(M_X/10^{16} \\textrm{GeV})^4}{\\alpha_{GUT}^2} (0.003 \\textrm{GeV}^3 / \\alpha)^2 \\textrm{years}$ in the Majorana and Dirac neutrino case, respectively. These bounds, in conjunction with experimental limits, put lower limit"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0410198","kind":"arxiv","version":4},"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/0410198/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/0410198","created_at":"2026-07-04T15:23:10.730836+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0410198v4","created_at":"2026-07-04T15:23:10.730836+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0410198","created_at":"2026-07-04T15:23:10.730836+00:00"},{"alias_kind":"pith_short_12","alias_value":"EGBA4F7MWPZ3","created_at":"2026-07-04T15:23:10.730836+00:00"},{"alias_kind":"pith_short_16","alias_value":"EGBA4F7MWPZ35IE7","created_at":"2026-07-04T15:23:10.730836+00:00"},{"alias_kind":"pith_short_8","alias_value":"EGBA4F7M","created_at":"2026-07-04T15:23:10.730836+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2504.16022","citing_title":"Non-Renormalizable SU(5) GUTs: Leptoquark-Induced Neutrino Masses","ref_index":14,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EGBA4F7MWPZ35IE7V3OBQMCHRW","json":"https://pith.science/pith/EGBA4F7MWPZ35IE7V3OBQMCHRW.json","graph_json":"https://pith.science/api/pith-number/EGBA4F7MWPZ35IE7V3OBQMCHRW/graph.json","events_json":"https://pith.science/api/pith-number/EGBA4F7MWPZ35IE7V3OBQMCHRW/events.json","paper":"https://pith.science/paper/EGBA4F7M"},"agent_actions":{"view_html":"https://pith.science/pith/EGBA4F7MWPZ35IE7V3OBQMCHRW","download_json":"https://pith.science/pith/EGBA4F7MWPZ35IE7V3OBQMCHRW.json","view_paper":"https://pith.science/paper/EGBA4F7M","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0410198&json=true","fetch_graph":"https://pith.science/api/pith-number/EGBA4F7MWPZ35IE7V3OBQMCHRW/graph.json","fetch_events":"https://pith.science/api/pith-number/EGBA4F7MWPZ35IE7V3OBQMCHRW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EGBA4F7MWPZ35IE7V3OBQMCHRW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EGBA4F7MWPZ35IE7V3OBQMCHRW/action/storage_attestation","attest_author":"https://pith.science/pith/EGBA4F7MWPZ35IE7V3OBQMCHRW/action/author_attestation","sign_citation":"https://pith.science/pith/EGBA4F7MWPZ35IE7V3OBQMCHRW/action/citation_signature","submit_replication":"https://pith.science/pith/EGBA4F7MWPZ35IE7V3OBQMCHRW/action/replication_record"}},"created_at":"2026-07-04T15:23:10.730836+00:00","updated_at":"2026-07-04T15:23:10.730836+00:00"}