{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:YNK3JZVL37OXC63TT4RJAPA7HO","short_pith_number":"pith:YNK3JZVL","schema_version":"1.0","canonical_sha256":"c355b4e6abdfdd717b739f22903c1f3ba51b7db0c8f3b0b7b51fa13cd0a2d311","source":{"kind":"arxiv","id":"hep-th/0405159","version":2},"attestation_state":"computed","paper":{"title":"Supersymmetric Unification Without Low Energy Supersymmetry And Signatures for Fine-Tuning at the LHC","license":"","headline":"","cross_cats":["astro-ph","hep-ph"],"primary_cat":"hep-th","authors_text":"Nima Arkani-Hamed, Savas Dimopoulos","submitted_at":"2004-05-18T19:46:33Z","abstract_excerpt":"The cosmological constant problem is a failure of naturalness and suggests that a fine-tuning mechanism is at work, which may also address the hierarchy problem. An example -- supported by Weinberg's successful prediction of the cosmological constant -- is the potentially vast landscape of vacua in string theory, where the existence of galaxies and atoms is promoted to a vacuum selection criterion. Then, low energy SUSY becomes unnecessary, and supersymmetry -- if present in the fundamental theory -- can be broken near the unification scale. All the scalars of the supersymmetric standard model"},"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-th/0405159","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2004-05-18T19:46:33Z","cross_cats_sorted":["astro-ph","hep-ph"],"title_canon_sha256":"fc5f425681b6215537674b47e14a62e38266fcef6b140fc8a891917d407c6339","abstract_canon_sha256":"f8d13918535e25f02475243d2ad8c1582cbcd82f622eb82626975830708310e6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:48:48.511373Z","signature_b64":"8zByIW81xzHaHuM7maqhHKXa/l5aNg6idptXQAwc+CHY0JSSwzmhunyMDhJ59a3C267zTOCTNnBZYeHQHdUhBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c355b4e6abdfdd717b739f22903c1f3ba51b7db0c8f3b0b7b51fa13cd0a2d311","last_reissued_at":"2026-07-04T16:48:48.510933Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:48:48.510933Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Supersymmetric Unification Without Low Energy Supersymmetry And Signatures for Fine-Tuning at the LHC","license":"","headline":"","cross_cats":["astro-ph","hep-ph"],"primary_cat":"hep-th","authors_text":"Nima Arkani-Hamed, Savas Dimopoulos","submitted_at":"2004-05-18T19:46:33Z","abstract_excerpt":"The cosmological constant problem is a failure of naturalness and suggests that a fine-tuning mechanism is at work, which may also address the hierarchy problem. An example -- supported by Weinberg's successful prediction of the cosmological constant -- is the potentially vast landscape of vacua in string theory, where the existence of galaxies and atoms is promoted to a vacuum selection criterion. Then, low energy SUSY becomes unnecessary, and supersymmetry -- if present in the fundamental theory -- can be broken near the unification scale. All the scalars of the supersymmetric standard model"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0405159","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/hep-th/0405159/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-th/0405159","created_at":"2026-07-04T16:48:48.511008+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0405159v2","created_at":"2026-07-04T16:48:48.511008+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0405159","created_at":"2026-07-04T16:48:48.511008+00:00"},{"alias_kind":"pith_short_12","alias_value":"YNK3JZVL37OX","created_at":"2026-07-04T16:48:48.511008+00:00"},{"alias_kind":"pith_short_16","alias_value":"YNK3JZVL37OXC63T","created_at":"2026-07-04T16:48:48.511008+00:00"},{"alias_kind":"pith_short_8","alias_value":"YNK3JZVL","created_at":"2026-07-04T16:48:48.511008+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":7,"sample":[{"citing_arxiv_id":"2606.05299","citing_title":"Heavy-element paleodetectors for Higgsino dark matter","ref_index":45,"is_internal_anchor":true},{"citing_arxiv_id":"1906.08721","citing_title":"Renormalization Effects on Electric Dipole Moments in Electroweakly Interacting Massive Particle Models","ref_index":6,"is_internal_anchor":true},{"citing_arxiv_id":"2506.05201","citing_title":"SUSY meets SMEFT: Complete one-loop matching of the general MSSM","ref_index":71,"is_internal_anchor":true},{"citing_arxiv_id":"2510.21420","citing_title":"The Standard Model partial unification scale as a guide to new physics model building","ref_index":14,"is_internal_anchor":true},{"citing_arxiv_id":"2512.11026","citing_title":"Weak Scale Triggers in the SMEFT","ref_index":56,"is_internal_anchor":true},{"citing_arxiv_id":"2601.11180","citing_title":"Fine-tunings in radiative $\\alpha$-particle capture on $^{12}$C at astrophysical energies","ref_index":3,"is_internal_anchor":true},{"citing_arxiv_id":"2603.01411","citing_title":"Naturalness and Fisher Information","ref_index":12,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YNK3JZVL37OXC63TT4RJAPA7HO","json":"https://pith.science/pith/YNK3JZVL37OXC63TT4RJAPA7HO.json","graph_json":"https://pith.science/api/pith-number/YNK3JZVL37OXC63TT4RJAPA7HO/graph.json","events_json":"https://pith.science/api/pith-number/YNK3JZVL37OXC63TT4RJAPA7HO/events.json","paper":"https://pith.science/paper/YNK3JZVL"},"agent_actions":{"view_html":"https://pith.science/pith/YNK3JZVL37OXC63TT4RJAPA7HO","download_json":"https://pith.science/pith/YNK3JZVL37OXC63TT4RJAPA7HO.json","view_paper":"https://pith.science/paper/YNK3JZVL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0405159&json=true","fetch_graph":"https://pith.science/api/pith-number/YNK3JZVL37OXC63TT4RJAPA7HO/graph.json","fetch_events":"https://pith.science/api/pith-number/YNK3JZVL37OXC63TT4RJAPA7HO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YNK3JZVL37OXC63TT4RJAPA7HO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YNK3JZVL37OXC63TT4RJAPA7HO/action/storage_attestation","attest_author":"https://pith.science/pith/YNK3JZVL37OXC63TT4RJAPA7HO/action/author_attestation","sign_citation":"https://pith.science/pith/YNK3JZVL37OXC63TT4RJAPA7HO/action/citation_signature","submit_replication":"https://pith.science/pith/YNK3JZVL37OXC63TT4RJAPA7HO/action/replication_record"}},"created_at":"2026-07-04T16:48:48.511008+00:00","updated_at":"2026-07-04T16:48:48.511008+00:00"}