{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:5RYD4JQ3HLMYBDWWCJGNU7SUXY","short_pith_number":"pith:5RYD4JQ3","schema_version":"1.0","canonical_sha256":"ec703e261b3ad9808ed6124cda7e54be0fbdb34e6aabf22514729830753da19d","source":{"kind":"arxiv","id":"1202.6088","version":2},"attestation_state":"computed","paper":{"title":"Electroweak Supersymmetry around the Electroweak Scale","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Chunli Tong, Dimitri V. Nanopoulos, Jinmian Li, Taoli Cheng, Tianjun Li","submitted_at":"2012-02-27T23:11:08Z","abstract_excerpt":"Inspired by the phenomenological constraints, LHC supersymmetry and Higgs searches, dark matter search as well as string model building, we propose the electroweak supersymmetry around the electroweak scale: the squarks and/or gluinos are around a few TeV while the sleptons, sneutrinos, bino and winos are within one TeV. The Higgsinos can be either heavy or light. We consider bino as the dominant component of dark matter candidate, and the observed dark matter relic density is achieved via the neutralino-stau coannihilations. Considering the Generalized Minimal Supergravity (GmSUGRA), we show "},"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":"1202.6088","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2012-02-27T23:11:08Z","cross_cats_sorted":[],"title_canon_sha256":"4214779c86d0eb3aa5401c8f57be91ff222a5fb99fd13eba33ee1dee8d17aa80","abstract_canon_sha256":"6f4744474b22b8dcc790a4b7545362267792303ea261b2777aa90c034af7316a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:18.958306Z","signature_b64":"3o7Ag+ugsG+HGCrxTBrgjVuZu85Fnv3oRZLG6Z4GJe0wtUk6bfJjRsfWXLZ9v4LZ7V/mQNpkzNntWlRL0zvFAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ec703e261b3ad9808ed6124cda7e54be0fbdb34e6aabf22514729830753da19d","last_reissued_at":"2026-05-18T01:58:18.957600Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:18.957600Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Electroweak Supersymmetry around the Electroweak Scale","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Chunli Tong, Dimitri V. Nanopoulos, Jinmian Li, Taoli Cheng, Tianjun Li","submitted_at":"2012-02-27T23:11:08Z","abstract_excerpt":"Inspired by the phenomenological constraints, LHC supersymmetry and Higgs searches, dark matter search as well as string model building, we propose the electroweak supersymmetry around the electroweak scale: the squarks and/or gluinos are around a few TeV while the sleptons, sneutrinos, bino and winos are within one TeV. The Higgsinos can be either heavy or light. We consider bino as the dominant component of dark matter candidate, and the observed dark matter relic density is achieved via the neutralino-stau coannihilations. Considering the Generalized Minimal Supergravity (GmSUGRA), we show "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1202.6088","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":""},"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":"1202.6088","created_at":"2026-05-18T01:58:18.957705+00:00"},{"alias_kind":"arxiv_version","alias_value":"1202.6088v2","created_at":"2026-05-18T01:58:18.957705+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1202.6088","created_at":"2026-05-18T01:58:18.957705+00:00"},{"alias_kind":"pith_short_12","alias_value":"5RYD4JQ3HLMY","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_16","alias_value":"5RYD4JQ3HLMYBDWW","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_8","alias_value":"5RYD4JQ3","created_at":"2026-05-18T12:26:56.085431+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.12039","citing_title":"The Light Neutralino Dark Matter in the Generalized Minimal Supergravity (GmSUGRA)","ref_index":50,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5RYD4JQ3HLMYBDWWCJGNU7SUXY","json":"https://pith.science/pith/5RYD4JQ3HLMYBDWWCJGNU7SUXY.json","graph_json":"https://pith.science/api/pith-number/5RYD4JQ3HLMYBDWWCJGNU7SUXY/graph.json","events_json":"https://pith.science/api/pith-number/5RYD4JQ3HLMYBDWWCJGNU7SUXY/events.json","paper":"https://pith.science/paper/5RYD4JQ3"},"agent_actions":{"view_html":"https://pith.science/pith/5RYD4JQ3HLMYBDWWCJGNU7SUXY","download_json":"https://pith.science/pith/5RYD4JQ3HLMYBDWWCJGNU7SUXY.json","view_paper":"https://pith.science/paper/5RYD4JQ3","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1202.6088&json=true","fetch_graph":"https://pith.science/api/pith-number/5RYD4JQ3HLMYBDWWCJGNU7SUXY/graph.json","fetch_events":"https://pith.science/api/pith-number/5RYD4JQ3HLMYBDWWCJGNU7SUXY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5RYD4JQ3HLMYBDWWCJGNU7SUXY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5RYD4JQ3HLMYBDWWCJGNU7SUXY/action/storage_attestation","attest_author":"https://pith.science/pith/5RYD4JQ3HLMYBDWWCJGNU7SUXY/action/author_attestation","sign_citation":"https://pith.science/pith/5RYD4JQ3HLMYBDWWCJGNU7SUXY/action/citation_signature","submit_replication":"https://pith.science/pith/5RYD4JQ3HLMYBDWWCJGNU7SUXY/action/replication_record"}},"created_at":"2026-05-18T01:58:18.957705+00:00","updated_at":"2026-05-18T01:58:18.957705+00:00"}