{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:G6LGEMDT5MCM6JAIMEHXEPG7W4","short_pith_number":"pith:G6LGEMDT","schema_version":"1.0","canonical_sha256":"3796623073eb04cf2408610f723cdfb714ec440351b76c650805daefddcf957a","source":{"kind":"arxiv","id":"1412.4789","version":3},"attestation_state":"computed","paper":{"title":"The Relic Neutralino Surface at a 100 TeV collider","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Adam Martin, Bryan Ostdiek, Joseph Bramante, Michihisa Takeuchi, Patrick J. Fox, Tilman Plehn, Torben Schell","submitted_at":"2014-12-15T21:01:13Z","abstract_excerpt":"We map the parameter space for MSSM neutralino dark matter which freezes out to the observed relic abundance, in the limit that all superpartners except the neutralinos and charginos are decoupled. In this space of relic neutralinos, we show the dominant dark matter annihilation modes, the mass splittings among the electroweakinos, direct detection rates, and collider cross-sections. The mass difference between the dark matter and the next-to-lightest neutral and charged states is typically much less than electroweak gauge boson masses. With these small mass differences, the relic neutralino s"},"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":"1412.4789","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-12-15T21:01:13Z","cross_cats_sorted":["astro-ph.CO","hep-ex"],"title_canon_sha256":"8477a800a52ceda46dfe326811ca1645c65e372e86360c566bc3bbf03bce27a9","abstract_canon_sha256":"2202e02febb3af752d1763ff83f151fef27e92fc8316f000c86032e91d0e8f9e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:20:12.311770Z","signature_b64":"uAmV+4lh3Nk82/rZ5JkZP77Jb8Xam/ow0S74Qc/NiN35s9ZXxvQM9OnOiCS/SJ36ECKKg7QgeBItaygFbH2JAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3796623073eb04cf2408610f723cdfb714ec440351b76c650805daefddcf957a","last_reissued_at":"2026-05-18T02:20:12.311339Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:20:12.311339Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Relic Neutralino Surface at a 100 TeV collider","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ex"],"primary_cat":"hep-ph","authors_text":"Adam Martin, Bryan Ostdiek, Joseph Bramante, Michihisa Takeuchi, Patrick J. Fox, Tilman Plehn, Torben Schell","submitted_at":"2014-12-15T21:01:13Z","abstract_excerpt":"We map the parameter space for MSSM neutralino dark matter which freezes out to the observed relic abundance, in the limit that all superpartners except the neutralinos and charginos are decoupled. In this space of relic neutralinos, we show the dominant dark matter annihilation modes, the mass splittings among the electroweakinos, direct detection rates, and collider cross-sections. The mass difference between the dark matter and the next-to-lightest neutral and charged states is typically much less than electroweak gauge boson masses. With these small mass differences, the relic neutralino s"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1412.4789","kind":"arxiv","version":3},"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":"1412.4789","created_at":"2026-05-18T02:20:12.311405+00:00"},{"alias_kind":"arxiv_version","alias_value":"1412.4789v3","created_at":"2026-05-18T02:20:12.311405+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1412.4789","created_at":"2026-05-18T02:20:12.311405+00:00"},{"alias_kind":"pith_short_12","alias_value":"G6LGEMDT5MCM","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_16","alias_value":"G6LGEMDT5MCM6JAI","created_at":"2026-05-18T12:28:28.263976+00:00"},{"alias_kind":"pith_short_8","alias_value":"G6LGEMDT","created_at":"2026-05-18T12:28:28.263976+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1907.11326","citing_title":"Higgs Assisted Razor Search for Higgsinos at a 100 TeV pp Collider","ref_index":31,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/G6LGEMDT5MCM6JAIMEHXEPG7W4","json":"https://pith.science/pith/G6LGEMDT5MCM6JAIMEHXEPG7W4.json","graph_json":"https://pith.science/api/pith-number/G6LGEMDT5MCM6JAIMEHXEPG7W4/graph.json","events_json":"https://pith.science/api/pith-number/G6LGEMDT5MCM6JAIMEHXEPG7W4/events.json","paper":"https://pith.science/paper/G6LGEMDT"},"agent_actions":{"view_html":"https://pith.science/pith/G6LGEMDT5MCM6JAIMEHXEPG7W4","download_json":"https://pith.science/pith/G6LGEMDT5MCM6JAIMEHXEPG7W4.json","view_paper":"https://pith.science/paper/G6LGEMDT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1412.4789&json=true","fetch_graph":"https://pith.science/api/pith-number/G6LGEMDT5MCM6JAIMEHXEPG7W4/graph.json","fetch_events":"https://pith.science/api/pith-number/G6LGEMDT5MCM6JAIMEHXEPG7W4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G6LGEMDT5MCM6JAIMEHXEPG7W4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G6LGEMDT5MCM6JAIMEHXEPG7W4/action/storage_attestation","attest_author":"https://pith.science/pith/G6LGEMDT5MCM6JAIMEHXEPG7W4/action/author_attestation","sign_citation":"https://pith.science/pith/G6LGEMDT5MCM6JAIMEHXEPG7W4/action/citation_signature","submit_replication":"https://pith.science/pith/G6LGEMDT5MCM6JAIMEHXEPG7W4/action/replication_record"}},"created_at":"2026-05-18T02:20:12.311405+00:00","updated_at":"2026-05-18T02:20:12.311405+00:00"}