{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2007:4DWAF3GCNKQYJK2PPGVD75MF36","short_pith_number":"pith:4DWAF3GC","schema_version":"1.0","canonical_sha256":"e0ec02ecc26aa184ab4f79aa3ff585dfa85a35f0f17e7d735eb9dca911593a8f","source":{"kind":"arxiv","id":"0709.4477","version":1},"attestation_state":"computed","paper":{"title":"Sneutrino cold dark matter, a new analysis: relic abundance and detection rates","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"hep-ph","authors_text":"Chiara Arina, INFN/Torino), Nicolao Fornengo (Department of Theoretical Physics, University of Torino","submitted_at":"2007-09-27T19:10:16Z","abstract_excerpt":"We perform a new and updated analysis of sneutrinos as dark matter candidates, in different classes of supersymmetric models. We extend previous analyses by studying sneutrino phenomenology for full variations of the supersymmetric parameters which define the various models. We first revisit the standard Minimal Supersymmetric Standard Model, concluding that sneutrinos are marginally compatible with existing experimental bounds, including direct detection, provided they compose a subdominant component of dark matter. We then study supersymmetric models with the inclusion of right-handed fields"},"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":"0709.4477","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2007-09-27T19:10:16Z","cross_cats_sorted":["astro-ph"],"title_canon_sha256":"58d200350fc38e25f0a100c2a3e1e3188f9f16f53ac8cdc23f4f0cc70a9c2a1e","abstract_canon_sha256":"eda34036a37e3d05e9cc843a51de01442a9bb2019047676b7dd0a76aa7a06495"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:35:24.737306Z","signature_b64":"dzkZ+kKWqalS0u3WerZWedcO9wf4PDEyqkUma2jJNZnu2g1JO/DBfqlyDpdntNp4PoawIKD/L04vfuQjD0FPAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e0ec02ecc26aa184ab4f79aa3ff585dfa85a35f0f17e7d735eb9dca911593a8f","last_reissued_at":"2026-07-04T15:35:24.736918Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:35:24.736918Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Sneutrino cold dark matter, a new analysis: relic abundance and detection rates","license":"","headline":"","cross_cats":["astro-ph"],"primary_cat":"hep-ph","authors_text":"Chiara Arina, INFN/Torino), Nicolao Fornengo (Department of Theoretical Physics, University of Torino","submitted_at":"2007-09-27T19:10:16Z","abstract_excerpt":"We perform a new and updated analysis of sneutrinos as dark matter candidates, in different classes of supersymmetric models. We extend previous analyses by studying sneutrino phenomenology for full variations of the supersymmetric parameters which define the various models. We first revisit the standard Minimal Supersymmetric Standard Model, concluding that sneutrinos are marginally compatible with existing experimental bounds, including direct detection, provided they compose a subdominant component of dark matter. We then study supersymmetric models with the inclusion of right-handed fields"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0709.4477","kind":"arxiv","version":1},"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/0709.4477/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":"0709.4477","created_at":"2026-07-04T15:35:24.736976+00:00"},{"alias_kind":"arxiv_version","alias_value":"0709.4477v1","created_at":"2026-07-04T15:35:24.736976+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0709.4477","created_at":"2026-07-04T15:35:24.736976+00:00"},{"alias_kind":"pith_short_12","alias_value":"4DWAF3GCNKQY","created_at":"2026-07-04T15:35:24.736976+00:00"},{"alias_kind":"pith_short_16","alias_value":"4DWAF3GCNKQYJK2P","created_at":"2026-07-04T15:35:24.736976+00:00"},{"alias_kind":"pith_short_8","alias_value":"4DWAF3GC","created_at":"2026-07-04T15:35:24.736976+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2604.21996","citing_title":"Solar Reflection of Inelastic Dark Matter","ref_index":8,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4DWAF3GCNKQYJK2PPGVD75MF36","json":"https://pith.science/pith/4DWAF3GCNKQYJK2PPGVD75MF36.json","graph_json":"https://pith.science/api/pith-number/4DWAF3GCNKQYJK2PPGVD75MF36/graph.json","events_json":"https://pith.science/api/pith-number/4DWAF3GCNKQYJK2PPGVD75MF36/events.json","paper":"https://pith.science/paper/4DWAF3GC"},"agent_actions":{"view_html":"https://pith.science/pith/4DWAF3GCNKQYJK2PPGVD75MF36","download_json":"https://pith.science/pith/4DWAF3GCNKQYJK2PPGVD75MF36.json","view_paper":"https://pith.science/paper/4DWAF3GC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0709.4477&json=true","fetch_graph":"https://pith.science/api/pith-number/4DWAF3GCNKQYJK2PPGVD75MF36/graph.json","fetch_events":"https://pith.science/api/pith-number/4DWAF3GCNKQYJK2PPGVD75MF36/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4DWAF3GCNKQYJK2PPGVD75MF36/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4DWAF3GCNKQYJK2PPGVD75MF36/action/storage_attestation","attest_author":"https://pith.science/pith/4DWAF3GCNKQYJK2PPGVD75MF36/action/author_attestation","sign_citation":"https://pith.science/pith/4DWAF3GCNKQYJK2PPGVD75MF36/action/citation_signature","submit_replication":"https://pith.science/pith/4DWAF3GCNKQYJK2PPGVD75MF36/action/replication_record"}},"created_at":"2026-07-04T15:35:24.736976+00:00","updated_at":"2026-07-04T15:35:24.736976+00:00"}