{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:WWKSFE3X5STZQTKJAR34SDZDED","short_pith_number":"pith:WWKSFE3X","schema_version":"1.0","canonical_sha256":"b595229377eca7984d490477c90f2320d78295bd1c8f428564d75a302da36593","source":{"kind":"arxiv","id":"1701.04436","version":1},"attestation_state":"computed","paper":{"title":"Dark Matter in B-L Supersymmetric Standard Model with Inverse Seesaw","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"S. Khalil, W. Abdallah","submitted_at":"2017-01-16T19:42:40Z","abstract_excerpt":"We show that the $B-L$ Supersymmetric Standard Model with Inverse Seesaw (BLSSMIS) provides new Dark Matter (DM) candidates (lightest right-handed sneutrino and lightest $B-L$ neutralino) with mass of order few hundreds GeV, while most of other SUSY spectrum can be quite heavy, consistently with the current Large Hadron Collider (LHC) constraints. We emphasize that the thermal relic abundance and direct detection experiments via relic neutralino scattering with nuclei impose stringent constraints on the $B-L$ neutralinos. These constraints can be satisfied by few points in the parameter space "},"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":"1701.04436","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2017-01-16T19:42:40Z","cross_cats_sorted":[],"title_canon_sha256":"879cdb1275dad61a1af78a1a36215ef8a75ed0ede977667a8f63a18a981c0b2c","abstract_canon_sha256":"b5eccbab7b6ea7cfc5e2170cb3faa5f446a2a5644e216a12dc59dda266f1d499"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:46:22.319043Z","signature_b64":"ld1D24Zb9CWQFfTnUkUMJTs//y5NI/NQlSxON9lTbVt0STPwiq0aaBh7BFX87w6lt0p55SL4LUBdFlbSHxL6AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b595229377eca7984d490477c90f2320d78295bd1c8f428564d75a302da36593","last_reissued_at":"2026-05-18T00:46:22.318671Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:46:22.318671Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark Matter in B-L Supersymmetric Standard Model with Inverse Seesaw","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"S. Khalil, W. Abdallah","submitted_at":"2017-01-16T19:42:40Z","abstract_excerpt":"We show that the $B-L$ Supersymmetric Standard Model with Inverse Seesaw (BLSSMIS) provides new Dark Matter (DM) candidates (lightest right-handed sneutrino and lightest $B-L$ neutralino) with mass of order few hundreds GeV, while most of other SUSY spectrum can be quite heavy, consistently with the current Large Hadron Collider (LHC) constraints. We emphasize that the thermal relic abundance and direct detection experiments via relic neutralino scattering with nuclei impose stringent constraints on the $B-L$ neutralinos. These constraints can be satisfied by few points in the parameter space "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.04436","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":""},"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":"1701.04436","created_at":"2026-05-18T00:46:22.318731+00:00"},{"alias_kind":"arxiv_version","alias_value":"1701.04436v1","created_at":"2026-05-18T00:46:22.318731+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.04436","created_at":"2026-05-18T00:46:22.318731+00:00"},{"alias_kind":"pith_short_12","alias_value":"WWKSFE3X5STZ","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_16","alias_value":"WWKSFE3X5STZQTKJ","created_at":"2026-05-18T12:31:53.515858+00:00"},{"alias_kind":"pith_short_8","alias_value":"WWKSFE3X","created_at":"2026-05-18T12:31:53.515858+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.19293","citing_title":"The $Z'$-boson of the $B-L$ Supersymmetric Standard Model and its Large Hadron Collider Searches","ref_index":80,"is_internal_anchor":true},{"citing_arxiv_id":"2604.23038","citing_title":"Mono-Z' Signatures in the B-L Supersymmetric Standard Model at the LHC","ref_index":13,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WWKSFE3X5STZQTKJAR34SDZDED","json":"https://pith.science/pith/WWKSFE3X5STZQTKJAR34SDZDED.json","graph_json":"https://pith.science/api/pith-number/WWKSFE3X5STZQTKJAR34SDZDED/graph.json","events_json":"https://pith.science/api/pith-number/WWKSFE3X5STZQTKJAR34SDZDED/events.json","paper":"https://pith.science/paper/WWKSFE3X"},"agent_actions":{"view_html":"https://pith.science/pith/WWKSFE3X5STZQTKJAR34SDZDED","download_json":"https://pith.science/pith/WWKSFE3X5STZQTKJAR34SDZDED.json","view_paper":"https://pith.science/paper/WWKSFE3X","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1701.04436&json=true","fetch_graph":"https://pith.science/api/pith-number/WWKSFE3X5STZQTKJAR34SDZDED/graph.json","fetch_events":"https://pith.science/api/pith-number/WWKSFE3X5STZQTKJAR34SDZDED/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WWKSFE3X5STZQTKJAR34SDZDED/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WWKSFE3X5STZQTKJAR34SDZDED/action/storage_attestation","attest_author":"https://pith.science/pith/WWKSFE3X5STZQTKJAR34SDZDED/action/author_attestation","sign_citation":"https://pith.science/pith/WWKSFE3X5STZQTKJAR34SDZDED/action/citation_signature","submit_replication":"https://pith.science/pith/WWKSFE3X5STZQTKJAR34SDZDED/action/replication_record"}},"created_at":"2026-05-18T00:46:22.318731+00:00","updated_at":"2026-05-18T00:46:22.318731+00:00"}