{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:CD3GTWHXHVVB2EBG55B52F6AUG","short_pith_number":"pith:CD3GTWHX","schema_version":"1.0","canonical_sha256":"10f669d8f73d6a1d1026ef43dd17c0a1a5c328a9ca3d53e11563b48ffdafe4b4","source":{"kind":"arxiv","id":"1401.1825","version":1},"attestation_state":"computed","paper":{"title":"Probing Light Nonthermal Dark Matter at the LHC","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Bhaskar Dutta, Teruki Kamon, Yu Gao","submitted_at":"2014-01-08T21:00:39Z","abstract_excerpt":"This paper investigates the collider phenomenolgy of a minimal nonthermal dark matter model with a 1-GeV dark matter candidate, which naturally explain baryongensis. Since the light dark matter is not parity-protected, it can be singly produced at the LHC. This leads to large missing energy associated with an energetic jet whose transverse momentum distribution is featured by a Jacobian-like shape. The monojet, dijet, paired dijet and 2 jets + missing energy channels are studied. Currently existing data at Tevatron and LHC offer significant bounds on our 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":"1401.1825","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-01-08T21:00:39Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"8ed619aad3b10fb14e7439ee77285edcfce3fa3abb23835f05e3c25f1c1a177f","abstract_canon_sha256":"58670c7b89dfd06ee8209948faea8c4001a002ea59f03654d712c77eaab0b70a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:50:02.806522Z","signature_b64":"3PpX1tfP/MlHwe0TOjdqWT7/pCiROUz3eI1hkxQnFEHVh1FnVEPcvWFDwzy4gfkxxzo2p9tawA6r5yozWFk8Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"10f669d8f73d6a1d1026ef43dd17c0a1a5c328a9ca3d53e11563b48ffdafe4b4","last_reissued_at":"2026-05-18T02:50:02.805844Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:50:02.805844Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing Light Nonthermal Dark Matter at the LHC","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Bhaskar Dutta, Teruki Kamon, Yu Gao","submitted_at":"2014-01-08T21:00:39Z","abstract_excerpt":"This paper investigates the collider phenomenolgy of a minimal nonthermal dark matter model with a 1-GeV dark matter candidate, which naturally explain baryongensis. Since the light dark matter is not parity-protected, it can be singly produced at the LHC. This leads to large missing energy associated with an energetic jet whose transverse momentum distribution is featured by a Jacobian-like shape. The monojet, dijet, paired dijet and 2 jets + missing energy channels are studied. Currently existing data at Tevatron and LHC offer significant bounds on our model."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1401.1825","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":"1401.1825","created_at":"2026-05-18T02:50:02.805914+00:00"},{"alias_kind":"arxiv_version","alias_value":"1401.1825v1","created_at":"2026-05-18T02:50:02.805914+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1401.1825","created_at":"2026-05-18T02:50:02.805914+00:00"},{"alias_kind":"pith_short_12","alias_value":"CD3GTWHXHVVB","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_16","alias_value":"CD3GTWHXHVVB2EBG","created_at":"2026-05-18T12:28:22.404517+00:00"},{"alias_kind":"pith_short_8","alias_value":"CD3GTWHX","created_at":"2026-05-18T12:28:22.404517+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.06796","citing_title":"Decaying spin-3/2 dark matter from baryon number violation","ref_index":119,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CD3GTWHXHVVB2EBG55B52F6AUG","json":"https://pith.science/pith/CD3GTWHXHVVB2EBG55B52F6AUG.json","graph_json":"https://pith.science/api/pith-number/CD3GTWHXHVVB2EBG55B52F6AUG/graph.json","events_json":"https://pith.science/api/pith-number/CD3GTWHXHVVB2EBG55B52F6AUG/events.json","paper":"https://pith.science/paper/CD3GTWHX"},"agent_actions":{"view_html":"https://pith.science/pith/CD3GTWHXHVVB2EBG55B52F6AUG","download_json":"https://pith.science/pith/CD3GTWHXHVVB2EBG55B52F6AUG.json","view_paper":"https://pith.science/paper/CD3GTWHX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1401.1825&json=true","fetch_graph":"https://pith.science/api/pith-number/CD3GTWHXHVVB2EBG55B52F6AUG/graph.json","fetch_events":"https://pith.science/api/pith-number/CD3GTWHXHVVB2EBG55B52F6AUG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CD3GTWHXHVVB2EBG55B52F6AUG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CD3GTWHXHVVB2EBG55B52F6AUG/action/storage_attestation","attest_author":"https://pith.science/pith/CD3GTWHXHVVB2EBG55B52F6AUG/action/author_attestation","sign_citation":"https://pith.science/pith/CD3GTWHXHVVB2EBG55B52F6AUG/action/citation_signature","submit_replication":"https://pith.science/pith/CD3GTWHXHVVB2EBG55B52F6AUG/action/replication_record"}},"created_at":"2026-05-18T02:50:02.805914+00:00","updated_at":"2026-05-18T02:50:02.805914+00:00"}