{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:PLO4WSFDVADHHFDXEUJGJDZVWN","short_pith_number":"pith:PLO4WSFD","schema_version":"1.0","canonical_sha256":"7addcb48a3a8067394772512648f35b3534d55df3a39c0ce1ee19cf21596d6fd","source":{"kind":"arxiv","id":"2003.03379","version":1},"attestation_state":"computed","paper":{"title":"On sub-GeV Dark Matter Production at Fixed-Target Experiments","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Adam Ritz, Asher Berlin, Natalia Toro, Patrick deNiverville, Philip Schuster","submitted_at":"2020-03-06T19:00:00Z","abstract_excerpt":"We analyze the sensitivity of fixed-target experiments to sub-GeV thermal relic dark matter models, accounting for variations in both mediator and dark matter mass, and including dark matter production through both on- and off-shell mediators. It is commonly thought that the sensitivity of such experiments is predicated on the existence of an on-shell mediator that is produced and then decays to dark matter. While accelerators do provide a unique opportunity to probe the mediator directly, our analysis demonstrates that their sensitivity extends beyond this commonly discussed regime. In partic"},"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":"2003.03379","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2020-03-06T19:00:00Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"316388b742acf6a96a0f68de2be09a1d10a4a32746aedb2714e85515b1c5a357","abstract_canon_sha256":"1f815bbd2345a3b32bae68331b8a90a518c6c826253ad09c3bd6083248fc107b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:52:16.855871Z","signature_b64":"uzjfCeZTnw2ZH6TO5NWNTWpRN0jqIdq5j53NHnJ6gI2PmhrhEyCi4A+JhkDouTsh1wH2kbNPyOpLGABmW6cFCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7addcb48a3a8067394772512648f35b3534d55df3a39c0ce1ee19cf21596d6fd","last_reissued_at":"2026-07-05T01:52:16.855414Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:52:16.855414Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On sub-GeV Dark Matter Production at Fixed-Target Experiments","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Adam Ritz, Asher Berlin, Natalia Toro, Patrick deNiverville, Philip Schuster","submitted_at":"2020-03-06T19:00:00Z","abstract_excerpt":"We analyze the sensitivity of fixed-target experiments to sub-GeV thermal relic dark matter models, accounting for variations in both mediator and dark matter mass, and including dark matter production through both on- and off-shell mediators. It is commonly thought that the sensitivity of such experiments is predicated on the existence of an on-shell mediator that is produced and then decays to dark matter. While accelerators do provide a unique opportunity to probe the mediator directly, our analysis demonstrates that their sensitivity extends beyond this commonly discussed regime. In partic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2003.03379","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/2003.03379/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":"2003.03379","created_at":"2026-07-05T01:52:16.855471+00:00"},{"alias_kind":"arxiv_version","alias_value":"2003.03379v1","created_at":"2026-07-05T01:52:16.855471+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2003.03379","created_at":"2026-07-05T01:52:16.855471+00:00"},{"alias_kind":"pith_short_12","alias_value":"PLO4WSFDVADH","created_at":"2026-07-05T01:52:16.855471+00:00"},{"alias_kind":"pith_short_16","alias_value":"PLO4WSFDVADHHFDX","created_at":"2026-07-05T01:52:16.855471+00:00"},{"alias_kind":"pith_short_8","alias_value":"PLO4WSFD","created_at":"2026-07-05T01:52:16.855471+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2510.25613","citing_title":"Muon Beam Dump Experiments explicate five-dimensional nature of $U(1)_{L_{\\mu}-L_{\\tau}}$","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15541","citing_title":"Probing inelastic sub-GeV dark matter at the DUNE near detector","ref_index":36,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PLO4WSFDVADHHFDXEUJGJDZVWN","json":"https://pith.science/pith/PLO4WSFDVADHHFDXEUJGJDZVWN.json","graph_json":"https://pith.science/api/pith-number/PLO4WSFDVADHHFDXEUJGJDZVWN/graph.json","events_json":"https://pith.science/api/pith-number/PLO4WSFDVADHHFDXEUJGJDZVWN/events.json","paper":"https://pith.science/paper/PLO4WSFD"},"agent_actions":{"view_html":"https://pith.science/pith/PLO4WSFDVADHHFDXEUJGJDZVWN","download_json":"https://pith.science/pith/PLO4WSFDVADHHFDXEUJGJDZVWN.json","view_paper":"https://pith.science/paper/PLO4WSFD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2003.03379&json=true","fetch_graph":"https://pith.science/api/pith-number/PLO4WSFDVADHHFDXEUJGJDZVWN/graph.json","fetch_events":"https://pith.science/api/pith-number/PLO4WSFDVADHHFDXEUJGJDZVWN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PLO4WSFDVADHHFDXEUJGJDZVWN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PLO4WSFDVADHHFDXEUJGJDZVWN/action/storage_attestation","attest_author":"https://pith.science/pith/PLO4WSFDVADHHFDXEUJGJDZVWN/action/author_attestation","sign_citation":"https://pith.science/pith/PLO4WSFDVADHHFDXEUJGJDZVWN/action/citation_signature","submit_replication":"https://pith.science/pith/PLO4WSFDVADHHFDXEUJGJDZVWN/action/replication_record"}},"created_at":"2026-07-05T01:52:16.855471+00:00","updated_at":"2026-07-05T01:52:16.855471+00:00"}