{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:LOQS7ZCSVA56MLB4XJTVCN23WX","short_pith_number":"pith:LOQS7ZCS","schema_version":"1.0","canonical_sha256":"5ba12fe452a83be62c3cba6751375bb5e8e8a186a31c5ce0fdb0a3b75b0f5617","source":{"kind":"arxiv","id":"2308.01960","version":1},"attestation_state":"computed","paper":{"title":"Resonant Pseudo-Dirac Dark Matter as a Sub-GeV Thermal Target","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Katelin Schutz, Nirmalya Brahma, Saniya Heeba","submitted_at":"2023-08-03T18:00:02Z","abstract_excerpt":"Dark matter (DM) could be a pseudo-Dirac thermal relic with a small mass splitting that is coupled off-diagonally to a kinetically mixed dark photon. This model, particularly in the sub-GeV mass range, is a key benchmark for accelerator searches and direct detection experiments. Typically, the presence of even a tiny fraction of pseudo-Dirac DM in the excited state around the time of recombination would be excluded by DM annihilation bounds from the cosmic microwave background (CMB); thus, viable thermal histories must typically feature an exponential suppression of the excited state. We revis"},"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":"2308.01960","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2023-08-03T18:00:02Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"1a15c8d4a8c95b8a55c6ef4f09a13e3a8aaaa63960fe714bbfb69009518b2264","abstract_canon_sha256":"6ba0c574c2efade9b61c27928d93e96e6fa4648941761fc7b29457abb72f59bd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:37:35.677422Z","signature_b64":"waIIyvIs3Hg+FGwsEQESOkJPZTE7vY8AJkr5EvvKZnKBupdgbufFthRpAMQeFrQv6Wi+9vOtRDbd8tan2MNtCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5ba12fe452a83be62c3cba6751375bb5e8e8a186a31c5ce0fdb0a3b75b0f5617","last_reissued_at":"2026-07-05T06:37:35.676927Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:37:35.676927Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Resonant Pseudo-Dirac Dark Matter as a Sub-GeV Thermal Target","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Katelin Schutz, Nirmalya Brahma, Saniya Heeba","submitted_at":"2023-08-03T18:00:02Z","abstract_excerpt":"Dark matter (DM) could be a pseudo-Dirac thermal relic with a small mass splitting that is coupled off-diagonally to a kinetically mixed dark photon. This model, particularly in the sub-GeV mass range, is a key benchmark for accelerator searches and direct detection experiments. Typically, the presence of even a tiny fraction of pseudo-Dirac DM in the excited state around the time of recombination would be excluded by DM annihilation bounds from the cosmic microwave background (CMB); thus, viable thermal histories must typically feature an exponential suppression of the excited state. We revis"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2308.01960","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/2308.01960/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":"2308.01960","created_at":"2026-07-05T06:37:35.677016+00:00"},{"alias_kind":"arxiv_version","alias_value":"2308.01960v1","created_at":"2026-07-05T06:37:35.677016+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2308.01960","created_at":"2026-07-05T06:37:35.677016+00:00"},{"alias_kind":"pith_short_12","alias_value":"LOQS7ZCSVA56","created_at":"2026-07-05T06:37:35.677016+00:00"},{"alias_kind":"pith_short_16","alias_value":"LOQS7ZCSVA56MLB4","created_at":"2026-07-05T06:37:35.677016+00:00"},{"alias_kind":"pith_short_8","alias_value":"LOQS7ZCS","created_at":"2026-07-05T06:37:35.677016+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2512.05694","citing_title":"Nearly Degenerate Majorana Dark Matter and Its Self-Interactions in a Gauged $U(1)_{L_\\mu - L_\\tau}$ Model","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06929","citing_title":"Direct-detection constraints on inelastic dark matter with a scalar mediator","ref_index":78,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LOQS7ZCSVA56MLB4XJTVCN23WX","json":"https://pith.science/pith/LOQS7ZCSVA56MLB4XJTVCN23WX.json","graph_json":"https://pith.science/api/pith-number/LOQS7ZCSVA56MLB4XJTVCN23WX/graph.json","events_json":"https://pith.science/api/pith-number/LOQS7ZCSVA56MLB4XJTVCN23WX/events.json","paper":"https://pith.science/paper/LOQS7ZCS"},"agent_actions":{"view_html":"https://pith.science/pith/LOQS7ZCSVA56MLB4XJTVCN23WX","download_json":"https://pith.science/pith/LOQS7ZCSVA56MLB4XJTVCN23WX.json","view_paper":"https://pith.science/paper/LOQS7ZCS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2308.01960&json=true","fetch_graph":"https://pith.science/api/pith-number/LOQS7ZCSVA56MLB4XJTVCN23WX/graph.json","fetch_events":"https://pith.science/api/pith-number/LOQS7ZCSVA56MLB4XJTVCN23WX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LOQS7ZCSVA56MLB4XJTVCN23WX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LOQS7ZCSVA56MLB4XJTVCN23WX/action/storage_attestation","attest_author":"https://pith.science/pith/LOQS7ZCSVA56MLB4XJTVCN23WX/action/author_attestation","sign_citation":"https://pith.science/pith/LOQS7ZCSVA56MLB4XJTVCN23WX/action/citation_signature","submit_replication":"https://pith.science/pith/LOQS7ZCSVA56MLB4XJTVCN23WX/action/replication_record"}},"created_at":"2026-07-05T06:37:35.677016+00:00","updated_at":"2026-07-05T06:37:35.677016+00:00"}