{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:64RG3WLFU2RB65JXAWPHWEHZRL","short_pith_number":"pith:64RG3WLF","schema_version":"1.0","canonical_sha256":"f7226dd965a6a21f7537059e7b10f98af977a87d8d98649404c5abf0ef229eaf","source":{"kind":"arxiv","id":"2408.03004","version":2},"attestation_state":"computed","paper":{"title":"Reconciling Cosmological Tensions with Inelastic Dark Matter and Dark Radiation in a $\\boldsymbol{U(1)_D}$ Framework","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Ki-Young Choi, Satyabrata Mahapatra, Wonsub Cho","submitted_at":"2024-08-06T07:30:07Z","abstract_excerpt":"We propose a novel and comprehensive particle physics framework that addresses multiple cosmological tensions observed in recent measurements of the Hubble parameter, $S_8$, and Lyman-$\\alpha$ forest data. Our model, termed `{\\bf SIDR$+\\boldsymbol{z_t}$}' (Self Interacting Dark Radiation with transition redshift), is based on an inelastic dark matter (IDM) scenario coupled with dark radiation, governed by a $U(1)_D$ gauge symmetry. This framework naturally incorporates cold dark matter (DM), strongly interacting dark radiation (SIDR), and the interactions between these components. The fluid-li"},"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":"2408.03004","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2024-08-06T07:30:07Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"c7787ba05c438626e9d7f7b57f05205778278c5daff413121bf4a7a13d3e1842","abstract_canon_sha256":"6d937b66ebff3792bb3617f40c02408831cd76d17505a10eeea9036eb0fef1e5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:17:47.056840Z","signature_b64":"lxXnwm9OJUITUG1ARllCs4SnCdh8OzZ9O5E1CWaxKGygZuSCxc3WtHKkw/RXOyX1m/rcNFBaxcd33iEeQJuMCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f7226dd965a6a21f7537059e7b10f98af977a87d8d98649404c5abf0ef229eaf","last_reissued_at":"2026-07-05T09:17:47.056345Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:17:47.056345Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Reconciling Cosmological Tensions with Inelastic Dark Matter and Dark Radiation in a $\\boldsymbol{U(1)_D}$ Framework","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Ki-Young Choi, Satyabrata Mahapatra, Wonsub Cho","submitted_at":"2024-08-06T07:30:07Z","abstract_excerpt":"We propose a novel and comprehensive particle physics framework that addresses multiple cosmological tensions observed in recent measurements of the Hubble parameter, $S_8$, and Lyman-$\\alpha$ forest data. Our model, termed `{\\bf SIDR$+\\boldsymbol{z_t}$}' (Self Interacting Dark Radiation with transition redshift), is based on an inelastic dark matter (IDM) scenario coupled with dark radiation, governed by a $U(1)_D$ gauge symmetry. This framework naturally incorporates cold dark matter (DM), strongly interacting dark radiation (SIDR), and the interactions between these components. The fluid-li"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2408.03004","kind":"arxiv","version":2},"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/2408.03004/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":"2408.03004","created_at":"2026-07-05T09:17:47.056409+00:00"},{"alias_kind":"arxiv_version","alias_value":"2408.03004v2","created_at":"2026-07-05T09:17:47.056409+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2408.03004","created_at":"2026-07-05T09:17:47.056409+00:00"},{"alias_kind":"pith_short_12","alias_value":"64RG3WLFU2RB","created_at":"2026-07-05T09:17:47.056409+00:00"},{"alias_kind":"pith_short_16","alias_value":"64RG3WLFU2RB65JX","created_at":"2026-07-05T09:17:47.056409+00:00"},{"alias_kind":"pith_short_8","alias_value":"64RG3WLF","created_at":"2026-07-05T09:17:47.056409+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.08097","citing_title":"Atomic Dark Matter, Interacting Dark Radiation, and the Hubble Tension","ref_index":42,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/64RG3WLFU2RB65JXAWPHWEHZRL","json":"https://pith.science/pith/64RG3WLFU2RB65JXAWPHWEHZRL.json","graph_json":"https://pith.science/api/pith-number/64RG3WLFU2RB65JXAWPHWEHZRL/graph.json","events_json":"https://pith.science/api/pith-number/64RG3WLFU2RB65JXAWPHWEHZRL/events.json","paper":"https://pith.science/paper/64RG3WLF"},"agent_actions":{"view_html":"https://pith.science/pith/64RG3WLFU2RB65JXAWPHWEHZRL","download_json":"https://pith.science/pith/64RG3WLFU2RB65JXAWPHWEHZRL.json","view_paper":"https://pith.science/paper/64RG3WLF","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2408.03004&json=true","fetch_graph":"https://pith.science/api/pith-number/64RG3WLFU2RB65JXAWPHWEHZRL/graph.json","fetch_events":"https://pith.science/api/pith-number/64RG3WLFU2RB65JXAWPHWEHZRL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/64RG3WLFU2RB65JXAWPHWEHZRL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/64RG3WLFU2RB65JXAWPHWEHZRL/action/storage_attestation","attest_author":"https://pith.science/pith/64RG3WLFU2RB65JXAWPHWEHZRL/action/author_attestation","sign_citation":"https://pith.science/pith/64RG3WLFU2RB65JXAWPHWEHZRL/action/citation_signature","submit_replication":"https://pith.science/pith/64RG3WLFU2RB65JXAWPHWEHZRL/action/replication_record"}},"created_at":"2026-07-05T09:17:47.056409+00:00","updated_at":"2026-07-05T09:17:47.056409+00:00"}