{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:HT4GCFEWGHQDQRYMZHQRUTM2TZ","short_pith_number":"pith:HT4GCFEW","schema_version":"1.0","canonical_sha256":"3cf861149631e038470cc9e11a4d9a9e6bb742d5a3b4870a78a36ad6c67c0566","source":{"kind":"arxiv","id":"1906.02199","version":1},"attestation_state":"computed","paper":{"title":"The Warped Dark Sector","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-ph","authors_text":"Philippe Brax, Philip Tanedo, Sylvain Fichet","submitted_at":"2019-06-05T18:00:00Z","abstract_excerpt":"Five-dimensional braneworld constructions in anti-de Sitter space naturally lead to dark sector scenarios in which parts of the dark sector vanish at high 4d momentum or temperature. In the language of modified gravity, such feature implies a new mechanism for hiding light scalars, as well as the possibility of UV-completing chameleon-like effective theories. In the language of dark matter phenomenology, the high-energy behaviour of the mediator sector changes dark matter observational complementarity. A multitude of signatures---including exotic ones---are present from laboratory to cosmologi"},"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":"1906.02199","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2019-06-05T18:00:00Z","cross_cats_sorted":["astro-ph.CO","gr-qc"],"title_canon_sha256":"b394eb2cead813d420bc059d4ce41c9c8322f2e0c5b5c583795a6afda26e28a7","abstract_canon_sha256":"a85d4d7d2defa8c5dd54a25a93d77eacce79275882b1033e16a1ee55296f8426"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:13:02.444241Z","signature_b64":"H2i8OVfiO99OPVKTQDF8noZFc9wgWG0NCtKg6lUqZgeGQ0fWxAa6qawrClC7KRKuRwnvEit4TX7gKwxz7K40Dw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3cf861149631e038470cc9e11a4d9a9e6bb742d5a3b4870a78a36ad6c67c0566","last_reissued_at":"2026-07-05T00:13:02.443740Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:13:02.443740Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Warped Dark Sector","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-ph","authors_text":"Philippe Brax, Philip Tanedo, Sylvain Fichet","submitted_at":"2019-06-05T18:00:00Z","abstract_excerpt":"Five-dimensional braneworld constructions in anti-de Sitter space naturally lead to dark sector scenarios in which parts of the dark sector vanish at high 4d momentum or temperature. In the language of modified gravity, such feature implies a new mechanism for hiding light scalars, as well as the possibility of UV-completing chameleon-like effective theories. In the language of dark matter phenomenology, the high-energy behaviour of the mediator sector changes dark matter observational complementarity. A multitude of signatures---including exotic ones---are present from laboratory to cosmologi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1906.02199","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/1906.02199/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":"1906.02199","created_at":"2026-07-05T00:13:02.443803+00:00"},{"alias_kind":"arxiv_version","alias_value":"1906.02199v1","created_at":"2026-07-05T00:13:02.443803+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1906.02199","created_at":"2026-07-05T00:13:02.443803+00:00"},{"alias_kind":"pith_short_12","alias_value":"HT4GCFEWGHQD","created_at":"2026-07-05T00:13:02.443803+00:00"},{"alias_kind":"pith_short_16","alias_value":"HT4GCFEWGHQDQRYM","created_at":"2026-07-05T00:13:02.443803+00:00"},{"alias_kind":"pith_short_8","alias_value":"HT4GCFEW","created_at":"2026-07-05T00:13:02.443803+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.25014","citing_title":"Probing Confining Dark Sectors with Cosmological Perturbations","ref_index":28,"is_internal_anchor":false},{"citing_arxiv_id":"2606.30760","citing_title":"Rich Phenomenology from Simple Ingredients: A Review of Confining Dark Sectors","ref_index":152,"is_internal_anchor":false},{"citing_arxiv_id":"2407.20615","citing_title":"Prospects of five-dimensional $L_\\mu-L_\\tau$ gauge interactions in the light of elastic neutrino-electron scatterings: The scope of the DUNE near detector","ref_index":114,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HT4GCFEWGHQDQRYMZHQRUTM2TZ","json":"https://pith.science/pith/HT4GCFEWGHQDQRYMZHQRUTM2TZ.json","graph_json":"https://pith.science/api/pith-number/HT4GCFEWGHQDQRYMZHQRUTM2TZ/graph.json","events_json":"https://pith.science/api/pith-number/HT4GCFEWGHQDQRYMZHQRUTM2TZ/events.json","paper":"https://pith.science/paper/HT4GCFEW"},"agent_actions":{"view_html":"https://pith.science/pith/HT4GCFEWGHQDQRYMZHQRUTM2TZ","download_json":"https://pith.science/pith/HT4GCFEWGHQDQRYMZHQRUTM2TZ.json","view_paper":"https://pith.science/paper/HT4GCFEW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1906.02199&json=true","fetch_graph":"https://pith.science/api/pith-number/HT4GCFEWGHQDQRYMZHQRUTM2TZ/graph.json","fetch_events":"https://pith.science/api/pith-number/HT4GCFEWGHQDQRYMZHQRUTM2TZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HT4GCFEWGHQDQRYMZHQRUTM2TZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HT4GCFEWGHQDQRYMZHQRUTM2TZ/action/storage_attestation","attest_author":"https://pith.science/pith/HT4GCFEWGHQDQRYMZHQRUTM2TZ/action/author_attestation","sign_citation":"https://pith.science/pith/HT4GCFEWGHQDQRYMZHQRUTM2TZ/action/citation_signature","submit_replication":"https://pith.science/pith/HT4GCFEWGHQDQRYMZHQRUTM2TZ/action/replication_record"}},"created_at":"2026-07-05T00:13:02.443803+00:00","updated_at":"2026-07-05T00:13:02.443803+00:00"}