{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:VE4QM2WAONJ6JK3GVQPT7AKSFG","short_pith_number":"pith:VE4QM2WA","schema_version":"1.0","canonical_sha256":"a939066ac07353e4ab66ac1f3f8152298f418a68b216714099e66a69f259033e","source":{"kind":"arxiv","id":"1907.04340","version":2},"attestation_state":"computed","paper":{"title":"Gravity-mediated Scalar Dark Matter in Warped Extra-Dimensions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Andrea Donini, Miguel G. Folgado, Nuria Rius","submitted_at":"2019-07-09T18:00:40Z","abstract_excerpt":"We revisit the case of scalar dark matter interacting just gravitationally with the Standard Model (SM) particles in an extra-dimensional Randall-Sundrum scenario. We assume that both, the dark matter and the Standard Model, are localized in the TeV brane and only interact via gravitational mediators, namely the graviton Kaluza-Klein modes and the radion. We analyze in detail the dark matter annihilation channel into two on-shell KK-gravitons, and contrary to previous studies which overlooked this process, we find that it is possible to obtain the correct relic abundance for dark matter masses"},"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":"1907.04340","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2019-07-09T18:00:40Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"cd3a01cc464416b00c6634281e817acabf022b85aeb0aab1de1f3c957b2e6f05","abstract_canon_sha256":"6d7554371d95f9772484d562af21e5abd9bc50cb0825ecf4a2cda2f22bb645f6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:38:33.001312Z","signature_b64":"IcNeOvB6o9qxmXoG/BV3bIMmN/HfIAyy8Iv0sxPshJsQBjgoamEEkv42P/NrmOVRMPTqOCV3l0dNwfn9aKV5DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a939066ac07353e4ab66ac1f3f8152298f418a68b216714099e66a69f259033e","last_reissued_at":"2026-07-05T00:38:33.000888Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:38:33.000888Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravity-mediated Scalar Dark Matter in Warped Extra-Dimensions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Andrea Donini, Miguel G. Folgado, Nuria Rius","submitted_at":"2019-07-09T18:00:40Z","abstract_excerpt":"We revisit the case of scalar dark matter interacting just gravitationally with the Standard Model (SM) particles in an extra-dimensional Randall-Sundrum scenario. We assume that both, the dark matter and the Standard Model, are localized in the TeV brane and only interact via gravitational mediators, namely the graviton Kaluza-Klein modes and the radion. We analyze in detail the dark matter annihilation channel into two on-shell KK-gravitons, and contrary to previous studies which overlooked this process, we find that it is possible to obtain the correct relic abundance for dark matter masses"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1907.04340","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/1907.04340/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":"1907.04340","created_at":"2026-07-05T00:38:33.000950+00:00"},{"alias_kind":"arxiv_version","alias_value":"1907.04340v2","created_at":"2026-07-05T00:38:33.000950+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1907.04340","created_at":"2026-07-05T00:38:33.000950+00:00"},{"alias_kind":"pith_short_12","alias_value":"VE4QM2WAONJ6","created_at":"2026-07-05T00:38:33.000950+00:00"},{"alias_kind":"pith_short_16","alias_value":"VE4QM2WAONJ6JK3G","created_at":"2026-07-05T00:38:33.000950+00:00"},{"alias_kind":"pith_short_8","alias_value":"VE4QM2WA","created_at":"2026-07-05T00:38:33.000950+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.25014","citing_title":"Probing Confining Dark Sectors with Cosmological Perturbations","ref_index":18,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/VE4QM2WAONJ6JK3GVQPT7AKSFG","json":"https://pith.science/pith/VE4QM2WAONJ6JK3GVQPT7AKSFG.json","graph_json":"https://pith.science/api/pith-number/VE4QM2WAONJ6JK3GVQPT7AKSFG/graph.json","events_json":"https://pith.science/api/pith-number/VE4QM2WAONJ6JK3GVQPT7AKSFG/events.json","paper":"https://pith.science/paper/VE4QM2WA"},"agent_actions":{"view_html":"https://pith.science/pith/VE4QM2WAONJ6JK3GVQPT7AKSFG","download_json":"https://pith.science/pith/VE4QM2WAONJ6JK3GVQPT7AKSFG.json","view_paper":"https://pith.science/paper/VE4QM2WA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1907.04340&json=true","fetch_graph":"https://pith.science/api/pith-number/VE4QM2WAONJ6JK3GVQPT7AKSFG/graph.json","fetch_events":"https://pith.science/api/pith-number/VE4QM2WAONJ6JK3GVQPT7AKSFG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/VE4QM2WAONJ6JK3GVQPT7AKSFG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/VE4QM2WAONJ6JK3GVQPT7AKSFG/action/storage_attestation","attest_author":"https://pith.science/pith/VE4QM2WAONJ6JK3GVQPT7AKSFG/action/author_attestation","sign_citation":"https://pith.science/pith/VE4QM2WAONJ6JK3GVQPT7AKSFG/action/citation_signature","submit_replication":"https://pith.science/pith/VE4QM2WAONJ6JK3GVQPT7AKSFG/action/replication_record"}},"created_at":"2026-07-05T00:38:33.000950+00:00","updated_at":"2026-07-05T00:38:33.000950+00:00"}