{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:54CAMX47ERMVVKEW2GPC3P6XQQ","short_pith_number":"pith:54CAMX47","schema_version":"1.0","canonical_sha256":"ef04065f9f24595aa896d19e2dbfd7842e1e88961338e11028f9c441c964c66d","source":{"kind":"arxiv","id":"1709.09819","version":2},"attestation_state":"computed","paper":{"title":"Analysis of branon dark matter and extra-dimensional models with AMS-02","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Alvaro de la Cruz-Dombriz, Jose A. R. Cembranos, Miguel Mendez-Isla, Peter K. S. Dunsby","submitted_at":"2017-09-28T06:41:26Z","abstract_excerpt":"In the following work, we compute the positron production from branon dark matter annihilations in order to constrain extra-dimensional theories. By having assumed that the positron fraction measured by AMS-02 is well explained just with astrophysical sources, exclusion diagrams for the branon mass and the tension of the brane, the two parameters characterising the branon phenomenology become possible. Our analysis has been performed for a minimal and a medium diffusion model in one extra dimension for both pseudo-isothermal and Navarro Frenck White dark matter haloes. Our constraints in the d"},"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":"1709.09819","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2017-09-28T06:41:26Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"dcef62ce0da70abf0f035534c7cdcc73eaba4784d018a72162f0869837010ac6","abstract_canon_sha256":"24eb076a043f942919b2d740f2be214f49dfe4bd2a670c8576e20225fd876fc4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:54:16.877423Z","signature_b64":"pkCCNzHvZI8ViKpNvTRzSwALvJi0XvudVDKwp6XUcMeLqqvZMmSFdDFia08TDLMGJBTdnUs5c2V+aqpbZnOWCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ef04065f9f24595aa896d19e2dbfd7842e1e88961338e11028f9c441c964c66d","last_reissued_at":"2026-05-17T23:54:16.876842Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:54:16.876842Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Analysis of branon dark matter and extra-dimensional models with AMS-02","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Alvaro de la Cruz-Dombriz, Jose A. R. Cembranos, Miguel Mendez-Isla, Peter K. S. Dunsby","submitted_at":"2017-09-28T06:41:26Z","abstract_excerpt":"In the following work, we compute the positron production from branon dark matter annihilations in order to constrain extra-dimensional theories. By having assumed that the positron fraction measured by AMS-02 is well explained just with astrophysical sources, exclusion diagrams for the branon mass and the tension of the brane, the two parameters characterising the branon phenomenology become possible. Our analysis has been performed for a minimal and a medium diffusion model in one extra dimension for both pseudo-isothermal and Navarro Frenck White dark matter haloes. Our constraints in the d"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.09819","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":""},"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":"1709.09819","created_at":"2026-05-17T23:54:16.876953+00:00"},{"alias_kind":"arxiv_version","alias_value":"1709.09819v2","created_at":"2026-05-17T23:54:16.876953+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.09819","created_at":"2026-05-17T23:54:16.876953+00:00"},{"alias_kind":"pith_short_12","alias_value":"54CAMX47ERMV","created_at":"2026-05-18T12:31:00.734936+00:00"},{"alias_kind":"pith_short_16","alias_value":"54CAMX47ERMVVKEW","created_at":"2026-05-18T12:31:00.734936+00:00"},{"alias_kind":"pith_short_8","alias_value":"54CAMX47","created_at":"2026-05-18T12:31:00.734936+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.20117","citing_title":"The potential of diffuse Galactic Ridge neutrino measurements to constrain dark matter","ref_index":86,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/54CAMX47ERMVVKEW2GPC3P6XQQ","json":"https://pith.science/pith/54CAMX47ERMVVKEW2GPC3P6XQQ.json","graph_json":"https://pith.science/api/pith-number/54CAMX47ERMVVKEW2GPC3P6XQQ/graph.json","events_json":"https://pith.science/api/pith-number/54CAMX47ERMVVKEW2GPC3P6XQQ/events.json","paper":"https://pith.science/paper/54CAMX47"},"agent_actions":{"view_html":"https://pith.science/pith/54CAMX47ERMVVKEW2GPC3P6XQQ","download_json":"https://pith.science/pith/54CAMX47ERMVVKEW2GPC3P6XQQ.json","view_paper":"https://pith.science/paper/54CAMX47","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1709.09819&json=true","fetch_graph":"https://pith.science/api/pith-number/54CAMX47ERMVVKEW2GPC3P6XQQ/graph.json","fetch_events":"https://pith.science/api/pith-number/54CAMX47ERMVVKEW2GPC3P6XQQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/54CAMX47ERMVVKEW2GPC3P6XQQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/54CAMX47ERMVVKEW2GPC3P6XQQ/action/storage_attestation","attest_author":"https://pith.science/pith/54CAMX47ERMVVKEW2GPC3P6XQQ/action/author_attestation","sign_citation":"https://pith.science/pith/54CAMX47ERMVVKEW2GPC3P6XQQ/action/citation_signature","submit_replication":"https://pith.science/pith/54CAMX47ERMVVKEW2GPC3P6XQQ/action/replication_record"}},"created_at":"2026-05-17T23:54:16.876953+00:00","updated_at":"2026-05-17T23:54:16.876953+00:00"}