{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:ZEWW2M32CGGJPDPYUZFH32QF3H","short_pith_number":"pith:ZEWW2M32","schema_version":"1.0","canonical_sha256":"c92d6d337a118c978df8a64a7dea05d9d171077b1a9d1b3523683af653630c15","source":{"kind":"arxiv","id":"2404.10066","version":1},"attestation_state":"computed","paper":{"title":"Solar reflection of dark matter with dark-photon mediators","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Hailin Xu, Rouven Essig, Timon Emken","submitted_at":"2024-04-15T18:14:54Z","abstract_excerpt":"We consider the scattering of low-mass halo dark-matter particles in the hot plasma of the Sun, focusing on dark matter that interact with ordinary matter through a dark-photon mediator. The resulting ``solar-reflected'' dark matter (SRDM) component contains high-velocity particles, which significantly extend the sensitivity of terrestrial direct-detection experiments to sub-MeV dark-matter masses. We use a detailed Monte-Carlo simulation to model the propagation and scattering of dark-matter particles in the Sun, including thermal effects, with special emphasis on ultralight dark-photon media"},"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":"2404.10066","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2024-04-15T18:14:54Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"54533ef9dc07e21d31d4f7c880ec95d0f0deea0c0088fa89a9db6b7843cc0620","abstract_canon_sha256":"d6a16656dbc5c97cccc55b1b7f88499cd553b0bc9a9d89c2a954dd248a78d9e4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:08:24.778181Z","signature_b64":"7eVV+DXFVvgdPXvM4iYE0eTBNJOu9vLtoDgOjVH46YU11orfyFHXA3cfAw9ZZ3sTgJyX8fM2TmQXbjEt2X02Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c92d6d337a118c978df8a64a7dea05d9d171077b1a9d1b3523683af653630c15","last_reissued_at":"2026-07-05T08:08:24.777754Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:08:24.777754Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Solar reflection of dark matter with dark-photon mediators","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"hep-ph","authors_text":"Hailin Xu, Rouven Essig, Timon Emken","submitted_at":"2024-04-15T18:14:54Z","abstract_excerpt":"We consider the scattering of low-mass halo dark-matter particles in the hot plasma of the Sun, focusing on dark matter that interact with ordinary matter through a dark-photon mediator. The resulting ``solar-reflected'' dark matter (SRDM) component contains high-velocity particles, which significantly extend the sensitivity of terrestrial direct-detection experiments to sub-MeV dark-matter masses. We use a detailed Monte-Carlo simulation to model the propagation and scattering of dark-matter particles in the Sun, including thermal effects, with special emphasis on ultralight dark-photon media"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2404.10066","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/2404.10066/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":"2404.10066","created_at":"2026-07-05T08:08:24.777809+00:00"},{"alias_kind":"arxiv_version","alias_value":"2404.10066v1","created_at":"2026-07-05T08:08:24.777809+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2404.10066","created_at":"2026-07-05T08:08:24.777809+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZEWW2M32CGGJ","created_at":"2026-07-05T08:08:24.777809+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZEWW2M32CGGJPDPY","created_at":"2026-07-05T08:08:24.777809+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZEWW2M32","created_at":"2026-07-05T08:08:24.777809+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.30724","citing_title":"Boosted Dark Matter from Sagittarius A$^\\star$","ref_index":20,"is_internal_anchor":false},{"citing_arxiv_id":"2602.04858","citing_title":"Primordial black holes as cosmic accelerators of light dark matter: Novel direct detection constraints","ref_index":105,"is_internal_anchor":false},{"citing_arxiv_id":"2604.21996","citing_title":"Solar Reflection of Inelastic Dark Matter","ref_index":4,"is_internal_anchor":false},{"citing_arxiv_id":"2604.19959","citing_title":"Sub-GeV dark matter from cosmic ray bremsstrahlung in the atmosphere","ref_index":15,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZEWW2M32CGGJPDPYUZFH32QF3H","json":"https://pith.science/pith/ZEWW2M32CGGJPDPYUZFH32QF3H.json","graph_json":"https://pith.science/api/pith-number/ZEWW2M32CGGJPDPYUZFH32QF3H/graph.json","events_json":"https://pith.science/api/pith-number/ZEWW2M32CGGJPDPYUZFH32QF3H/events.json","paper":"https://pith.science/paper/ZEWW2M32"},"agent_actions":{"view_html":"https://pith.science/pith/ZEWW2M32CGGJPDPYUZFH32QF3H","download_json":"https://pith.science/pith/ZEWW2M32CGGJPDPYUZFH32QF3H.json","view_paper":"https://pith.science/paper/ZEWW2M32","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2404.10066&json=true","fetch_graph":"https://pith.science/api/pith-number/ZEWW2M32CGGJPDPYUZFH32QF3H/graph.json","fetch_events":"https://pith.science/api/pith-number/ZEWW2M32CGGJPDPYUZFH32QF3H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZEWW2M32CGGJPDPYUZFH32QF3H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZEWW2M32CGGJPDPYUZFH32QF3H/action/storage_attestation","attest_author":"https://pith.science/pith/ZEWW2M32CGGJPDPYUZFH32QF3H/action/author_attestation","sign_citation":"https://pith.science/pith/ZEWW2M32CGGJPDPYUZFH32QF3H/action/citation_signature","submit_replication":"https://pith.science/pith/ZEWW2M32CGGJPDPYUZFH32QF3H/action/replication_record"}},"created_at":"2026-07-05T08:08:24.777809+00:00","updated_at":"2026-07-05T08:08:24.777809+00:00"}