{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:RINF43DBIGF72SV3HLN6XCXAXH","short_pith_number":"pith:RINF43DB","schema_version":"1.0","canonical_sha256":"8a1a5e6c61418bfd4abb3adbeb8ae0b9dc8fdf7d40f10c743f318107a222428f","source":{"kind":"arxiv","id":"2201.11497","version":1},"attestation_state":"computed","paper":{"title":"Revisiting the Fermionic Dark Matter Absorption on Electron Target","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Jie Sheng, Shao-Feng Ge, Xiao-Dong Ma, Xiao-Gang He","submitted_at":"2022-01-27T13:19:51Z","abstract_excerpt":"We perform a systematic study of the fermionic DM absorption interactions on electron target in the context of effective field theory. The fermionic DM absorption is not just sensitive to sub-MeV DM with efficient energy release, but also gives a unique signature with clear peak in the electron recoil spectrum whose shape is largely determined by the atomic effects. Fitting with the Xenon1T and PandaX-II data prefers DM mass at $m_\\chi = 59$keV and 105keV, respectively, while the cut-off scale is probed up to around 1TeV. The DM overproduction in the early Universe, the invisible decay effect "},"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":"2201.11497","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","primary_cat":"hep-ph","submitted_at":"2022-01-27T13:19:51Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"c3dc8c74e732b76ab0e395a9c7d9a06aa169ca0a0d39f71187e2d7583468baa5","abstract_canon_sha256":"812ced914d256c553b76851adbe5b46f1b1c25d270dc9c2718a344eb92a87f84"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:31:31.952801Z","signature_b64":"Vyogkwa9zIpAZc3oU9lNgtz3KMFoapbTOUqi5ZM3BOSI0BbYAM9O+5yBe1WBf9Plbw3w9t499nsSKODbc64vDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8a1a5e6c61418bfd4abb3adbeb8ae0b9dc8fdf7d40f10c743f318107a222428f","last_reissued_at":"2026-07-05T04:31:31.952307Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:31:31.952307Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Revisiting the Fermionic Dark Matter Absorption on Electron Target","license":"http://creativecommons.org/licenses/by-nc-nd/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Jie Sheng, Shao-Feng Ge, Xiao-Dong Ma, Xiao-Gang He","submitted_at":"2022-01-27T13:19:51Z","abstract_excerpt":"We perform a systematic study of the fermionic DM absorption interactions on electron target in the context of effective field theory. The fermionic DM absorption is not just sensitive to sub-MeV DM with efficient energy release, but also gives a unique signature with clear peak in the electron recoil spectrum whose shape is largely determined by the atomic effects. Fitting with the Xenon1T and PandaX-II data prefers DM mass at $m_\\chi = 59$keV and 105keV, respectively, while the cut-off scale is probed up to around 1TeV. The DM overproduction in the early Universe, the invisible decay effect "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2201.11497","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/2201.11497/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":"2201.11497","created_at":"2026-07-05T04:31:31.952373+00:00"},{"alias_kind":"arxiv_version","alias_value":"2201.11497v1","created_at":"2026-07-05T04:31:31.952373+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2201.11497","created_at":"2026-07-05T04:31:31.952373+00:00"},{"alias_kind":"pith_short_12","alias_value":"RINF43DBIGF7","created_at":"2026-07-05T04:31:31.952373+00:00"},{"alias_kind":"pith_short_16","alias_value":"RINF43DBIGF72SV3","created_at":"2026-07-05T04:31:31.952373+00:00"},{"alias_kind":"pith_short_8","alias_value":"RINF43DB","created_at":"2026-07-05T04:31:31.952373+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2602.07384","citing_title":"Constraints on Fermionic Dark Matter Absorption from Radiochemical Solar-Neutrino Measurements","ref_index":8,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/RINF43DBIGF72SV3HLN6XCXAXH","json":"https://pith.science/pith/RINF43DBIGF72SV3HLN6XCXAXH.json","graph_json":"https://pith.science/api/pith-number/RINF43DBIGF72SV3HLN6XCXAXH/graph.json","events_json":"https://pith.science/api/pith-number/RINF43DBIGF72SV3HLN6XCXAXH/events.json","paper":"https://pith.science/paper/RINF43DB"},"agent_actions":{"view_html":"https://pith.science/pith/RINF43DBIGF72SV3HLN6XCXAXH","download_json":"https://pith.science/pith/RINF43DBIGF72SV3HLN6XCXAXH.json","view_paper":"https://pith.science/paper/RINF43DB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2201.11497&json=true","fetch_graph":"https://pith.science/api/pith-number/RINF43DBIGF72SV3HLN6XCXAXH/graph.json","fetch_events":"https://pith.science/api/pith-number/RINF43DBIGF72SV3HLN6XCXAXH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/RINF43DBIGF72SV3HLN6XCXAXH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/RINF43DBIGF72SV3HLN6XCXAXH/action/storage_attestation","attest_author":"https://pith.science/pith/RINF43DBIGF72SV3HLN6XCXAXH/action/author_attestation","sign_citation":"https://pith.science/pith/RINF43DBIGF72SV3HLN6XCXAXH/action/citation_signature","submit_replication":"https://pith.science/pith/RINF43DBIGF72SV3HLN6XCXAXH/action/replication_record"}},"created_at":"2026-07-05T04:31:31.952373+00:00","updated_at":"2026-07-05T04:31:31.952373+00:00"}