{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:PDF65H5HI35PQ7AABNECP35HHN","short_pith_number":"pith:PDF65H5H","schema_version":"1.0","canonical_sha256":"78cbee9fa746faf87c000b4827efa73b4b18ed969968f9efdee03998648b015e","source":{"kind":"arxiv","id":"1806.01291","version":2},"attestation_state":"computed","paper":{"title":"A complete Lorentz-to-Galileo dictionary for direct Dark Matter detection","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Eugenio Del Nobile","submitted_at":"2018-06-04T18:00:08Z","abstract_excerpt":"We determine the most general non-relativistic theory of DM-nucleon scattering complying with the sole requirement of Lorentz invariance, for spin-0 and spin-1/2 DM. To do so, we first classify a comprehensive list of amplitude terms encompassing the most general Lorentz-covariant 2-to-2 DM-nucleon scattering amplitude. We then match each term to a Galilean-invariant operator at leading-order in the non-relativistic expansion, for both elastic and inelastic (endothermic and exothermic) scattering. Our complete Lorentz-to-Galileo mapping can be used to promptly determine the non-relativistic DM"},"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":"1806.01291","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2018-06-04T18:00:08Z","cross_cats_sorted":[],"title_canon_sha256":"b41e03e4aaba43eb83f4b53e7fcecd83f026c338505b5a3c83e596fb197ab5d6","abstract_canon_sha256":"19ac48250054b21cad00548712d9f1211f0dd4e4c77997f01ea194c8074d7054"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:58:04.744656Z","signature_b64":"clZNJhutoYJfasasQGL0RF+PxjAsfybSYb9tCnSiFePJcR8vsaUnHBmPe7F1OJRH6duyy6IG3/9mO3vsGHNxBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"78cbee9fa746faf87c000b4827efa73b4b18ed969968f9efdee03998648b015e","last_reissued_at":"2026-05-17T23:58:04.744261Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:58:04.744261Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A complete Lorentz-to-Galileo dictionary for direct Dark Matter detection","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Eugenio Del Nobile","submitted_at":"2018-06-04T18:00:08Z","abstract_excerpt":"We determine the most general non-relativistic theory of DM-nucleon scattering complying with the sole requirement of Lorentz invariance, for spin-0 and spin-1/2 DM. To do so, we first classify a comprehensive list of amplitude terms encompassing the most general Lorentz-covariant 2-to-2 DM-nucleon scattering amplitude. We then match each term to a Galilean-invariant operator at leading-order in the non-relativistic expansion, for both elastic and inelastic (endothermic and exothermic) scattering. Our complete Lorentz-to-Galileo mapping can be used to promptly determine the non-relativistic DM"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.01291","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":"1806.01291","created_at":"2026-05-17T23:58:04.744324+00:00"},{"alias_kind":"arxiv_version","alias_value":"1806.01291v2","created_at":"2026-05-17T23:58:04.744324+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1806.01291","created_at":"2026-05-17T23:58:04.744324+00:00"},{"alias_kind":"pith_short_12","alias_value":"PDF65H5HI35P","created_at":"2026-05-18T12:32:43.782077+00:00"},{"alias_kind":"pith_short_16","alias_value":"PDF65H5HI35PQ7AA","created_at":"2026-05-18T12:32:43.782077+00:00"},{"alias_kind":"pith_short_8","alias_value":"PDF65H5H","created_at":"2026-05-18T12:32:43.782077+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.05312","citing_title":"Monochromatic neutrinos from scotogenic dark matter","ref_index":34,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PDF65H5HI35PQ7AABNECP35HHN","json":"https://pith.science/pith/PDF65H5HI35PQ7AABNECP35HHN.json","graph_json":"https://pith.science/api/pith-number/PDF65H5HI35PQ7AABNECP35HHN/graph.json","events_json":"https://pith.science/api/pith-number/PDF65H5HI35PQ7AABNECP35HHN/events.json","paper":"https://pith.science/paper/PDF65H5H"},"agent_actions":{"view_html":"https://pith.science/pith/PDF65H5HI35PQ7AABNECP35HHN","download_json":"https://pith.science/pith/PDF65H5HI35PQ7AABNECP35HHN.json","view_paper":"https://pith.science/paper/PDF65H5H","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1806.01291&json=true","fetch_graph":"https://pith.science/api/pith-number/PDF65H5HI35PQ7AABNECP35HHN/graph.json","fetch_events":"https://pith.science/api/pith-number/PDF65H5HI35PQ7AABNECP35HHN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PDF65H5HI35PQ7AABNECP35HHN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PDF65H5HI35PQ7AABNECP35HHN/action/storage_attestation","attest_author":"https://pith.science/pith/PDF65H5HI35PQ7AABNECP35HHN/action/author_attestation","sign_citation":"https://pith.science/pith/PDF65H5HI35PQ7AABNECP35HHN/action/citation_signature","submit_replication":"https://pith.science/pith/PDF65H5HI35PQ7AABNECP35HHN/action/replication_record"}},"created_at":"2026-05-17T23:58:04.744324+00:00","updated_at":"2026-05-17T23:58:04.744324+00:00"}