{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:32BFFQVNOMFP2DE4XATD2EOFUB","short_pith_number":"pith:32BFFQVN","schema_version":"1.0","canonical_sha256":"de8252c2ad730afd0c9cb8263d11c5a07459510da90c2df6272b5cb037d9cc41","source":{"kind":"arxiv","id":"1810.04709","version":2},"attestation_state":"computed","paper":{"title":"Velocity Dependence from Resonant Self-Interacting Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Camilo Garcia-Cely, Hitoshi Murayama, Xiaoyong Chu","submitted_at":"2018-10-10T18:59:48Z","abstract_excerpt":"The dark matter density distribution in small-scale astrophysical objects may indicate that dark matter is self-interacting, while observations from clusters of galaxies suggest that the corresponding cross section depends on the velocity. Using a model-independent approach, we show that resonant self-interacting dark matter (RSIDM) can naturally explain such a behavior. In contrast to what is often assumed, this does not require a light mediator. We present explicit realizations of this mechanism and discuss the corresponding astrophysical constraints."},"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":"1810.04709","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2018-10-10T18:59:48Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"141c81de0841d581ee2d18b83d489018e5742fdc3b2802413d1899ec42544f06","abstract_canon_sha256":"0fe65b4fed0f7c5e931b288eecb53b8854d72904b79fcff533c06efb131dc81f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:52:40.554389Z","signature_b64":"wWURuyuHXLqMy1P/6kHzIjPrMyaeOiVXzrngpkdJGM8Vs5gkNOKg3ifh7NqhXMoHfU2X8r8Wqa4/R11vVIRhAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"de8252c2ad730afd0c9cb8263d11c5a07459510da90c2df6272b5cb037d9cc41","last_reissued_at":"2026-05-17T23:52:40.553756Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:52:40.553756Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Velocity Dependence from Resonant Self-Interacting Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Camilo Garcia-Cely, Hitoshi Murayama, Xiaoyong Chu","submitted_at":"2018-10-10T18:59:48Z","abstract_excerpt":"The dark matter density distribution in small-scale astrophysical objects may indicate that dark matter is self-interacting, while observations from clusters of galaxies suggest that the corresponding cross section depends on the velocity. Using a model-independent approach, we show that resonant self-interacting dark matter (RSIDM) can naturally explain such a behavior. In contrast to what is often assumed, this does not require a light mediator. We present explicit realizations of this mechanism and discuss the corresponding astrophysical constraints."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1810.04709","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":"1810.04709","created_at":"2026-05-17T23:52:40.553853+00:00"},{"alias_kind":"arxiv_version","alias_value":"1810.04709v2","created_at":"2026-05-17T23:52:40.553853+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1810.04709","created_at":"2026-05-17T23:52:40.553853+00:00"},{"alias_kind":"pith_short_12","alias_value":"32BFFQVNOMFP","created_at":"2026-05-18T12:32:02.567920+00:00"},{"alias_kind":"pith_short_16","alias_value":"32BFFQVNOMFP2DE4","created_at":"2026-05-18T12:32:02.567920+00:00"},{"alias_kind":"pith_short_8","alias_value":"32BFFQVN","created_at":"2026-05-18T12:32:02.567920+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.22685","citing_title":"Dwarf Galaxy Constraints on Interacting Fermionic Dark Matter","ref_index":64,"is_internal_anchor":true},{"citing_arxiv_id":"2511.09306","citing_title":"Self-Interaction of Super-Resonant Dark Matter","ref_index":29,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/32BFFQVNOMFP2DE4XATD2EOFUB","json":"https://pith.science/pith/32BFFQVNOMFP2DE4XATD2EOFUB.json","graph_json":"https://pith.science/api/pith-number/32BFFQVNOMFP2DE4XATD2EOFUB/graph.json","events_json":"https://pith.science/api/pith-number/32BFFQVNOMFP2DE4XATD2EOFUB/events.json","paper":"https://pith.science/paper/32BFFQVN"},"agent_actions":{"view_html":"https://pith.science/pith/32BFFQVNOMFP2DE4XATD2EOFUB","download_json":"https://pith.science/pith/32BFFQVNOMFP2DE4XATD2EOFUB.json","view_paper":"https://pith.science/paper/32BFFQVN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1810.04709&json=true","fetch_graph":"https://pith.science/api/pith-number/32BFFQVNOMFP2DE4XATD2EOFUB/graph.json","fetch_events":"https://pith.science/api/pith-number/32BFFQVNOMFP2DE4XATD2EOFUB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/32BFFQVNOMFP2DE4XATD2EOFUB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/32BFFQVNOMFP2DE4XATD2EOFUB/action/storage_attestation","attest_author":"https://pith.science/pith/32BFFQVNOMFP2DE4XATD2EOFUB/action/author_attestation","sign_citation":"https://pith.science/pith/32BFFQVNOMFP2DE4XATD2EOFUB/action/citation_signature","submit_replication":"https://pith.science/pith/32BFFQVNOMFP2DE4XATD2EOFUB/action/replication_record"}},"created_at":"2026-05-17T23:52:40.553853+00:00","updated_at":"2026-05-17T23:52:40.553853+00:00"}