{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:XYX6BBXSZPFC3SHBNZZM5IKZGM","short_pith_number":"pith:XYX6BBXS","schema_version":"1.0","canonical_sha256":"be2fe086f2cbca2dc8e16e72cea1593305259499d0e4307456583d87e558abc1","source":{"kind":"arxiv","id":"1611.02716","version":1},"attestation_state":"computed","paper":{"title":"How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.GA","authors_text":"Andrew B. Pace, Ayuki Kamada, Hai-Bo Yu, Manoj Kaplinghat","submitted_at":"2016-11-08T21:01:50Z","abstract_excerpt":"The rotation curves of spiral galaxies exhibit a diversity that has been difficult to understand in the cold dark matter (CDM) paradigm. We show that the self-interacting dark matter (SIDM) model provides excellent fits to the rotation curves of a sample of galaxies with asymptotic velocities in the 25 to 300 km/s range that exemplify the full range of diversity. We only assume the halo concentration-mass relation predicted by the CDM model and a fixed value of the self-interaction cross section.In dark matter dominated galaxies, thermalization due to self-interactions creates large cores and "},"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":"1611.02716","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2016-11-08T21:01:50Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"1e303e894a7c047146f6580489f61fbe7d74f0e10ae019e0755acddb42fdc58a","abstract_canon_sha256":"cf3162dd6f3b8a170a46b76ac96466fd85a68e194e9a47abe1080f3cdbb0982b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:34:52.431773Z","signature_b64":"XKs0IG27Di32zcBI4DcUcpDxEtImqT3tJK7pMxTzwF2A9YxjdSjIXokdTzXa2JshyBAlYeiIrSxiBmlqo4rCDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"be2fe086f2cbca2dc8e16e72cea1593305259499d0e4307456583d87e558abc1","last_reissued_at":"2026-05-18T00:34:52.431038Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:34:52.431038Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.GA","authors_text":"Andrew B. Pace, Ayuki Kamada, Hai-Bo Yu, Manoj Kaplinghat","submitted_at":"2016-11-08T21:01:50Z","abstract_excerpt":"The rotation curves of spiral galaxies exhibit a diversity that has been difficult to understand in the cold dark matter (CDM) paradigm. We show that the self-interacting dark matter (SIDM) model provides excellent fits to the rotation curves of a sample of galaxies with asymptotic velocities in the 25 to 300 km/s range that exemplify the full range of diversity. We only assume the halo concentration-mass relation predicted by the CDM model and a fixed value of the self-interaction cross section.In dark matter dominated galaxies, thermalization due to self-interactions creates large cores and "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1611.02716","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":""},"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":"1611.02716","created_at":"2026-05-18T00:34:52.431168+00:00"},{"alias_kind":"arxiv_version","alias_value":"1611.02716v1","created_at":"2026-05-18T00:34:52.431168+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1611.02716","created_at":"2026-05-18T00:34:52.431168+00:00"},{"alias_kind":"pith_short_12","alias_value":"XYX6BBXSZPFC","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_16","alias_value":"XYX6BBXSZPFC3SHB","created_at":"2026-05-18T12:30:51.357362+00:00"},{"alias_kind":"pith_short_8","alias_value":"XYX6BBXS","created_at":"2026-05-18T12:30:51.357362+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2512.18959","citing_title":"Scalar-Mediated Inelastic Dark Matter as a Solution to Small-Scale Structure Anomalies","ref_index":28,"is_internal_anchor":true},{"citing_arxiv_id":"2604.19726","citing_title":"Breaking the UV Luminosity Function Degeneracy:Self-Interacting Dark Matter Constraints from Reionization Topology","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2604.10726","citing_title":"Reionization Topology as a Probe of Self-Interacting Dark Matter","ref_index":7,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XYX6BBXSZPFC3SHBNZZM5IKZGM","json":"https://pith.science/pith/XYX6BBXSZPFC3SHBNZZM5IKZGM.json","graph_json":"https://pith.science/api/pith-number/XYX6BBXSZPFC3SHBNZZM5IKZGM/graph.json","events_json":"https://pith.science/api/pith-number/XYX6BBXSZPFC3SHBNZZM5IKZGM/events.json","paper":"https://pith.science/paper/XYX6BBXS"},"agent_actions":{"view_html":"https://pith.science/pith/XYX6BBXSZPFC3SHBNZZM5IKZGM","download_json":"https://pith.science/pith/XYX6BBXSZPFC3SHBNZZM5IKZGM.json","view_paper":"https://pith.science/paper/XYX6BBXS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1611.02716&json=true","fetch_graph":"https://pith.science/api/pith-number/XYX6BBXSZPFC3SHBNZZM5IKZGM/graph.json","fetch_events":"https://pith.science/api/pith-number/XYX6BBXSZPFC3SHBNZZM5IKZGM/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XYX6BBXSZPFC3SHBNZZM5IKZGM/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XYX6BBXSZPFC3SHBNZZM5IKZGM/action/storage_attestation","attest_author":"https://pith.science/pith/XYX6BBXSZPFC3SHBNZZM5IKZGM/action/author_attestation","sign_citation":"https://pith.science/pith/XYX6BBXSZPFC3SHBNZZM5IKZGM/action/citation_signature","submit_replication":"https://pith.science/pith/XYX6BBXSZPFC3SHBNZZM5IKZGM/action/replication_record"}},"created_at":"2026-05-18T00:34:52.431168+00:00","updated_at":"2026-05-18T00:34:52.431168+00:00"}