{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:THPFSC7JWGFP3ZU5HUU6U6OAUE","short_pith_number":"pith:THPFSC7J","schema_version":"1.0","canonical_sha256":"99de590be9b18afde69d3d29ea79c0a10c17fba224db4811b6e99df599dfc12e","source":{"kind":"arxiv","id":"2204.06568","version":2},"attestation_state":"computed","paper":{"title":"Universal gravothermal evolution of isolated self-interacting dark matter halos for velocity-dependent cross sections","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.GA","authors_text":"Kimberly K. Boddy, Laura Sagunski, Manoj Kaplinghat, Nadav Joseph Outmezguine, Sophia Gad-Nasr","submitted_at":"2022-04-13T18:00:00Z","abstract_excerpt":"We study the evolution of isolated self-interacting dark matter (SIDM) halos using spherically-symmetric gravothermal equations allowing for the scattering cross section to be velocity dependent. We focus our attention on the large class of models where the core is in the long mean free path regime for a substantial time. We find that the temporal evolution exhibits an approximate universality that allows velocity-dependent models to be mapped onto velocity-independent models in a well-defined way using the scattering timescale computed when the halo achieves its minimum central density. We sh"},"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":"2204.06568","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.GA","submitted_at":"2022-04-13T18:00:00Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"c30d56cf137a513f758c23121e27cf560a71b8fabac53594cf80e1b343f8a1a2","abstract_canon_sha256":"d9b166a64172cea035d0f0a87314224f0de657285e81d97e969024ac0a556519"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:23:53.616997Z","signature_b64":"8VCjdvAevdQNj/PhZgKzIElYGeDZEl1C/G+3KM1JMBn5dAUVvadFEPEydFiHsQr8NaHifw4uR0i4xVEo+QWoDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"99de590be9b18afde69d3d29ea79c0a10c17fba224db4811b6e99df599dfc12e","last_reissued_at":"2026-07-05T07:23:53.616588Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:23:53.616588Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Universal gravothermal evolution of isolated self-interacting dark matter halos for velocity-dependent cross sections","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.GA","authors_text":"Kimberly K. Boddy, Laura Sagunski, Manoj Kaplinghat, Nadav Joseph Outmezguine, Sophia Gad-Nasr","submitted_at":"2022-04-13T18:00:00Z","abstract_excerpt":"We study the evolution of isolated self-interacting dark matter (SIDM) halos using spherically-symmetric gravothermal equations allowing for the scattering cross section to be velocity dependent. We focus our attention on the large class of models where the core is in the long mean free path regime for a substantial time. We find that the temporal evolution exhibits an approximate universality that allows velocity-dependent models to be mapped onto velocity-independent models in a well-defined way using the scattering timescale computed when the halo achieves its minimum central density. We sh"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2204.06568","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2204.06568/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":"2204.06568","created_at":"2026-07-05T07:23:53.616646+00:00"},{"alias_kind":"arxiv_version","alias_value":"2204.06568v2","created_at":"2026-07-05T07:23:53.616646+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2204.06568","created_at":"2026-07-05T07:23:53.616646+00:00"},{"alias_kind":"pith_short_12","alias_value":"THPFSC7JWGFP","created_at":"2026-07-05T07:23:53.616646+00:00"},{"alias_kind":"pith_short_16","alias_value":"THPFSC7JWGFP3ZU5","created_at":"2026-07-05T07:23:53.616646+00:00"},{"alias_kind":"pith_short_8","alias_value":"THPFSC7J","created_at":"2026-07-05T07:23:53.616646+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.19428","citing_title":"Cooling, conduction, compact objects: Gravothermal evolution of dissipative self-interacting dark matter halos","ref_index":18,"is_internal_anchor":false},{"citing_arxiv_id":"2606.12909","citing_title":"SIDM and CDM interpretations of the million-solar-mass lensing perturber JVAS B1938+666-$\\mathcal{V}$","ref_index":16,"is_internal_anchor":false},{"citing_arxiv_id":"2607.02151","citing_title":"Spherically Symmetric Fluid Simulations of Black Hole Accretion in Self-Interacting Dark Matter Halos","ref_index":58,"is_internal_anchor":false},{"citing_arxiv_id":"2504.13004","citing_title":"Calibrating the SIDM Gravothermal Catastrophe with N-body Simulations","ref_index":54,"is_internal_anchor":false},{"citing_arxiv_id":"2506.14898","citing_title":"Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses","ref_index":21,"is_internal_anchor":false},{"citing_arxiv_id":"2601.17117","citing_title":"Non-Equilibrium Relativistic Core Collapse of Self-Interacting Dark Matter Halos -- Limits On Seed Black Hole Mass","ref_index":97,"is_internal_anchor":false},{"citing_arxiv_id":"2604.12189","citing_title":"Probing Collapsed Dark Matter Halos with Fast Radio Bursts","ref_index":57,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/THPFSC7JWGFP3ZU5HUU6U6OAUE","json":"https://pith.science/pith/THPFSC7JWGFP3ZU5HUU6U6OAUE.json","graph_json":"https://pith.science/api/pith-number/THPFSC7JWGFP3ZU5HUU6U6OAUE/graph.json","events_json":"https://pith.science/api/pith-number/THPFSC7JWGFP3ZU5HUU6U6OAUE/events.json","paper":"https://pith.science/paper/THPFSC7J"},"agent_actions":{"view_html":"https://pith.science/pith/THPFSC7JWGFP3ZU5HUU6U6OAUE","download_json":"https://pith.science/pith/THPFSC7JWGFP3ZU5HUU6U6OAUE.json","view_paper":"https://pith.science/paper/THPFSC7J","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2204.06568&json=true","fetch_graph":"https://pith.science/api/pith-number/THPFSC7JWGFP3ZU5HUU6U6OAUE/graph.json","fetch_events":"https://pith.science/api/pith-number/THPFSC7JWGFP3ZU5HUU6U6OAUE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/THPFSC7JWGFP3ZU5HUU6U6OAUE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/THPFSC7JWGFP3ZU5HUU6U6OAUE/action/storage_attestation","attest_author":"https://pith.science/pith/THPFSC7JWGFP3ZU5HUU6U6OAUE/action/author_attestation","sign_citation":"https://pith.science/pith/THPFSC7JWGFP3ZU5HUU6U6OAUE/action/citation_signature","submit_replication":"https://pith.science/pith/THPFSC7JWGFP3ZU5HUU6U6OAUE/action/replication_record"}},"created_at":"2026-07-05T07:23:53.616646+00:00","updated_at":"2026-07-05T07:23:53.616646+00:00"}