{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2026:YWEULRFL6YEJJ3KVWHEWHE2WUD","short_pith_number":"pith:YWEULRFL","schema_version":"1.0","canonical_sha256":"c58945c4abf60894ed55b1c9639356a0ff184a75dd42ac2482dea8d81c31675f","source":{"kind":"arxiv","id":"2605.31335","version":1},"attestation_state":"computed","paper":{"title":"Gravothermal Collapse: Robust Against Baryonic Feedback","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Demao Kong, Hai-Bo Yu","submitted_at":"2026-05-29T14:16:44Z","abstract_excerpt":"We perform a stress test of gravothermal collapse in self-interacting dark matter (SIDM) halos under baryonic feedback using a semi-analytical oscillating-potential model in controlled N-body simulations. For high-concentration halos, where the SIDM thermalization timescale is short, gravothermal collapse is only mildly delayed and never stalled, even under extremely strong feedback. In contrast, the collapse of a median-concentration halo can be significantly delayed, but it resumes once feedback ceases. The final density profile of such halos depends sensitively on the episodic feedback hist"},"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":"2605.31335","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2026-05-29T14:16:44Z","cross_cats_sorted":["astro-ph.GA","hep-ph"],"title_canon_sha256":"fe09303dd17f79c553a7ec11877293a11908b71d09b82a230fbbe67a7e1fa597","abstract_canon_sha256":"ffbb638190a17815669e9ca63ed69332878bac8ba2c9d3667ae3fc271b733976"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-01T02:03:59.243642Z","signature_b64":"0BH0Mfg+e8UVikR5DEro7F+joHOcJSNTgh+HOuDEsl+PEbwGu729SYJuJK0MQklLegABEHQ8XmOtaUnG5I47Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c58945c4abf60894ed55b1c9639356a0ff184a75dd42ac2482dea8d81c31675f","last_reissued_at":"2026-06-01T02:03:59.242752Z","signature_status":"signed_v1","first_computed_at":"2026-06-01T02:03:59.242752Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravothermal Collapse: Robust Against Baryonic Feedback","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.GA","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"Demao Kong, Hai-Bo Yu","submitted_at":"2026-05-29T14:16:44Z","abstract_excerpt":"We perform a stress test of gravothermal collapse in self-interacting dark matter (SIDM) halos under baryonic feedback using a semi-analytical oscillating-potential model in controlled N-body simulations. For high-concentration halos, where the SIDM thermalization timescale is short, gravothermal collapse is only mildly delayed and never stalled, even under extremely strong feedback. In contrast, the collapse of a median-concentration halo can be significantly delayed, but it resumes once feedback ceases. The final density profile of such halos depends sensitively on the episodic feedback hist"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2605.31335","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/2605.31335/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":"2605.31335","created_at":"2026-06-01T02:03:59.242884+00:00"},{"alias_kind":"arxiv_version","alias_value":"2605.31335v1","created_at":"2026-06-01T02:03:59.242884+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.31335","created_at":"2026-06-01T02:03:59.242884+00:00"},{"alias_kind":"pith_short_12","alias_value":"YWEULRFL6YEJ","created_at":"2026-06-01T02:03:59.242884+00:00"},{"alias_kind":"pith_short_16","alias_value":"YWEULRFL6YEJJ3KV","created_at":"2026-06-01T02:03:59.242884+00:00"},{"alias_kind":"pith_short_8","alias_value":"YWEULRFL","created_at":"2026-06-01T02:03:59.242884+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YWEULRFL6YEJJ3KVWHEWHE2WUD","json":"https://pith.science/pith/YWEULRFL6YEJJ3KVWHEWHE2WUD.json","graph_json":"https://pith.science/api/pith-number/YWEULRFL6YEJJ3KVWHEWHE2WUD/graph.json","events_json":"https://pith.science/api/pith-number/YWEULRFL6YEJJ3KVWHEWHE2WUD/events.json","paper":"https://pith.science/paper/YWEULRFL"},"agent_actions":{"view_html":"https://pith.science/pith/YWEULRFL6YEJJ3KVWHEWHE2WUD","download_json":"https://pith.science/pith/YWEULRFL6YEJJ3KVWHEWHE2WUD.json","view_paper":"https://pith.science/paper/YWEULRFL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2605.31335&json=true","fetch_graph":"https://pith.science/api/pith-number/YWEULRFL6YEJJ3KVWHEWHE2WUD/graph.json","fetch_events":"https://pith.science/api/pith-number/YWEULRFL6YEJJ3KVWHEWHE2WUD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YWEULRFL6YEJJ3KVWHEWHE2WUD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YWEULRFL6YEJJ3KVWHEWHE2WUD/action/storage_attestation","attest_author":"https://pith.science/pith/YWEULRFL6YEJJ3KVWHEWHE2WUD/action/author_attestation","sign_citation":"https://pith.science/pith/YWEULRFL6YEJJ3KVWHEWHE2WUD/action/citation_signature","submit_replication":"https://pith.science/pith/YWEULRFL6YEJJ3KVWHEWHE2WUD/action/replication_record"}},"created_at":"2026-06-01T02:03:59.242884+00:00","updated_at":"2026-06-01T02:03:59.242884+00:00"}