{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:BFC653Q2FQHMKMAWSY4TCLOB7U","short_pith_number":"pith:BFC653Q2","schema_version":"1.0","canonical_sha256":"0945eeee1a2c0ec530169639312dc1fd32928c6e3388b7a416215be189061b5e","source":{"kind":"arxiv","id":"2209.00064","version":3},"attestation_state":"computed","paper":{"title":"A Lower Bound on the Mass of Compact Objects from Dissipative Dark Matter","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Donghui Jeong, James Gurian, Michael Ryan, Sarah Schon, Sarah Shandera","submitted_at":"2022-08-31T18:48:29Z","abstract_excerpt":"We study the minimum mass of dark compact objects formed in dissipative dark-matter halos and show that the simple atomic-dark-matter model consistent with all current observations can create low-mass fragments that can evolve into compact objects forbidden by stellar astrophysics. We model the collapse of the dark halo's dense core by tracing the thermo-chemical evolution of a uniform-density volume element under two extreme assumptions for density evolution: hydrostatic equilibrium and pressure-free collapse. We then compute the opacity-limited minimum fragment mass from the minimum temperat"},"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":"2209.00064","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.CO","submitted_at":"2022-08-31T18:48:29Z","cross_cats_sorted":[],"title_canon_sha256":"4a53c752cabb9446cf8054219a5d1dad3fe7ebf46e95e38290765b045f8ba690","abstract_canon_sha256":"b056dda556e85d5aaa89409d0844516ee3e9d3db3f6b8c81dc03c389665b4e41"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:11:01.267164Z","signature_b64":"E3KHig0p5LhjNXXlYgKMfMDe1jgQXvRrGrtXsj3UofBXDYFbCJXTgmZdvgyXRkIDgwc7OKdUEo7nN2kQlve6Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0945eeee1a2c0ec530169639312dc1fd32928c6e3388b7a416215be189061b5e","last_reissued_at":"2026-07-05T06:11:01.266744Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:11:01.266744Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A Lower Bound on the Mass of Compact Objects from Dissipative Dark Matter","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.CO","authors_text":"Donghui Jeong, James Gurian, Michael Ryan, Sarah Schon, Sarah Shandera","submitted_at":"2022-08-31T18:48:29Z","abstract_excerpt":"We study the minimum mass of dark compact objects formed in dissipative dark-matter halos and show that the simple atomic-dark-matter model consistent with all current observations can create low-mass fragments that can evolve into compact objects forbidden by stellar astrophysics. We model the collapse of the dark halo's dense core by tracing the thermo-chemical evolution of a uniform-density volume element under two extreme assumptions for density evolution: hydrostatic equilibrium and pressure-free collapse. We then compute the opacity-limited minimum fragment mass from the minimum temperat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2209.00064","kind":"arxiv","version":3},"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/2209.00064/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":"2209.00064","created_at":"2026-07-05T06:11:01.266800+00:00"},{"alias_kind":"arxiv_version","alias_value":"2209.00064v3","created_at":"2026-07-05T06:11:01.266800+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2209.00064","created_at":"2026-07-05T06:11:01.266800+00:00"},{"alias_kind":"pith_short_12","alias_value":"BFC653Q2FQHM","created_at":"2026-07-05T06:11:01.266800+00:00"},{"alias_kind":"pith_short_16","alias_value":"BFC653Q2FQHMKMAW","created_at":"2026-07-05T06:11:01.266800+00:00"},{"alias_kind":"pith_short_8","alias_value":"BFC653Q2","created_at":"2026-07-05T06:11:01.266800+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"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":19,"is_internal_anchor":false},{"citing_arxiv_id":"2606.28482","citing_title":"Strongest constraints on dark acoustic oscillations from the Lyman-alpha forest","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25434","citing_title":"Microlensing of fast and slow compact objects","ref_index":33,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/BFC653Q2FQHMKMAWSY4TCLOB7U","json":"https://pith.science/pith/BFC653Q2FQHMKMAWSY4TCLOB7U.json","graph_json":"https://pith.science/api/pith-number/BFC653Q2FQHMKMAWSY4TCLOB7U/graph.json","events_json":"https://pith.science/api/pith-number/BFC653Q2FQHMKMAWSY4TCLOB7U/events.json","paper":"https://pith.science/paper/BFC653Q2"},"agent_actions":{"view_html":"https://pith.science/pith/BFC653Q2FQHMKMAWSY4TCLOB7U","download_json":"https://pith.science/pith/BFC653Q2FQHMKMAWSY4TCLOB7U.json","view_paper":"https://pith.science/paper/BFC653Q2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2209.00064&json=true","fetch_graph":"https://pith.science/api/pith-number/BFC653Q2FQHMKMAWSY4TCLOB7U/graph.json","fetch_events":"https://pith.science/api/pith-number/BFC653Q2FQHMKMAWSY4TCLOB7U/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BFC653Q2FQHMKMAWSY4TCLOB7U/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BFC653Q2FQHMKMAWSY4TCLOB7U/action/storage_attestation","attest_author":"https://pith.science/pith/BFC653Q2FQHMKMAWSY4TCLOB7U/action/author_attestation","sign_citation":"https://pith.science/pith/BFC653Q2FQHMKMAWSY4TCLOB7U/action/citation_signature","submit_replication":"https://pith.science/pith/BFC653Q2FQHMKMAWSY4TCLOB7U/action/replication_record"}},"created_at":"2026-07-05T06:11:01.266800+00:00","updated_at":"2026-07-05T06:11:01.266800+00:00"}