{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:BJKW3U2BXQHVHCD3YMI32A5G3R","short_pith_number":"pith:BJKW3U2B","schema_version":"1.0","canonical_sha256":"0a556dd341bc0f53887bc311bd03a6dc543a310c4fa0aa0d88eed8924521eb44","source":{"kind":"arxiv","id":"1812.03104","version":1},"attestation_state":"computed","paper":{"title":"Black hole formation in the context of dissipative dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"A. Lupi, D. R. G. Schleicher, G. D'Amico, M. A. Latif, P. Panci, S. Bovino","submitted_at":"2018-12-07T17:03:51Z","abstract_excerpt":"Black holes with masses of $\\rm 10^6-10^9~M_{\\odot}$ dwell in the centers of most galaxies, but their formation mechanisms are not well known. A subdominant dissipative component of dark matter with similar properties to the ordinary baryons, known as mirror dark matter, may collapse to form massive black holes during the epoch of first galaxies formation. In this study, we explore the possibility of massive black hole formation via this alternative scenario. We perform three-dimensional cosmological simulations for four distinct halos and compare their thermal, chemical and dynamical evolutio"},"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":"1812.03104","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.CO","submitted_at":"2018-12-07T17:03:51Z","cross_cats_sorted":["astro-ph.GA","hep-ph"],"title_canon_sha256":"077939f728e2abb0e848f818a49f36759c542f3377fd682e3142bede7eb43d87","abstract_canon_sha256":"bc79ff2eeb441fb553de82aba8a26ed35b96be35946c02dc498e737dd4711e79"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:50:56.465830Z","signature_b64":"QdjxrIdXvUtdg58NuH/xh9DCp+hjnJmpEkWz2sdUIBt2sM/Qzqe/Zh+SmRjRZtoCFuNlcDRirFYb8Dzgg1yCCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0a556dd341bc0f53887bc311bd03a6dc543a310c4fa0aa0d88eed8924521eb44","last_reissued_at":"2026-05-17T23:50:56.465045Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:50:56.465045Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black hole formation in the context of dissipative dark matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","hep-ph"],"primary_cat":"astro-ph.CO","authors_text":"A. Lupi, D. R. G. Schleicher, G. D'Amico, M. A. Latif, P. Panci, S. Bovino","submitted_at":"2018-12-07T17:03:51Z","abstract_excerpt":"Black holes with masses of $\\rm 10^6-10^9~M_{\\odot}$ dwell in the centers of most galaxies, but their formation mechanisms are not well known. A subdominant dissipative component of dark matter with similar properties to the ordinary baryons, known as mirror dark matter, may collapse to form massive black holes during the epoch of first galaxies formation. In this study, we explore the possibility of massive black hole formation via this alternative scenario. We perform three-dimensional cosmological simulations for four distinct halos and compare their thermal, chemical and dynamical evolutio"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1812.03104","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":"1812.03104","created_at":"2026-05-17T23:50:56.465159+00:00"},{"alias_kind":"arxiv_version","alias_value":"1812.03104v1","created_at":"2026-05-17T23:50:56.465159+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1812.03104","created_at":"2026-05-17T23:50:56.465159+00:00"},{"alias_kind":"pith_short_12","alias_value":"BJKW3U2BXQHV","created_at":"2026-05-18T12:32:16.446611+00:00"},{"alias_kind":"pith_short_16","alias_value":"BJKW3U2BXQHVHCD3","created_at":"2026-05-18T12:32:16.446611+00:00"},{"alias_kind":"pith_short_8","alias_value":"BJKW3U2B","created_at":"2026-05-18T12:32:16.446611+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/BJKW3U2BXQHVHCD3YMI32A5G3R","json":"https://pith.science/pith/BJKW3U2BXQHVHCD3YMI32A5G3R.json","graph_json":"https://pith.science/api/pith-number/BJKW3U2BXQHVHCD3YMI32A5G3R/graph.json","events_json":"https://pith.science/api/pith-number/BJKW3U2BXQHVHCD3YMI32A5G3R/events.json","paper":"https://pith.science/paper/BJKW3U2B"},"agent_actions":{"view_html":"https://pith.science/pith/BJKW3U2BXQHVHCD3YMI32A5G3R","download_json":"https://pith.science/pith/BJKW3U2BXQHVHCD3YMI32A5G3R.json","view_paper":"https://pith.science/paper/BJKW3U2B","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1812.03104&json=true","fetch_graph":"https://pith.science/api/pith-number/BJKW3U2BXQHVHCD3YMI32A5G3R/graph.json","fetch_events":"https://pith.science/api/pith-number/BJKW3U2BXQHVHCD3YMI32A5G3R/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BJKW3U2BXQHVHCD3YMI32A5G3R/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BJKW3U2BXQHVHCD3YMI32A5G3R/action/storage_attestation","attest_author":"https://pith.science/pith/BJKW3U2BXQHVHCD3YMI32A5G3R/action/author_attestation","sign_citation":"https://pith.science/pith/BJKW3U2BXQHVHCD3YMI32A5G3R/action/citation_signature","submit_replication":"https://pith.science/pith/BJKW3U2BXQHVHCD3YMI32A5G3R/action/replication_record"}},"created_at":"2026-05-17T23:50:56.465159+00:00","updated_at":"2026-05-17T23:50:56.465159+00:00"}