{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:DABWNRR5FOGTRCOW7VJUWRSDKX","short_pith_number":"pith:DABWNRR5","schema_version":"1.0","canonical_sha256":"180366c63d2b8d3889d6fd534b464355f0d688d80d91c13e157895457219314d","source":{"kind":"arxiv","id":"astro-ph/0603613","version":1},"attestation_state":"computed","paper":{"title":"Gravitational cooling of self-gravitating Bose-Condensates","license":"","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"astro-ph","authors_text":"F. Siddhartha Guzman, L. Arturo Urena-Lopez","submitted_at":"2006-03-22T18:53:13Z","abstract_excerpt":"Equilibrium configurations for a self-gravitating scalar field with self-interaction are constructed. The corresponding Schr\\\"odinger-Poisson (SP) system is solved using finite differences assuming spherical symmetry. It is shown that equilibrium configurations of the SP system are late-time attractor solutions for initially quite arbitrary density profiles, which relax and virialize through the emission of scalar field bursts; a process dubbed gravitational cooling. Among other potential applications, these results indicate that scalar field dark matter models (in its different flavors) toler"},"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":"astro-ph/0603613","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-03-22T18:53:13Z","cross_cats_sorted":["gr-qc","hep-th"],"title_canon_sha256":"25aeedabec5793a88556781018fa8cfdb41ecae3f2ca6a5128e1f1193f8228ec","abstract_canon_sha256":"4a56cd45c01083cfbd45fb4c29f233d9a646000e084f376e53f67ed9e6f37512"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:36:21.569392Z","signature_b64":"Kjv+sot64C2xmG/KTfb99MSQltUX2W7M/qhA+SMKpAOGa/w45wtWDSqFn2SZwIPEgKCk+5ZSMyvq+dmJ7nSnDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"180366c63d2b8d3889d6fd534b464355f0d688d80d91c13e157895457219314d","last_reissued_at":"2026-05-18T04:36:21.568871Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:36:21.568871Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational cooling of self-gravitating Bose-Condensates","license":"","headline":"","cross_cats":["gr-qc","hep-th"],"primary_cat":"astro-ph","authors_text":"F. Siddhartha Guzman, L. Arturo Urena-Lopez","submitted_at":"2006-03-22T18:53:13Z","abstract_excerpt":"Equilibrium configurations for a self-gravitating scalar field with self-interaction are constructed. The corresponding Schr\\\"odinger-Poisson (SP) system is solved using finite differences assuming spherical symmetry. It is shown that equilibrium configurations of the SP system are late-time attractor solutions for initially quite arbitrary density profiles, which relax and virialize through the emission of scalar field bursts; a process dubbed gravitational cooling. Among other potential applications, these results indicate that scalar field dark matter models (in its different flavors) toler"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0603613","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":"astro-ph/0603613","created_at":"2026-05-18T04:36:21.568954+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0603613v1","created_at":"2026-05-18T04:36:21.568954+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0603613","created_at":"2026-05-18T04:36:21.568954+00:00"},{"alias_kind":"pith_short_12","alias_value":"DABWNRR5FOGT","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_16","alias_value":"DABWNRR5FOGTRCOW","created_at":"2026-05-18T12:25:53.939244+00:00"},{"alias_kind":"pith_short_8","alias_value":"DABWNRR5","created_at":"2026-05-18T12:25:53.939244+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"1907.08193","citing_title":"The three dynamical fates of Boson Stars","ref_index":1,"is_internal_anchor":true},{"citing_arxiv_id":"1202.5809","citing_title":"Dynamical Boson Stars","ref_index":235,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DABWNRR5FOGTRCOW7VJUWRSDKX","json":"https://pith.science/pith/DABWNRR5FOGTRCOW7VJUWRSDKX.json","graph_json":"https://pith.science/api/pith-number/DABWNRR5FOGTRCOW7VJUWRSDKX/graph.json","events_json":"https://pith.science/api/pith-number/DABWNRR5FOGTRCOW7VJUWRSDKX/events.json","paper":"https://pith.science/paper/DABWNRR5"},"agent_actions":{"view_html":"https://pith.science/pith/DABWNRR5FOGTRCOW7VJUWRSDKX","download_json":"https://pith.science/pith/DABWNRR5FOGTRCOW7VJUWRSDKX.json","view_paper":"https://pith.science/paper/DABWNRR5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0603613&json=true","fetch_graph":"https://pith.science/api/pith-number/DABWNRR5FOGTRCOW7VJUWRSDKX/graph.json","fetch_events":"https://pith.science/api/pith-number/DABWNRR5FOGTRCOW7VJUWRSDKX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DABWNRR5FOGTRCOW7VJUWRSDKX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DABWNRR5FOGTRCOW7VJUWRSDKX/action/storage_attestation","attest_author":"https://pith.science/pith/DABWNRR5FOGTRCOW7VJUWRSDKX/action/author_attestation","sign_citation":"https://pith.science/pith/DABWNRR5FOGTRCOW7VJUWRSDKX/action/citation_signature","submit_replication":"https://pith.science/pith/DABWNRR5FOGTRCOW7VJUWRSDKX/action/replication_record"}},"created_at":"2026-05-18T04:36:21.568954+00:00","updated_at":"2026-05-18T04:36:21.568954+00:00"}