{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:47PVOXJHMKZOZJNFSPBHAN6ZMU","short_pith_number":"pith:47PVOXJH","schema_version":"1.0","canonical_sha256":"e7df575d2762b2eca5a593c27037d965375c6cc642b40f5f2b8f4d3d54973dbd","source":{"kind":"arxiv","id":"1704.07286","version":1},"attestation_state":"computed","paper":{"title":"Dark stars: gravitational and electromagnetic observables","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrea Maselli, Chris Kouvaris, Kostas D. Kokkotas, Niklas G{\\o}nlund Nielsen, Pantelis Pnigouras","submitted_at":"2017-04-24T15:32:26Z","abstract_excerpt":"Theoretical models of self-interacting dark matter represent a promising answer to a series of open problems within the so-called collisionless cold dark matter (CCDM) paradigm. In case of asymmetric dark matter, self-interactions might facilitate gravitational collapse and potentially lead to formation of compact objects predominantly made of dark matter. Considering both fermionic and bosonic equations of state, we construct the equilibrium structure of rotating dark stars, focusing on their bulk properties, and comparing them with baryonic neutron stars. We also show that these dark objects"},"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":"1704.07286","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-04-24T15:32:26Z","cross_cats_sorted":[],"title_canon_sha256":"09ce0ac00134c409bbeadacc2f97d950683198396457ecbc41a1c76aab75dd40","abstract_canon_sha256":"ec0c54b61c4735555d7d4bdcc0e174399bd6e240c8c8539a4d9336c6d8e6d395"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:38:55.169380Z","signature_b64":"S4FWw0Kef7gchOfjjgnDdw1oQD5uGqT7pNxvAtJ3ibEJzSKfDyLlJ9qgM+G8YtvakzGv1NESnilbTjXqI0qkBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e7df575d2762b2eca5a593c27037d965375c6cc642b40f5f2b8f4d3d54973dbd","last_reissued_at":"2026-05-18T00:38:55.168788Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:38:55.168788Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dark stars: gravitational and electromagnetic observables","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrea Maselli, Chris Kouvaris, Kostas D. Kokkotas, Niklas G{\\o}nlund Nielsen, Pantelis Pnigouras","submitted_at":"2017-04-24T15:32:26Z","abstract_excerpt":"Theoretical models of self-interacting dark matter represent a promising answer to a series of open problems within the so-called collisionless cold dark matter (CCDM) paradigm. In case of asymmetric dark matter, self-interactions might facilitate gravitational collapse and potentially lead to formation of compact objects predominantly made of dark matter. Considering both fermionic and bosonic equations of state, we construct the equilibrium structure of rotating dark stars, focusing on their bulk properties, and comparing them with baryonic neutron stars. We also show that these dark objects"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.07286","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":"1704.07286","created_at":"2026-05-18T00:38:55.168869+00:00"},{"alias_kind":"arxiv_version","alias_value":"1704.07286v1","created_at":"2026-05-18T00:38:55.168869+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.07286","created_at":"2026-05-18T00:38:55.168869+00:00"},{"alias_kind":"pith_short_12","alias_value":"47PVOXJHMKZO","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_16","alias_value":"47PVOXJHMKZOZJNF","created_at":"2026-05-18T12:30:58.224056+00:00"},{"alias_kind":"pith_short_8","alias_value":"47PVOXJH","created_at":"2026-05-18T12:30:58.224056+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2504.17064","citing_title":"Imprints of energy injection by compact dark stars in the 21-cm signal","ref_index":18,"is_internal_anchor":true},{"citing_arxiv_id":"2605.10467","citing_title":"Axial Quasi-normal Modes of Admixed Neutron Stars","ref_index":14,"is_internal_anchor":false},{"citing_arxiv_id":"2605.02633","citing_title":"Axial tidal Love numbers of black holes in matter environments","ref_index":51,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/47PVOXJHMKZOZJNFSPBHAN6ZMU","json":"https://pith.science/pith/47PVOXJHMKZOZJNFSPBHAN6ZMU.json","graph_json":"https://pith.science/api/pith-number/47PVOXJHMKZOZJNFSPBHAN6ZMU/graph.json","events_json":"https://pith.science/api/pith-number/47PVOXJHMKZOZJNFSPBHAN6ZMU/events.json","paper":"https://pith.science/paper/47PVOXJH"},"agent_actions":{"view_html":"https://pith.science/pith/47PVOXJHMKZOZJNFSPBHAN6ZMU","download_json":"https://pith.science/pith/47PVOXJHMKZOZJNFSPBHAN6ZMU.json","view_paper":"https://pith.science/paper/47PVOXJH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1704.07286&json=true","fetch_graph":"https://pith.science/api/pith-number/47PVOXJHMKZOZJNFSPBHAN6ZMU/graph.json","fetch_events":"https://pith.science/api/pith-number/47PVOXJHMKZOZJNFSPBHAN6ZMU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/47PVOXJHMKZOZJNFSPBHAN6ZMU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/47PVOXJHMKZOZJNFSPBHAN6ZMU/action/storage_attestation","attest_author":"https://pith.science/pith/47PVOXJHMKZOZJNFSPBHAN6ZMU/action/author_attestation","sign_citation":"https://pith.science/pith/47PVOXJHMKZOZJNFSPBHAN6ZMU/action/citation_signature","submit_replication":"https://pith.science/pith/47PVOXJHMKZOZJNFSPBHAN6ZMU/action/replication_record"}},"created_at":"2026-05-18T00:38:55.168869+00:00","updated_at":"2026-05-18T00:38:55.168869+00:00"}