{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:LQS7ULVD2JCDJJ6RDCL7WD7H2I","short_pith_number":"pith:LQS7ULVD","schema_version":"1.0","canonical_sha256":"5c25fa2ea3d24434a7d11897fb0fe7d20397c92e002ee534c34629c57fa331ae","source":{"kind":"arxiv","id":"1305.4241","version":1},"attestation_state":"computed","paper":{"title":"On charged boson stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Daniela Pugliese, Hernando Quevedo, Jorge A. Rueda H., Remo Ruffini","submitted_at":"2013-05-18T08:21:48Z","abstract_excerpt":"We study static, spherically symmetric, self-gravitating systems minimally coupled to a scalar field with U(1) gauge symmetry: charged boson stars. We find numerical solutions to the EinsteinMaxwell equations coupled to the relativistic Klein-Gordon equation. It is shown that bound stable configurations exist only for values of the coupling constant less than or equal to a certain critical value. The metric coefficients and the relevant physical quantities such as the total mass and charge, turn out to be in general bound functions of the radial coordinate, reaching their maximum values at a c"},"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":"1305.4241","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2013-05-18T08:21:48Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"367d19cd1fe954cdfa057c951878c7cab048bb5fb26651872128324f22fe0b41","abstract_canon_sha256":"f91ae7306503cee749db221bbf3264c3f36651dceaf0b0ac67c0a1b1197b9efa"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:16:50.978306Z","signature_b64":"eWZEbV/CYYsTJfxHkX01qFI1cXOTrnKC3wcHjwpuVnuueHAruz5z5vyLQZ0+euz8ZtGgpv4VNyN5ZahrVYLEAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5c25fa2ea3d24434a7d11897fb0fe7d20397c92e002ee534c34629c57fa331ae","last_reissued_at":"2026-05-18T03:16:50.977435Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:16:50.977435Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On charged boson stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Daniela Pugliese, Hernando Quevedo, Jorge A. Rueda H., Remo Ruffini","submitted_at":"2013-05-18T08:21:48Z","abstract_excerpt":"We study static, spherically symmetric, self-gravitating systems minimally coupled to a scalar field with U(1) gauge symmetry: charged boson stars. We find numerical solutions to the EinsteinMaxwell equations coupled to the relativistic Klein-Gordon equation. It is shown that bound stable configurations exist only for values of the coupling constant less than or equal to a certain critical value. The metric coefficients and the relevant physical quantities such as the total mass and charge, turn out to be in general bound functions of the radial coordinate, reaching their maximum values at a c"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1305.4241","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":"1305.4241","created_at":"2026-05-18T03:16:50.977563+00:00"},{"alias_kind":"arxiv_version","alias_value":"1305.4241v1","created_at":"2026-05-18T03:16:50.977563+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1305.4241","created_at":"2026-05-18T03:16:50.977563+00:00"},{"alias_kind":"pith_short_12","alias_value":"LQS7ULVD2JCD","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_16","alias_value":"LQS7ULVD2JCDJJ6R","created_at":"2026-05-18T12:27:51.066281+00:00"},{"alias_kind":"pith_short_8","alias_value":"LQS7ULVD","created_at":"2026-05-18T12:27:51.066281+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.20450","citing_title":"Splitting the Gravitational Atom: Instabilities of Black Holes with Synchronized or Resonant Hair","ref_index":57,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LQS7ULVD2JCDJJ6RDCL7WD7H2I","json":"https://pith.science/pith/LQS7ULVD2JCDJJ6RDCL7WD7H2I.json","graph_json":"https://pith.science/api/pith-number/LQS7ULVD2JCDJJ6RDCL7WD7H2I/graph.json","events_json":"https://pith.science/api/pith-number/LQS7ULVD2JCDJJ6RDCL7WD7H2I/events.json","paper":"https://pith.science/paper/LQS7ULVD"},"agent_actions":{"view_html":"https://pith.science/pith/LQS7ULVD2JCDJJ6RDCL7WD7H2I","download_json":"https://pith.science/pith/LQS7ULVD2JCDJJ6RDCL7WD7H2I.json","view_paper":"https://pith.science/paper/LQS7ULVD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1305.4241&json=true","fetch_graph":"https://pith.science/api/pith-number/LQS7ULVD2JCDJJ6RDCL7WD7H2I/graph.json","fetch_events":"https://pith.science/api/pith-number/LQS7ULVD2JCDJJ6RDCL7WD7H2I/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LQS7ULVD2JCDJJ6RDCL7WD7H2I/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LQS7ULVD2JCDJJ6RDCL7WD7H2I/action/storage_attestation","attest_author":"https://pith.science/pith/LQS7ULVD2JCDJJ6RDCL7WD7H2I/action/author_attestation","sign_citation":"https://pith.science/pith/LQS7ULVD2JCDJJ6RDCL7WD7H2I/action/citation_signature","submit_replication":"https://pith.science/pith/LQS7ULVD2JCDJJ6RDCL7WD7H2I/action/replication_record"}},"created_at":"2026-05-18T03:16:50.977563+00:00","updated_at":"2026-05-18T03:16:50.977563+00:00"}