{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:JVKIMRQPCFQ5OW6I7WI56YLV2C","short_pith_number":"pith:JVKIMRQP","schema_version":"1.0","canonical_sha256":"4d5486460f1161d75bc8fd91df6175d0b7e203c2e7c3c054a2304aa4981f2bc4","source":{"kind":"arxiv","id":"1912.00470","version":3},"attestation_state":"computed","paper":{"title":"Static spherically symmetric configurations with N non-linear scalar fields: global and asymptotic properties","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"O.S. Stashko, V.I. Zhdanov","submitted_at":"2019-12-01T18:33:48Z","abstract_excerpt":"In case of a spherically symmetric non-linear scalar field (SF) in flat space, besides singularity at the center, spherical singularities can occur for non-zero values of radial variable $r>0$. We show that in the General Relativity the gravitational field suppresses the occurrence of the spherical singularities under some generic conditions. Our consideration deals with asymptotically flat space-times around static spherically symmetric configurations in presence of $N$ non-linear SFs, which are minimally coupled to gravity. Constraints are imposed on the SF potentials, which guarantee a mono"},"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":"1912.00470","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-12-01T18:33:48Z","cross_cats_sorted":[],"title_canon_sha256":"4d518e5abdc35eec58b8886b46c270bccda41c43caa6250908bf866ea4e5f835","abstract_canon_sha256":"7f11659ca816f6f8733ca09333b4505bdbb1195fda99b96fba848c0f10a5cef9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:51:35.030377Z","signature_b64":"F5w7MRyXkrvrfPXvWD9CRMyTxbpsyKUDLUCQrnKWMJstNDS4S9ovU8Ydp+9yRrrMbSPEI4SoE/tex9i1uFYMAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4d5486460f1161d75bc8fd91df6175d0b7e203c2e7c3c054a2304aa4981f2bc4","last_reissued_at":"2026-07-05T00:51:35.029957Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:51:35.029957Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Static spherically symmetric configurations with N non-linear scalar fields: global and asymptotic properties","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"O.S. Stashko, V.I. Zhdanov","submitted_at":"2019-12-01T18:33:48Z","abstract_excerpt":"In case of a spherically symmetric non-linear scalar field (SF) in flat space, besides singularity at the center, spherical singularities can occur for non-zero values of radial variable $r>0$. We show that in the General Relativity the gravitational field suppresses the occurrence of the spherical singularities under some generic conditions. Our consideration deals with asymptotically flat space-times around static spherically symmetric configurations in presence of $N$ non-linear SFs, which are minimally coupled to gravity. Constraints are imposed on the SF potentials, which guarantee a mono"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1912.00470","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/1912.00470/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":"1912.00470","created_at":"2026-07-05T00:51:35.030012+00:00"},{"alias_kind":"arxiv_version","alias_value":"1912.00470v3","created_at":"2026-07-05T00:51:35.030012+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1912.00470","created_at":"2026-07-05T00:51:35.030012+00:00"},{"alias_kind":"pith_short_12","alias_value":"JVKIMRQPCFQ5","created_at":"2026-07-05T00:51:35.030012+00:00"},{"alias_kind":"pith_short_16","alias_value":"JVKIMRQPCFQ5OW6I","created_at":"2026-07-05T00:51:35.030012+00:00"},{"alias_kind":"pith_short_8","alias_value":"JVKIMRQP","created_at":"2026-07-05T00:51:35.030012+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2412.03759","citing_title":"Universality in static spherically symmetric solutions of f(R) gravity","ref_index":40,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JVKIMRQPCFQ5OW6I7WI56YLV2C","json":"https://pith.science/pith/JVKIMRQPCFQ5OW6I7WI56YLV2C.json","graph_json":"https://pith.science/api/pith-number/JVKIMRQPCFQ5OW6I7WI56YLV2C/graph.json","events_json":"https://pith.science/api/pith-number/JVKIMRQPCFQ5OW6I7WI56YLV2C/events.json","paper":"https://pith.science/paper/JVKIMRQP"},"agent_actions":{"view_html":"https://pith.science/pith/JVKIMRQPCFQ5OW6I7WI56YLV2C","download_json":"https://pith.science/pith/JVKIMRQPCFQ5OW6I7WI56YLV2C.json","view_paper":"https://pith.science/paper/JVKIMRQP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1912.00470&json=true","fetch_graph":"https://pith.science/api/pith-number/JVKIMRQPCFQ5OW6I7WI56YLV2C/graph.json","fetch_events":"https://pith.science/api/pith-number/JVKIMRQPCFQ5OW6I7WI56YLV2C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JVKIMRQPCFQ5OW6I7WI56YLV2C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JVKIMRQPCFQ5OW6I7WI56YLV2C/action/storage_attestation","attest_author":"https://pith.science/pith/JVKIMRQPCFQ5OW6I7WI56YLV2C/action/author_attestation","sign_citation":"https://pith.science/pith/JVKIMRQPCFQ5OW6I7WI56YLV2C/action/citation_signature","submit_replication":"https://pith.science/pith/JVKIMRQPCFQ5OW6I7WI56YLV2C/action/replication_record"}},"created_at":"2026-07-05T00:51:35.030012+00:00","updated_at":"2026-07-05T00:51:35.030012+00:00"}