{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:4A57CY5RILY3ZSHSH2XDCP4PYE","short_pith_number":"pith:4A57CY5R","schema_version":"1.0","canonical_sha256":"e03bf163b142f1bcc8f23eae313f8fc1116281c8c7e5892cf141cf8579dd5d31","source":{"kind":"arxiv","id":"2310.01560","version":3},"attestation_state":"computed","paper":{"title":"Remnant loop quantum black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"F. C. Sobrinho, H. A. Borges, I. P. R. Baranov, S. Carneiro","submitted_at":"2023-10-02T18:53:01Z","abstract_excerpt":"Polymer models inspired by Loop Quantum Gravity (LQG) have been used to describe non-singular quantum black holes with spherical symmetry, with the classical singularity replaced by a transition from a black hole to a white hole. A recent model, with a single polymerisation parameter, leads to a symmetric transition with same mass for the black and white phases, and to an asymptotically flat exterior metric. The radius of the transition surface is, however, not fixed, increasing with the mass. Following similar procedures, in a previous paper we have fixed that radius by identifying the minima"},"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":"2310.01560","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2023-10-02T18:53:01Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"614440a511822923a781c6cab59e0f32b72fa02313c327e5fa06ca3aac070f4e","abstract_canon_sha256":"58ad1604fd1e114483eca2094293e808d2ae7e7d6f6f1ec1b6f64158b57780af"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:39:30.660955Z","signature_b64":"dItcoUrlhTUCXZBsQEalQtzLcYojBKP30Pu3tmozjoox4LDtP4nYlCGbb9Glk77btMMkurDIKHUv68LF9/DlDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e03bf163b142f1bcc8f23eae313f8fc1116281c8c7e5892cf141cf8579dd5d31","last_reissued_at":"2026-07-05T07:39:30.660410Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:39:30.660410Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Remnant loop quantum black holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"F. C. Sobrinho, H. A. Borges, I. P. R. Baranov, S. Carneiro","submitted_at":"2023-10-02T18:53:01Z","abstract_excerpt":"Polymer models inspired by Loop Quantum Gravity (LQG) have been used to describe non-singular quantum black holes with spherical symmetry, with the classical singularity replaced by a transition from a black hole to a white hole. A recent model, with a single polymerisation parameter, leads to a symmetric transition with same mass for the black and white phases, and to an asymptotically flat exterior metric. The radius of the transition surface is, however, not fixed, increasing with the mass. Following similar procedures, in a previous paper we have fixed that radius by identifying the minima"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2310.01560","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/2310.01560/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":"2310.01560","created_at":"2026-07-05T07:39:30.660475+00:00"},{"alias_kind":"arxiv_version","alias_value":"2310.01560v3","created_at":"2026-07-05T07:39:30.660475+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2310.01560","created_at":"2026-07-05T07:39:30.660475+00:00"},{"alias_kind":"pith_short_12","alias_value":"4A57CY5RILY3","created_at":"2026-07-05T07:39:30.660475+00:00"},{"alias_kind":"pith_short_16","alias_value":"4A57CY5RILY3ZSHS","created_at":"2026-07-05T07:39:30.660475+00:00"},{"alias_kind":"pith_short_8","alias_value":"4A57CY5R","created_at":"2026-07-05T07:39:30.660475+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.11728","citing_title":"Periodic orbits as probes of charged loop quantum gravity black holes through gravitational waves","ref_index":26,"is_internal_anchor":false},{"citing_arxiv_id":"2603.25084","citing_title":"Particle motions and gravitational waveforms in rotating black hole spacetimes of loop quantum gravity","ref_index":35,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4A57CY5RILY3ZSHSH2XDCP4PYE","json":"https://pith.science/pith/4A57CY5RILY3ZSHSH2XDCP4PYE.json","graph_json":"https://pith.science/api/pith-number/4A57CY5RILY3ZSHSH2XDCP4PYE/graph.json","events_json":"https://pith.science/api/pith-number/4A57CY5RILY3ZSHSH2XDCP4PYE/events.json","paper":"https://pith.science/paper/4A57CY5R"},"agent_actions":{"view_html":"https://pith.science/pith/4A57CY5RILY3ZSHSH2XDCP4PYE","download_json":"https://pith.science/pith/4A57CY5RILY3ZSHSH2XDCP4PYE.json","view_paper":"https://pith.science/paper/4A57CY5R","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2310.01560&json=true","fetch_graph":"https://pith.science/api/pith-number/4A57CY5RILY3ZSHSH2XDCP4PYE/graph.json","fetch_events":"https://pith.science/api/pith-number/4A57CY5RILY3ZSHSH2XDCP4PYE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4A57CY5RILY3ZSHSH2XDCP4PYE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4A57CY5RILY3ZSHSH2XDCP4PYE/action/storage_attestation","attest_author":"https://pith.science/pith/4A57CY5RILY3ZSHSH2XDCP4PYE/action/author_attestation","sign_citation":"https://pith.science/pith/4A57CY5RILY3ZSHSH2XDCP4PYE/action/citation_signature","submit_replication":"https://pith.science/pith/4A57CY5RILY3ZSHSH2XDCP4PYE/action/replication_record"}},"created_at":"2026-07-05T07:39:30.660475+00:00","updated_at":"2026-07-05T07:39:30.660475+00:00"}