{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:A6F4EW7G6C6PATV4WORXLYCF4R","short_pith_number":"pith:A6F4EW7G","schema_version":"1.0","canonical_sha256":"078bc25be6f0bcf04ebcb3a375e045e45ae3c2fd2c6b3af56f0c8d9c7960fccb","source":{"kind":"arxiv","id":"1908.07986","version":1},"attestation_state":"computed","paper":{"title":"Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","nucl-th"],"primary_cat":"gr-qc","authors_text":"A. A. Hujeirat, R. Samtaney","submitted_at":"2019-08-21T16:57:06Z","abstract_excerpt":"We present a modification of our previous model for the mechanisms underlying the glitch phenomena in pulsars and young neutron stars. Accordingly, pulsars are born with embryonic cores comprising of purely incompressible superconducting gluon-quark superfluid (henceforth SuSu-cores). As the ambient medium cools and spins down due to emission of magnetic dipole radiation, the mass and size of SuSu-cores are set to grow discretely with time, in accordance with the Onsager-Feynmann analysis of superfluidity. Presently, we propose that the spacetime embedding glitching pulsars is dynamical and of"},"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":"1908.07986","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-08-21T16:57:06Z","cross_cats_sorted":["astro-ph.HE","nucl-th"],"title_canon_sha256":"aaca33b144f359de5cf87f15f1e1d973c6390f5c84330fbac0c70caf504b60ca","abstract_canon_sha256":"a8f107c619826bead81d53eddaa18a592d19fffc523635e69d6c7d32f79a1ebe"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:17:18.429886Z","signature_b64":"GkajU6ClIQ02ciW4GgF1f79ocgdrzoXk+qQNJnJFiVbgGZdtvGilJdyVhI8qEh0TAKV+xA64ScSuQhK8jPc1Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"078bc25be6f0bcf04ebcb3a375e045e45ae3c2fd2c6b3af56f0c8d9c7960fccb","last_reissued_at":"2026-07-05T02:17:18.429473Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:17:18.429473Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Glitching pulsars: unraveling the interactions of general relativity with quantum fields in the strong field regimes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","nucl-th"],"primary_cat":"gr-qc","authors_text":"A. A. Hujeirat, R. Samtaney","submitted_at":"2019-08-21T16:57:06Z","abstract_excerpt":"We present a modification of our previous model for the mechanisms underlying the glitch phenomena in pulsars and young neutron stars. Accordingly, pulsars are born with embryonic cores comprising of purely incompressible superconducting gluon-quark superfluid (henceforth SuSu-cores). As the ambient medium cools and spins down due to emission of magnetic dipole radiation, the mass and size of SuSu-cores are set to grow discretely with time, in accordance with the Onsager-Feynmann analysis of superfluidity. Presently, we propose that the spacetime embedding glitching pulsars is dynamical and of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1908.07986","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1908.07986/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":"1908.07986","created_at":"2026-07-05T02:17:18.429533+00:00"},{"alias_kind":"arxiv_version","alias_value":"1908.07986v1","created_at":"2026-07-05T02:17:18.429533+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1908.07986","created_at":"2026-07-05T02:17:18.429533+00:00"},{"alias_kind":"pith_short_12","alias_value":"A6F4EW7G6C6P","created_at":"2026-07-05T02:17:18.429533+00:00"},{"alias_kind":"pith_short_16","alias_value":"A6F4EW7G6C6PATV4","created_at":"2026-07-05T02:17:18.429533+00:00"},{"alias_kind":"pith_short_8","alias_value":"A6F4EW7G","created_at":"2026-07-05T02:17:18.429533+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/A6F4EW7G6C6PATV4WORXLYCF4R","json":"https://pith.science/pith/A6F4EW7G6C6PATV4WORXLYCF4R.json","graph_json":"https://pith.science/api/pith-number/A6F4EW7G6C6PATV4WORXLYCF4R/graph.json","events_json":"https://pith.science/api/pith-number/A6F4EW7G6C6PATV4WORXLYCF4R/events.json","paper":"https://pith.science/paper/A6F4EW7G"},"agent_actions":{"view_html":"https://pith.science/pith/A6F4EW7G6C6PATV4WORXLYCF4R","download_json":"https://pith.science/pith/A6F4EW7G6C6PATV4WORXLYCF4R.json","view_paper":"https://pith.science/paper/A6F4EW7G","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1908.07986&json=true","fetch_graph":"https://pith.science/api/pith-number/A6F4EW7G6C6PATV4WORXLYCF4R/graph.json","fetch_events":"https://pith.science/api/pith-number/A6F4EW7G6C6PATV4WORXLYCF4R/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/A6F4EW7G6C6PATV4WORXLYCF4R/action/timestamp_anchor","attest_storage":"https://pith.science/pith/A6F4EW7G6C6PATV4WORXLYCF4R/action/storage_attestation","attest_author":"https://pith.science/pith/A6F4EW7G6C6PATV4WORXLYCF4R/action/author_attestation","sign_citation":"https://pith.science/pith/A6F4EW7G6C6PATV4WORXLYCF4R/action/citation_signature","submit_replication":"https://pith.science/pith/A6F4EW7G6C6PATV4WORXLYCF4R/action/replication_record"}},"created_at":"2026-07-05T02:17:18.429533+00:00","updated_at":"2026-07-05T02:17:18.429533+00:00"}