{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:4GURRIK4PD4SOIF45E42HFR47F","short_pith_number":"pith:4GURRIK4","schema_version":"1.0","canonical_sha256":"e1a918a15c78f92720bce939a3963cf94994ddbfde0967c918bc7e80a9cd7103","source":{"kind":"arxiv","id":"1907.12843","version":2},"attestation_state":"computed","paper":{"title":"Domain walls in neutron $^{3}P_{2}$ superfluids in neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph","hep-th"],"primary_cat":"nucl-th","authors_text":"Muneto Nitta, Shigehiro Yasui","submitted_at":"2019-07-30T11:51:48Z","abstract_excerpt":"We work out domain walls in neutron $^{3}P_{2}$ superfluids realized in the core of neutron stars. Adopting the Ginzburg-Landau (GL) theory as a bosonic low-energy effective theory, we consider configurations of domain walls interpolating ground states, i.e., the uniaxial nematic (UN), D$_{2}$-biaxial nematic (D$_{2}$-BN), and D$_{4}$-biaxial nematic (D$_{4}$-BN) phases in the presence of zero, small and large magnetic fields, respectively. We solve the Euler-Lagrange equation from the GL free energy density, and calculate surface energy densities of the domain walls. We find that one extra Na"},"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":"1907.12843","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2019-07-30T11:51:48Z","cross_cats_sorted":["astro-ph.HE","hep-ph","hep-th"],"title_canon_sha256":"a6bda7f6ac931b36e5bcbee9b326037a9311e59f54bf7897d85832b31e3ca155","abstract_canon_sha256":"20b57a71bc4067466e7d70c5ea9db918843998fad53a1395bf1a51b84332a611"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:36:30.463293Z","signature_b64":"omVpYpHeUKLOPYkJDeeiENoeHVeFj/roQCIVFQrWgAiMj4gmb2j7/XSEgbPZ4QMpEQ7qvXTsx2/7BmP/y1QEAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e1a918a15c78f92720bce939a3963cf94994ddbfde0967c918bc7e80a9cd7103","last_reissued_at":"2026-07-05T00:36:30.462884Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:36:30.462884Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Domain walls in neutron $^{3}P_{2}$ superfluids in neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ph","hep-th"],"primary_cat":"nucl-th","authors_text":"Muneto Nitta, Shigehiro Yasui","submitted_at":"2019-07-30T11:51:48Z","abstract_excerpt":"We work out domain walls in neutron $^{3}P_{2}$ superfluids realized in the core of neutron stars. Adopting the Ginzburg-Landau (GL) theory as a bosonic low-energy effective theory, we consider configurations of domain walls interpolating ground states, i.e., the uniaxial nematic (UN), D$_{2}$-biaxial nematic (D$_{2}$-BN), and D$_{4}$-biaxial nematic (D$_{4}$-BN) phases in the presence of zero, small and large magnetic fields, respectively. We solve the Euler-Lagrange equation from the GL free energy density, and calculate surface energy densities of the domain walls. We find that one extra Na"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1907.12843","kind":"arxiv","version":2},"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/1907.12843/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":"1907.12843","created_at":"2026-07-05T00:36:30.462939+00:00"},{"alias_kind":"arxiv_version","alias_value":"1907.12843v2","created_at":"2026-07-05T00:36:30.462939+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1907.12843","created_at":"2026-07-05T00:36:30.462939+00:00"},{"alias_kind":"pith_short_12","alias_value":"4GURRIK4PD4S","created_at":"2026-07-05T00:36:30.462939+00:00"},{"alias_kind":"pith_short_16","alias_value":"4GURRIK4PD4SOIF4","created_at":"2026-07-05T00:36:30.462939+00:00"},{"alias_kind":"pith_short_8","alias_value":"4GURRIK4","created_at":"2026-07-05T00:36:30.462939+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.28718","citing_title":"Formation of bound composite vortices of a singly-quantized $^1$S$_0$ vortex and half-quantized $^3$P$_2$ vortices in the $^1$S$_0$-$^3$P$_2$ coexisting phase in neutron stars","ref_index":60,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4GURRIK4PD4SOIF45E42HFR47F","json":"https://pith.science/pith/4GURRIK4PD4SOIF45E42HFR47F.json","graph_json":"https://pith.science/api/pith-number/4GURRIK4PD4SOIF45E42HFR47F/graph.json","events_json":"https://pith.science/api/pith-number/4GURRIK4PD4SOIF45E42HFR47F/events.json","paper":"https://pith.science/paper/4GURRIK4"},"agent_actions":{"view_html":"https://pith.science/pith/4GURRIK4PD4SOIF45E42HFR47F","download_json":"https://pith.science/pith/4GURRIK4PD4SOIF45E42HFR47F.json","view_paper":"https://pith.science/paper/4GURRIK4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1907.12843&json=true","fetch_graph":"https://pith.science/api/pith-number/4GURRIK4PD4SOIF45E42HFR47F/graph.json","fetch_events":"https://pith.science/api/pith-number/4GURRIK4PD4SOIF45E42HFR47F/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4GURRIK4PD4SOIF45E42HFR47F/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4GURRIK4PD4SOIF45E42HFR47F/action/storage_attestation","attest_author":"https://pith.science/pith/4GURRIK4PD4SOIF45E42HFR47F/action/author_attestation","sign_citation":"https://pith.science/pith/4GURRIK4PD4SOIF45E42HFR47F/action/citation_signature","submit_replication":"https://pith.science/pith/4GURRIK4PD4SOIF45E42HFR47F/action/replication_record"}},"created_at":"2026-07-05T00:36:30.462939+00:00","updated_at":"2026-07-05T00:36:30.462939+00:00"}