{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:D33OHUX4HLTWVGSOYVUGJAAGTP","short_pith_number":"pith:D33OHUX4","schema_version":"1.0","canonical_sha256":"1ef6e3d2fc3ae76a9a4ec5686480069bd101735a3918b60138aee9573af38516","source":{"kind":"arxiv","id":"1707.05203","version":1},"attestation_state":"computed","paper":{"title":"Anderson-Bogoliubov phonon in inner crust of neutron stars: Dipole excitation in spherical Wigner-Seitz cell","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"Masayuki Matsuo, Tsunenori Inakura","submitted_at":"2017-07-17T15:05:48Z","abstract_excerpt":"Background: The Anderson-Bogoliubov (AB) phonon, called also the superfluid phonon, has attracted attentions since it may influence the thermal conductivity and other properties of inner crust of neutron stars. However, there are limited number of microscopic studies of the AB phonon where the presence of clusters is explicitly taken into account.\\\\ Purpose: We intend to clarify how the presence of clusters affects the AB phonon in order to obtain microscopic information relevant to the coupling between the AB phonon and the lattice phonon. \\\\ Methods: The Hartree-Fock-Bogoliubov model and the"},"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":"1707.05203","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2017-07-17T15:05:48Z","cross_cats_sorted":[],"title_canon_sha256":"fdc272ca6da8f5d8be9bba9c9c88b67f6016e976a1485fdf5204c01b7591fe30","abstract_canon_sha256":"7725871089e98ff801f5f9a29a6d504941fc942d63907c453b55ba0db686e177"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:35:58.305366Z","signature_b64":"jDVT8Ocg0a4QvTPpot/sMn5kilkbgzcJuaBbppEMDGBFw5F8ivCgPHX+b8J58/lYIGlbn1O3hBd8uu11SiUNAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1ef6e3d2fc3ae76a9a4ec5686480069bd101735a3918b60138aee9573af38516","last_reissued_at":"2026-05-18T00:35:58.304761Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:35:58.304761Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Anderson-Bogoliubov phonon in inner crust of neutron stars: Dipole excitation in spherical Wigner-Seitz cell","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"nucl-th","authors_text":"Masayuki Matsuo, Tsunenori Inakura","submitted_at":"2017-07-17T15:05:48Z","abstract_excerpt":"Background: The Anderson-Bogoliubov (AB) phonon, called also the superfluid phonon, has attracted attentions since it may influence the thermal conductivity and other properties of inner crust of neutron stars. However, there are limited number of microscopic studies of the AB phonon where the presence of clusters is explicitly taken into account.\\\\ Purpose: We intend to clarify how the presence of clusters affects the AB phonon in order to obtain microscopic information relevant to the coupling between the AB phonon and the lattice phonon. \\\\ Methods: The Hartree-Fock-Bogoliubov model and the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1707.05203","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":"1707.05203","created_at":"2026-05-18T00:35:58.304832+00:00"},{"alias_kind":"arxiv_version","alias_value":"1707.05203v1","created_at":"2026-05-18T00:35:58.304832+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1707.05203","created_at":"2026-05-18T00:35:58.304832+00:00"},{"alias_kind":"pith_short_12","alias_value":"D33OHUX4HLTW","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_16","alias_value":"D33OHUX4HLTWVGSO","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_8","alias_value":"D33OHUX4","created_at":"2026-05-18T12:31:10.602751+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.20725","citing_title":"Interaction between nuclear clusters and superfluid phonons in the neutron-star inner crust","ref_index":22,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/D33OHUX4HLTWVGSOYVUGJAAGTP","json":"https://pith.science/pith/D33OHUX4HLTWVGSOYVUGJAAGTP.json","graph_json":"https://pith.science/api/pith-number/D33OHUX4HLTWVGSOYVUGJAAGTP/graph.json","events_json":"https://pith.science/api/pith-number/D33OHUX4HLTWVGSOYVUGJAAGTP/events.json","paper":"https://pith.science/paper/D33OHUX4"},"agent_actions":{"view_html":"https://pith.science/pith/D33OHUX4HLTWVGSOYVUGJAAGTP","download_json":"https://pith.science/pith/D33OHUX4HLTWVGSOYVUGJAAGTP.json","view_paper":"https://pith.science/paper/D33OHUX4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1707.05203&json=true","fetch_graph":"https://pith.science/api/pith-number/D33OHUX4HLTWVGSOYVUGJAAGTP/graph.json","fetch_events":"https://pith.science/api/pith-number/D33OHUX4HLTWVGSOYVUGJAAGTP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/D33OHUX4HLTWVGSOYVUGJAAGTP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/D33OHUX4HLTWVGSOYVUGJAAGTP/action/storage_attestation","attest_author":"https://pith.science/pith/D33OHUX4HLTWVGSOYVUGJAAGTP/action/author_attestation","sign_citation":"https://pith.science/pith/D33OHUX4HLTWVGSOYVUGJAAGTP/action/citation_signature","submit_replication":"https://pith.science/pith/D33OHUX4HLTWVGSOYVUGJAAGTP/action/replication_record"}},"created_at":"2026-05-18T00:35:58.304832+00:00","updated_at":"2026-05-18T00:35:58.304832+00:00"}