{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:J2JKHK5FQ6B6Q4HXHNKV5BACE3","short_pith_number":"pith:J2JKHK5F","schema_version":"1.0","canonical_sha256":"4e92a3aba58783e870f73b555e840226e2bebc159ab2fdd6d46de2a19a6d7e21","source":{"kind":"arxiv","id":"1110.4650","version":3},"attestation_state":"computed","paper":{"title":"Shear modulus of the hadron-quark mixed phase","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","nucl-th"],"primary_cat":"astro-ph.SR","authors_text":"Benjamin J. Owen, Nathan K. Johnson-McDaniel","submitted_at":"2011-10-20T21:16:33Z","abstract_excerpt":"Robust arguments predict that a hadron-quark mixed phase may exist in the cores of some \"neutron\" stars. Such a phase forms a crystalline lattice with a shear modulus higher than that of the crust due to the high density and charge separation, even allowing for the effects of charge screening. This may lead to strong continuous gravitational-wave emission from rapidly rotating neutron stars and gravitational-wave bursts associated with magnetar flares and pulsar glitches. We present the first detailed calculation of the shear modulus of the mixed phase. We describe the quark phase using the ba"},"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":"1110.4650","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.SR","submitted_at":"2011-10-20T21:16:33Z","cross_cats_sorted":["hep-ph","nucl-th"],"title_canon_sha256":"43ae2327a49e41a2607dc5f6f7ac9f6322d6298f42bdcb64f2e63278de2e798a","abstract_canon_sha256":"ad48a5c15baca89b3ad673cc5658bb48e9f2f3f9deccb2bbe1bf3e6c67b4c6bd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:20:57.054488Z","signature_b64":"ob+N/afVN+Pdio7tKoUmuADs9pyp+2/PlnDFqZ7/Rwpp2P7BQ+Jm18AzsUmOt5myq1CKf/p3nu1WpZOC9MKnDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4e92a3aba58783e870f73b555e840226e2bebc159ab2fdd6d46de2a19a6d7e21","last_reissued_at":"2026-05-18T03:20:57.053780Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:20:57.053780Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Shear modulus of the hadron-quark mixed phase","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","nucl-th"],"primary_cat":"astro-ph.SR","authors_text":"Benjamin J. Owen, Nathan K. Johnson-McDaniel","submitted_at":"2011-10-20T21:16:33Z","abstract_excerpt":"Robust arguments predict that a hadron-quark mixed phase may exist in the cores of some \"neutron\" stars. Such a phase forms a crystalline lattice with a shear modulus higher than that of the crust due to the high density and charge separation, even allowing for the effects of charge screening. This may lead to strong continuous gravitational-wave emission from rapidly rotating neutron stars and gravitational-wave bursts associated with magnetar flares and pulsar glitches. We present the first detailed calculation of the shear modulus of the mixed phase. We describe the quark phase using the ba"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1110.4650","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":""},"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":"1110.4650","created_at":"2026-05-18T03:20:57.053886+00:00"},{"alias_kind":"arxiv_version","alias_value":"1110.4650v3","created_at":"2026-05-18T03:20:57.053886+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1110.4650","created_at":"2026-05-18T03:20:57.053886+00:00"},{"alias_kind":"pith_short_12","alias_value":"J2JKHK5FQ6B6","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_16","alias_value":"J2JKHK5FQ6B6Q4HX","created_at":"2026-05-18T12:26:32.869790+00:00"},{"alias_kind":"pith_short_8","alias_value":"J2JKHK5F","created_at":"2026-05-18T12:26:32.869790+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/J2JKHK5FQ6B6Q4HXHNKV5BACE3","json":"https://pith.science/pith/J2JKHK5FQ6B6Q4HXHNKV5BACE3.json","graph_json":"https://pith.science/api/pith-number/J2JKHK5FQ6B6Q4HXHNKV5BACE3/graph.json","events_json":"https://pith.science/api/pith-number/J2JKHK5FQ6B6Q4HXHNKV5BACE3/events.json","paper":"https://pith.science/paper/J2JKHK5F"},"agent_actions":{"view_html":"https://pith.science/pith/J2JKHK5FQ6B6Q4HXHNKV5BACE3","download_json":"https://pith.science/pith/J2JKHK5FQ6B6Q4HXHNKV5BACE3.json","view_paper":"https://pith.science/paper/J2JKHK5F","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1110.4650&json=true","fetch_graph":"https://pith.science/api/pith-number/J2JKHK5FQ6B6Q4HXHNKV5BACE3/graph.json","fetch_events":"https://pith.science/api/pith-number/J2JKHK5FQ6B6Q4HXHNKV5BACE3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/J2JKHK5FQ6B6Q4HXHNKV5BACE3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/J2JKHK5FQ6B6Q4HXHNKV5BACE3/action/storage_attestation","attest_author":"https://pith.science/pith/J2JKHK5FQ6B6Q4HXHNKV5BACE3/action/author_attestation","sign_citation":"https://pith.science/pith/J2JKHK5FQ6B6Q4HXHNKV5BACE3/action/citation_signature","submit_replication":"https://pith.science/pith/J2JKHK5FQ6B6Q4HXHNKV5BACE3/action/replication_record"}},"created_at":"2026-05-18T03:20:57.053886+00:00","updated_at":"2026-05-18T03:20:57.053886+00:00"}