{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:IDE5DGSICRKEF7UWFGRNG4RP7D","short_pith_number":"pith:IDE5DGSI","schema_version":"1.0","canonical_sha256":"40c9d19a48145442fe9629a2d3722ff8ce1c17784f04421e2953e94370417824","source":{"kind":"arxiv","id":"1012.0345","version":1},"attestation_state":"computed","paper":{"title":"Dissipative processes in superfluid neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"Cristina Manuel, Giuseppe Colucci, Massimo Mannarelli","submitted_at":"2010-12-01T23:01:35Z","abstract_excerpt":"We present some results about a novel damping mechanism of r-mode oscillations in neutron stars due to processes that change the number of protons, neutrons and electrons. Deviations from equilibrium of the number densities of the various species lead to the appearance in the Euler equations of the system of a dissipative mechanism, the so-called rocket effect. The evolution of the r-mode oscillations of a rotating neutron star are influenced by the rocket effect and we present estimates of the corresponding damping timescales. In the description of the system we employ a two-fluid model, with"},"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":"1012.0345","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-12-01T23:01:35Z","cross_cats_sorted":["hep-ph","nucl-th"],"title_canon_sha256":"73ed64bcffb43398bf5e0519e191280e7c62a54d37ff4f8b7aa6025ea3078027","abstract_canon_sha256":"1df2044e49a028a8c28dee964dd4655c96b087dc7773ef49705b2e0c2bc0e6a2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:04:36.181338Z","signature_b64":"uhLH08V8vHJrEI3ZTiAZnqu6zCt8HNyhTEJwNB0T75hhK093dYkEZj/fmRidm9q1Ll+KFRtbYifEqlmbHBUSDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"40c9d19a48145442fe9629a2d3722ff8ce1c17784f04421e2953e94370417824","last_reissued_at":"2026-05-18T02:04:36.180843Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:04:36.180843Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dissipative processes in superfluid neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"Cristina Manuel, Giuseppe Colucci, Massimo Mannarelli","submitted_at":"2010-12-01T23:01:35Z","abstract_excerpt":"We present some results about a novel damping mechanism of r-mode oscillations in neutron stars due to processes that change the number of protons, neutrons and electrons. Deviations from equilibrium of the number densities of the various species lead to the appearance in the Euler equations of the system of a dissipative mechanism, the so-called rocket effect. The evolution of the r-mode oscillations of a rotating neutron star are influenced by the rocket effect and we present estimates of the corresponding damping timescales. In the description of the system we employ a two-fluid model, with"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1012.0345","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":"1012.0345","created_at":"2026-05-18T02:04:36.180915+00:00"},{"alias_kind":"arxiv_version","alias_value":"1012.0345v1","created_at":"2026-05-18T02:04:36.180915+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1012.0345","created_at":"2026-05-18T02:04:36.180915+00:00"},{"alias_kind":"pith_short_12","alias_value":"IDE5DGSICRKE","created_at":"2026-05-18T12:26:09.077623+00:00"},{"alias_kind":"pith_short_16","alias_value":"IDE5DGSICRKEF7UW","created_at":"2026-05-18T12:26:09.077623+00:00"},{"alias_kind":"pith_short_8","alias_value":"IDE5DGSI","created_at":"2026-05-18T12:26:09.077623+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/IDE5DGSICRKEF7UWFGRNG4RP7D","json":"https://pith.science/pith/IDE5DGSICRKEF7UWFGRNG4RP7D.json","graph_json":"https://pith.science/api/pith-number/IDE5DGSICRKEF7UWFGRNG4RP7D/graph.json","events_json":"https://pith.science/api/pith-number/IDE5DGSICRKEF7UWFGRNG4RP7D/events.json","paper":"https://pith.science/paper/IDE5DGSI"},"agent_actions":{"view_html":"https://pith.science/pith/IDE5DGSICRKEF7UWFGRNG4RP7D","download_json":"https://pith.science/pith/IDE5DGSICRKEF7UWFGRNG4RP7D.json","view_paper":"https://pith.science/paper/IDE5DGSI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1012.0345&json=true","fetch_graph":"https://pith.science/api/pith-number/IDE5DGSICRKEF7UWFGRNG4RP7D/graph.json","fetch_events":"https://pith.science/api/pith-number/IDE5DGSICRKEF7UWFGRNG4RP7D/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IDE5DGSICRKEF7UWFGRNG4RP7D/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IDE5DGSICRKEF7UWFGRNG4RP7D/action/storage_attestation","attest_author":"https://pith.science/pith/IDE5DGSICRKEF7UWFGRNG4RP7D/action/author_attestation","sign_citation":"https://pith.science/pith/IDE5DGSICRKEF7UWFGRNG4RP7D/action/citation_signature","submit_replication":"https://pith.science/pith/IDE5DGSICRKEF7UWFGRNG4RP7D/action/replication_record"}},"created_at":"2026-05-18T02:04:36.180915+00:00","updated_at":"2026-05-18T02:04:36.180915+00:00"}