{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:UZD52S5S57G5QQPAG66KDHRTW4","short_pith_number":"pith:UZD52S5S","canonical_record":{"source":{"id":"1610.06380","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-10-20T12:35:16Z","cross_cats_sorted":["astro-ph.SR","gr-qc"],"title_canon_sha256":"7a06c85f1c64365f803dc09adfe1e06d5d10fee844a57f18931cdecd21bfb327","abstract_canon_sha256":"739598745e6059c2853b3e09459be4034bb73af6f9a825919d52eca5ab54f9d0"},"schema_version":"1.0"},"canonical_sha256":"a647dd4bb2efcdd841e037bca19e33b731212bd3cb40de96f3f2a97f16d40ce3","source":{"kind":"arxiv","id":"1610.06380","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1610.06380","created_at":"2026-05-18T00:48:05Z"},{"alias_kind":"arxiv_version","alias_value":"1610.06380v2","created_at":"2026-05-18T00:48:05Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.06380","created_at":"2026-05-18T00:48:05Z"},{"alias_kind":"pith_short_12","alias_value":"UZD52S5S57G5","created_at":"2026-05-18T12:30:46Z"},{"alias_kind":"pith_short_16","alias_value":"UZD52S5S57G5QQPA","created_at":"2026-05-18T12:30:46Z"},{"alias_kind":"pith_short_8","alias_value":"UZD52S5S","created_at":"2026-05-18T12:30:46Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:UZD52S5S57G5QQPAG66KDHRTW4","target":"record","payload":{"canonical_record":{"source":{"id":"1610.06380","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-10-20T12:35:16Z","cross_cats_sorted":["astro-ph.SR","gr-qc"],"title_canon_sha256":"7a06c85f1c64365f803dc09adfe1e06d5d10fee844a57f18931cdecd21bfb327","abstract_canon_sha256":"739598745e6059c2853b3e09459be4034bb73af6f9a825919d52eca5ab54f9d0"},"schema_version":"1.0"},"canonical_sha256":"a647dd4bb2efcdd841e037bca19e33b731212bd3cb40de96f3f2a97f16d40ce3","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:48:05.413448Z","signature_b64":"pNxrSnAEMfBw7kXlzE8sGcSs0TjZgTulqt/w4N07OV7x1HaAn5/gdhQg7zvgslJYinZoSPm2BRSsFvkbOLF5Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a647dd4bb2efcdd841e037bca19e33b731212bd3cb40de96f3f2a97f16d40ce3","last_reissued_at":"2026-05-18T00:48:05.412913Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:48:05.412913Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1610.06380","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:48:05Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"EIC62QqCUD4mZByohfcZMBCOwDiM+e7VsP9pP+h/f3N8hGvKdgCaaYUb4RkWbxpRjVNTwhkp9boWjb0xIW5bBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T10:03:14.156114Z"},"content_sha256":"94170185d3f3685248c189b5b0a06567a3098186bd1373ef03c5bd8d55eaacd2","schema_version":"1.0","event_id":"sha256:94170185d3f3685248c189b5b0a06567a3098186bd1373ef03c5bd8d55eaacd2"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:UZD52S5S57G5QQPAG66KDHRTW4","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"R-modes and neutron star recycling scenario","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.SR","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Andrey I. Chugunov, Elena M. Kantor (Ioffe Institute), Mikhail E. Gusakov","submitted_at":"2016-10-20T12:35:16Z","abstract_excerpt":"To put new constraints on the r-mode instability window, we analyse the formation of millisecond pulsars (MSPs) within the recycling scenario, making use of three sets of observations: (a) X-ray observations of neutron stars (NSs) in low-mass X-ray binaries; (b) timing of millisecond pulsars; and (c) X-ray and UV observations of MSPs. As shown in previous works, r-mode dissipation by shear viscosity is not sufficient to explain observational set (a), and enhanced r-mode dissipation at the red-shifted internal temperatures $T^\\infty\\sim 10^8$ K is required to stabilize the observed NSs. Here, w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.06380","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":""},"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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:48:05Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"RezglFI8S2/V9kkN1Th3/EGDwNXzSa1TCGtxzMxJclKArAzJbNGC9diWW38ttmSPBa1O95b9XVs9Cx8rElYxDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T10:03:14.156495Z"},"content_sha256":"54f69e409c4c95cb432351a757473e4d29964ca9b4036fe91ddb3f5804106703","schema_version":"1.0","event_id":"sha256:54f69e409c4c95cb432351a757473e4d29964ca9b4036fe91ddb3f5804106703"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/UZD52S5S57G5QQPAG66KDHRTW4/bundle.json","state_url":"https://pith.science/pith/UZD52S5S57G5QQPAG66KDHRTW4/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/UZD52S5S57G5QQPAG66KDHRTW4/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-06-04T10:03:14Z","links":{"resolver":"https://pith.science/pith/UZD52S5S57G5QQPAG66KDHRTW4","bundle":"https://pith.science/pith/UZD52S5S57G5QQPAG66KDHRTW4/bundle.json","state":"https://pith.science/pith/UZD52S5S57G5QQPAG66KDHRTW4/state.json","well_known_bundle":"https://pith.science/.well-known/pith/UZD52S5S57G5QQPAG66KDHRTW4/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:UZD52S5S57G5QQPAG66KDHRTW4","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"739598745e6059c2853b3e09459be4034bb73af6f9a825919d52eca5ab54f9d0","cross_cats_sorted":["astro-ph.SR","gr-qc"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-10-20T12:35:16Z","title_canon_sha256":"7a06c85f1c64365f803dc09adfe1e06d5d10fee844a57f18931cdecd21bfb327"},"schema_version":"1.0","source":{"id":"1610.06380","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1610.06380","created_at":"2026-05-18T00:48:05Z"},{"alias_kind":"arxiv_version","alias_value":"1610.06380v2","created_at":"2026-05-18T00:48:05Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.06380","created_at":"2026-05-18T00:48:05Z"},{"alias_kind":"pith_short_12","alias_value":"UZD52S5S57G5","created_at":"2026-05-18T12:30:46Z"},{"alias_kind":"pith_short_16","alias_value":"UZD52S5S57G5QQPA","created_at":"2026-05-18T12:30:46Z"},{"alias_kind":"pith_short_8","alias_value":"UZD52S5S","created_at":"2026-05-18T12:30:46Z"}],"graph_snapshots":[{"event_id":"sha256:54f69e409c4c95cb432351a757473e4d29964ca9b4036fe91ddb3f5804106703","target":"graph","created_at":"2026-05-18T00:48:05Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"To put new constraints on the r-mode instability window, we analyse the formation of millisecond pulsars (MSPs) within the recycling scenario, making use of three sets of observations: (a) X-ray observations of neutron stars (NSs) in low-mass X-ray binaries; (b) timing of millisecond pulsars; and (c) X-ray and UV observations of MSPs. As shown in previous works, r-mode dissipation by shear viscosity is not sufficient to explain observational set (a), and enhanced r-mode dissipation at the red-shifted internal temperatures $T^\\infty\\sim 10^8$ K is required to stabilize the observed NSs. Here, w","authors_text":"Andrey I. Chugunov, Elena M. Kantor (Ioffe Institute), Mikhail E. Gusakov","cross_cats":["astro-ph.SR","gr-qc"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-10-20T12:35:16Z","title":"R-modes and neutron star recycling scenario"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.06380","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:94170185d3f3685248c189b5b0a06567a3098186bd1373ef03c5bd8d55eaacd2","target":"record","created_at":"2026-05-18T00:48:05Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"739598745e6059c2853b3e09459be4034bb73af6f9a825919d52eca5ab54f9d0","cross_cats_sorted":["astro-ph.SR","gr-qc"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-10-20T12:35:16Z","title_canon_sha256":"7a06c85f1c64365f803dc09adfe1e06d5d10fee844a57f18931cdecd21bfb327"},"schema_version":"1.0","source":{"id":"1610.06380","kind":"arxiv","version":2}},"canonical_sha256":"a647dd4bb2efcdd841e037bca19e33b731212bd3cb40de96f3f2a97f16d40ce3","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"a647dd4bb2efcdd841e037bca19e33b731212bd3cb40de96f3f2a97f16d40ce3","first_computed_at":"2026-05-18T00:48:05.412913Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:48:05.412913Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"pNxrSnAEMfBw7kXlzE8sGcSs0TjZgTulqt/w4N07OV7x1HaAn5/gdhQg7zvgslJYinZoSPm2BRSsFvkbOLF5Cg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:48:05.413448Z","signed_message":"canonical_sha256_bytes"},"source_id":"1610.06380","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:94170185d3f3685248c189b5b0a06567a3098186bd1373ef03c5bd8d55eaacd2","sha256:54f69e409c4c95cb432351a757473e4d29964ca9b4036fe91ddb3f5804106703"],"state_sha256":"0a126cf83e7ea5e865bea966e26fafc834b55531b0c222175dd538a84f813a45"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"TCvWfop5o3PxKG+71YZH+4ln+O6ogl0CjN1pcxLX3DSO9MIRxYzDnDYtlXfn2RI4SdmAJCPXLGcjLbgVpIRuCg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-04T10:03:14.158530Z","bundle_sha256":"baa9113b3cb0162aa9a4956792229a9f4ce3876946e8b6debf616403d6bd588c"}}