{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:CFPFFX2ZP74IT6MSE2XVMVLJV3","short_pith_number":"pith:CFPFFX2Z","canonical_record":{"source":{"id":"1609.06362","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-09-20T21:12:44Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"401ecef6794bf0c1f5f64d8f5daef6d826393e9996d0e04c13af159f00d5280c","abstract_canon_sha256":"bb7fd5c9c02e1f303e3574020368ceabbf3a8066121c7c3be588207a4e2e7c97"},"schema_version":"1.0"},"canonical_sha256":"115e52df597ff889f99226af565569aec623f87efe7cfe09f3ec116bf550d39b","source":{"kind":"arxiv","id":"1609.06362","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1609.06362","created_at":"2026-05-18T00:55:41Z"},{"alias_kind":"arxiv_version","alias_value":"1609.06362v2","created_at":"2026-05-18T00:55:41Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1609.06362","created_at":"2026-05-18T00:55:41Z"},{"alias_kind":"pith_short_12","alias_value":"CFPFFX2ZP74I","created_at":"2026-05-18T12:30:09Z"},{"alias_kind":"pith_short_16","alias_value":"CFPFFX2ZP74IT6MS","created_at":"2026-05-18T12:30:09Z"},{"alias_kind":"pith_short_8","alias_value":"CFPFFX2Z","created_at":"2026-05-18T12:30:09Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:CFPFFX2ZP74IT6MSE2XVMVLJV3","target":"record","payload":{"canonical_record":{"source":{"id":"1609.06362","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-09-20T21:12:44Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"401ecef6794bf0c1f5f64d8f5daef6d826393e9996d0e04c13af159f00d5280c","abstract_canon_sha256":"bb7fd5c9c02e1f303e3574020368ceabbf3a8066121c7c3be588207a4e2e7c97"},"schema_version":"1.0"},"canonical_sha256":"115e52df597ff889f99226af565569aec623f87efe7cfe09f3ec116bf550d39b","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:55:41.370751Z","signature_b64":"2mj2kv0FfASlGn2Ot5Km/8jBNWNGYu4ZQm20yTulIR3qaNNLtRRhanlsopvsPToJ2wYqNjxNeyph1/uBa3DqAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"115e52df597ff889f99226af565569aec623f87efe7cfe09f3ec116bf550d39b","last_reissued_at":"2026-05-18T00:55:41.370266Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:55:41.370266Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1609.06362","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":"2026-05-18T00:55:41Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"NlAiXOTcRqc/YxQteZezfGnCpg1/xmA6zj/YLBjMySAWukWmsFHTDUVGnZFvg172WBKDqhwAa3/Qu1IQMZ9oBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T17:41:14.626414Z"},"content_sha256":"cc170e36e72f0d606ca457873501cda310d71788b33ca602289ce993e9306f19","schema_version":"1.0","event_id":"sha256:cc170e36e72f0d606ca457873501cda310d71788b33ca602289ce993e9306f19"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:CFPFFX2ZP74IT6MSE2XVMVLJV3","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Impact of the tidal p-g instability on the gravitational wave signal from coalescing binary neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Nevin N. Weinberg, Reed Essick, Salvatore Vitale","submitted_at":"2016-09-20T21:12:44Z","abstract_excerpt":"Recent studies suggest that coalescing neutron stars are subject to a fluid instability involving the nonlinear coupling of the tide to $p$-modes and $g$-modes. Its influence on the inspiral dynamics and thus the gravitational wave signal is, however, uncertain because we do not know precisely how the instability saturates. Here we construct a simple, physically motivated model of the saturation that allows us to explore the instability's impact as a function of the model parameters. We find that for plausible assumptions about the saturation, current gravitational wave detectors might miss $>"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1609.06362","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":"2026-05-18T00:55:41Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"WHEORsaKnCa/3LjIfjm6wXpy6kncBXtmZ7dog4u2UZ2GY2GMarLMKWB+ABDUkP1wxb5iUDVcONZ+s4wlkzcRCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-27T17:41:14.627102Z"},"content_sha256":"7791b682e86b95234b23478147d98fdc063b4d86ce9665b57e2987a357676770","schema_version":"1.0","event_id":"sha256:7791b682e86b95234b23478147d98fdc063b4d86ce9665b57e2987a357676770"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/CFPFFX2ZP74IT6MSE2XVMVLJV3/bundle.json","state_url":"https://pith.science/pith/CFPFFX2ZP74IT6MSE2XVMVLJV3/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/CFPFFX2ZP74IT6MSE2XVMVLJV3/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":"2026-05-27T17:41:14Z","links":{"resolver":"https://pith.science/pith/CFPFFX2ZP74IT6MSE2XVMVLJV3","bundle":"https://pith.science/pith/CFPFFX2ZP74IT6MSE2XVMVLJV3/bundle.json","state":"https://pith.science/pith/CFPFFX2ZP74IT6MSE2XVMVLJV3/state.json","well_known_bundle":"https://pith.science/.well-known/pith/CFPFFX2ZP74IT6MSE2XVMVLJV3/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:CFPFFX2ZP74IT6MSE2XVMVLJV3","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":"bb7fd5c9c02e1f303e3574020368ceabbf3a8066121c7c3be588207a4e2e7c97","cross_cats_sorted":["gr-qc"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-09-20T21:12:44Z","title_canon_sha256":"401ecef6794bf0c1f5f64d8f5daef6d826393e9996d0e04c13af159f00d5280c"},"schema_version":"1.0","source":{"id":"1609.06362","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1609.06362","created_at":"2026-05-18T00:55:41Z"},{"alias_kind":"arxiv_version","alias_value":"1609.06362v2","created_at":"2026-05-18T00:55:41Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1609.06362","created_at":"2026-05-18T00:55:41Z"},{"alias_kind":"pith_short_12","alias_value":"CFPFFX2ZP74I","created_at":"2026-05-18T12:30:09Z"},{"alias_kind":"pith_short_16","alias_value":"CFPFFX2ZP74IT6MS","created_at":"2026-05-18T12:30:09Z"},{"alias_kind":"pith_short_8","alias_value":"CFPFFX2Z","created_at":"2026-05-18T12:30:09Z"}],"graph_snapshots":[{"event_id":"sha256:7791b682e86b95234b23478147d98fdc063b4d86ce9665b57e2987a357676770","target":"graph","created_at":"2026-05-18T00:55:41Z","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":"Recent studies suggest that coalescing neutron stars are subject to a fluid instability involving the nonlinear coupling of the tide to $p$-modes and $g$-modes. Its influence on the inspiral dynamics and thus the gravitational wave signal is, however, uncertain because we do not know precisely how the instability saturates. Here we construct a simple, physically motivated model of the saturation that allows us to explore the instability's impact as a function of the model parameters. We find that for plausible assumptions about the saturation, current gravitational wave detectors might miss $>","authors_text":"Nevin N. Weinberg, Reed Essick, Salvatore Vitale","cross_cats":["gr-qc"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-09-20T21:12:44Z","title":"Impact of the tidal p-g instability on the gravitational wave signal from coalescing binary neutron stars"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1609.06362","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:cc170e36e72f0d606ca457873501cda310d71788b33ca602289ce993e9306f19","target":"record","created_at":"2026-05-18T00:55:41Z","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":"bb7fd5c9c02e1f303e3574020368ceabbf3a8066121c7c3be588207a4e2e7c97","cross_cats_sorted":["gr-qc"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2016-09-20T21:12:44Z","title_canon_sha256":"401ecef6794bf0c1f5f64d8f5daef6d826393e9996d0e04c13af159f00d5280c"},"schema_version":"1.0","source":{"id":"1609.06362","kind":"arxiv","version":2}},"canonical_sha256":"115e52df597ff889f99226af565569aec623f87efe7cfe09f3ec116bf550d39b","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"115e52df597ff889f99226af565569aec623f87efe7cfe09f3ec116bf550d39b","first_computed_at":"2026-05-18T00:55:41.370266Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:55:41.370266Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"2mj2kv0FfASlGn2Ot5Km/8jBNWNGYu4ZQm20yTulIR3qaNNLtRRhanlsopvsPToJ2wYqNjxNeyph1/uBa3DqAQ==","signature_status":"signed_v1","signed_at":"2026-05-18T00:55:41.370751Z","signed_message":"canonical_sha256_bytes"},"source_id":"1609.06362","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:cc170e36e72f0d606ca457873501cda310d71788b33ca602289ce993e9306f19","sha256:7791b682e86b95234b23478147d98fdc063b4d86ce9665b57e2987a357676770"],"state_sha256":"0f0abeaab82d55a23badb750998c81cdf75e0e8b031bff3389b77461059d4bfc"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"J8dn2zTKggaF6qxyI6bttiBqy+2UwHHNcnbyAdJ5AM0cvl6F4S/qGKTalLvdJR92sOwSWjZCuBzBfsRAIYh0Dg==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-27T17:41:14.630817Z","bundle_sha256":"db19f7bc62c27da64a6e1e4f123ca7409166cafb41937271164529ad16466299"}}