{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:E2S566FWIVASTWVIHHSBMBJXX2","short_pith_number":"pith:E2S566FW","canonical_record":{"source":{"id":"1610.07929","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2016-10-22T07:52:29Z","cross_cats_sorted":["astro-ph.HE","astro-ph.SR"],"title_canon_sha256":"821e742d3066e025ddc8767cb3d52293d5d38e882c0830088684b975f5d9a3cb","abstract_canon_sha256":"126a822b25637433092c7532e72314d31ff32e881ae47cd4b4462a76151b28a2"},"schema_version":"1.0"},"canonical_sha256":"26a5df78b6454129daa839e4160537be8bf6bfa7b617f93929f0782a58de1d65","source":{"kind":"arxiv","id":"1610.07929","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1610.07929","created_at":"2026-05-18T00:43:30Z"},{"alias_kind":"arxiv_version","alias_value":"1610.07929v1","created_at":"2026-05-18T00:43:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.07929","created_at":"2026-05-18T00:43:30Z"},{"alias_kind":"pith_short_12","alias_value":"E2S566FWIVAS","created_at":"2026-05-18T12:30:12Z"},{"alias_kind":"pith_short_16","alias_value":"E2S566FWIVASTWVI","created_at":"2026-05-18T12:30:12Z"},{"alias_kind":"pith_short_8","alias_value":"E2S566FW","created_at":"2026-05-18T12:30:12Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:E2S566FWIVASTWVIHHSBMBJXX2","target":"record","payload":{"canonical_record":{"source":{"id":"1610.07929","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2016-10-22T07:52:29Z","cross_cats_sorted":["astro-ph.HE","astro-ph.SR"],"title_canon_sha256":"821e742d3066e025ddc8767cb3d52293d5d38e882c0830088684b975f5d9a3cb","abstract_canon_sha256":"126a822b25637433092c7532e72314d31ff32e881ae47cd4b4462a76151b28a2"},"schema_version":"1.0"},"canonical_sha256":"26a5df78b6454129daa839e4160537be8bf6bfa7b617f93929f0782a58de1d65","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:43:30.171706Z","signature_b64":"pNnYF6GryP465175QlboVcZnttXabxj5aKW1A9TUiU+d43WI20hrUE45sZFT7tsduezcA894SAdifn+Ke1RVBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"26a5df78b6454129daa839e4160537be8bf6bfa7b617f93929f0782a58de1d65","last_reissued_at":"2026-05-18T00:43:30.171022Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:43:30.171022Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1610.07929","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:43:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"fheLvP1BbAxqdORcYkxlUkCjqQaJnyAa/4yXcUdqcFDOByBXpxU0SblLCkMeZ4VgXwhx3OJuF30pK4JdW97TBA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-29T18:13:51.872968Z"},"content_sha256":"3e2c9e9ce188223e0d5c9d7c576559a3dfc1f21312e0eb828d143d70136f41f4","schema_version":"1.0","event_id":"sha256:3e2c9e9ce188223e0d5c9d7c576559a3dfc1f21312e0eb828d143d70136f41f4"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:E2S566FWIVASTWVIHHSBMBJXX2","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Impact of new data for neutron-rich heavy nuclei on theoretical models for $r$-process nucleosynthesis","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","astro-ph.SR"],"primary_cat":"nucl-th","authors_text":"Grant J. Mathews, Toshitaka Kajino","submitted_at":"2016-10-22T07:52:29Z","abstract_excerpt":"Current models for the $r$ process are summarized with an emphasis on the key constraints from both nuclear physics measurements and astronomical observations. In particular, we analyze the importance of nuclear physics input such as beta-decay rates; nuclear masses; neutron-capture cross sections; beta-delayed neutron emission; probability of spontaneous fission, beta- and neutron-induced fission, fission fragment mass distributions; neutrino-induced reaction cross sections, etc. We highlight the effects on models for $r$-process nucleosynthesis of newly measured $\\beta$-decay half-lives, mas"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.07929","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T00:43:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"gUQVFjoEMeyw3jboCDq5/GHAIQlmRSiLG2dJQJHDOmLlx+g43f6Gl7Q6Ro7lLXlvuQka1mUrKYFWjg8plhwhCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-29T18:13:51.873324Z"},"content_sha256":"26e1b588e5d61c4715fc1e2023ec77a092915be0589c5d26109f42a68aff8684","schema_version":"1.0","event_id":"sha256:26e1b588e5d61c4715fc1e2023ec77a092915be0589c5d26109f42a68aff8684"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/E2S566FWIVASTWVIHHSBMBJXX2/bundle.json","state_url":"https://pith.science/pith/E2S566FWIVASTWVIHHSBMBJXX2/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/E2S566FWIVASTWVIHHSBMBJXX2/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":"2026-06-29T18:13:51Z","links":{"resolver":"https://pith.science/pith/E2S566FWIVASTWVIHHSBMBJXX2","bundle":"https://pith.science/pith/E2S566FWIVASTWVIHHSBMBJXX2/bundle.json","state":"https://pith.science/pith/E2S566FWIVASTWVIHHSBMBJXX2/state.json","well_known_bundle":"https://pith.science/.well-known/pith/E2S566FWIVASTWVIHHSBMBJXX2/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:E2S566FWIVASTWVIHHSBMBJXX2","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":"126a822b25637433092c7532e72314d31ff32e881ae47cd4b4462a76151b28a2","cross_cats_sorted":["astro-ph.HE","astro-ph.SR"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2016-10-22T07:52:29Z","title_canon_sha256":"821e742d3066e025ddc8767cb3d52293d5d38e882c0830088684b975f5d9a3cb"},"schema_version":"1.0","source":{"id":"1610.07929","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1610.07929","created_at":"2026-05-18T00:43:30Z"},{"alias_kind":"arxiv_version","alias_value":"1610.07929v1","created_at":"2026-05-18T00:43:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1610.07929","created_at":"2026-05-18T00:43:30Z"},{"alias_kind":"pith_short_12","alias_value":"E2S566FWIVAS","created_at":"2026-05-18T12:30:12Z"},{"alias_kind":"pith_short_16","alias_value":"E2S566FWIVASTWVI","created_at":"2026-05-18T12:30:12Z"},{"alias_kind":"pith_short_8","alias_value":"E2S566FW","created_at":"2026-05-18T12:30:12Z"}],"graph_snapshots":[{"event_id":"sha256:26e1b588e5d61c4715fc1e2023ec77a092915be0589c5d26109f42a68aff8684","target":"graph","created_at":"2026-05-18T00:43:30Z","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":"Current models for the $r$ process are summarized with an emphasis on the key constraints from both nuclear physics measurements and astronomical observations. In particular, we analyze the importance of nuclear physics input such as beta-decay rates; nuclear masses; neutron-capture cross sections; beta-delayed neutron emission; probability of spontaneous fission, beta- and neutron-induced fission, fission fragment mass distributions; neutrino-induced reaction cross sections, etc. We highlight the effects on models for $r$-process nucleosynthesis of newly measured $\\beta$-decay half-lives, mas","authors_text":"Grant J. Mathews, Toshitaka Kajino","cross_cats":["astro-ph.HE","astro-ph.SR"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2016-10-22T07:52:29Z","title":"Impact of new data for neutron-rich heavy nuclei on theoretical models for $r$-process nucleosynthesis"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1610.07929","kind":"arxiv","version":1},"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":"sha256:3e2c9e9ce188223e0d5c9d7c576559a3dfc1f21312e0eb828d143d70136f41f4","target":"record","created_at":"2026-05-18T00:43:30Z","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":"126a822b25637433092c7532e72314d31ff32e881ae47cd4b4462a76151b28a2","cross_cats_sorted":["astro-ph.HE","astro-ph.SR"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"nucl-th","submitted_at":"2016-10-22T07:52:29Z","title_canon_sha256":"821e742d3066e025ddc8767cb3d52293d5d38e882c0830088684b975f5d9a3cb"},"schema_version":"1.0","source":{"id":"1610.07929","kind":"arxiv","version":1}},"canonical_sha256":"26a5df78b6454129daa839e4160537be8bf6bfa7b617f93929f0782a58de1d65","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"26a5df78b6454129daa839e4160537be8bf6bfa7b617f93929f0782a58de1d65","first_computed_at":"2026-05-18T00:43:30.171022Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:43:30.171022Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"pNnYF6GryP465175QlboVcZnttXabxj5aKW1A9TUiU+d43WI20hrUE45sZFT7tsduezcA894SAdifn+Ke1RVBg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:43:30.171706Z","signed_message":"canonical_sha256_bytes"},"source_id":"1610.07929","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:3e2c9e9ce188223e0d5c9d7c576559a3dfc1f21312e0eb828d143d70136f41f4","sha256:26e1b588e5d61c4715fc1e2023ec77a092915be0589c5d26109f42a68aff8684"],"state_sha256":"8b6f18a1ee4cd2c807b4f3e4db477ab60f566891ad502589b3ee8511aaa7862f"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"dmoisI6Mv6o2h/pdvWmSNwC8Fgou+c0t7qPln0F25wWZzIlRgTgrTke2iPREP8yjiBXdWCNhzPFzopR4VBeIDw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-29T18:13:51.875260Z","bundle_sha256":"60bebecbfb3d97c1a51b0c7b27777fdff4f877b5e3a9a263784e448334aebb28"}}