{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2011:MFZIIRAI4YE5ZY32IBELFE2PL2","short_pith_number":"pith:MFZIIRAI","canonical_record":{"source":{"id":"1103.4559","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2011-03-23T15:48:51Z","cross_cats_sorted":[],"title_canon_sha256":"5b9d48c8f96c71815adbf708dd474e3b1739c957af5bec738c7e5843896b01f0","abstract_canon_sha256":"162ec013bad78a5725799bd141b9bc0d80094cda57905a57eacf33514990d345"},"schema_version":"1.0"},"canonical_sha256":"6172844408e609dce37a4048b2934f5e9a439d1c7d86136d6b54af733c1fee1f","source":{"kind":"arxiv","id":"1103.4559","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1103.4559","created_at":"2026-05-18T04:16:30Z"},{"alias_kind":"arxiv_version","alias_value":"1103.4559v2","created_at":"2026-05-18T04:16:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1103.4559","created_at":"2026-05-18T04:16:30Z"},{"alias_kind":"pith_short_12","alias_value":"MFZIIRAI4YE5","created_at":"2026-05-18T12:26:34Z"},{"alias_kind":"pith_short_16","alias_value":"MFZIIRAI4YE5ZY32","created_at":"2026-05-18T12:26:34Z"},{"alias_kind":"pith_short_8","alias_value":"MFZIIRAI","created_at":"2026-05-18T12:26:34Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2011:MFZIIRAI4YE5ZY32IBELFE2PL2","target":"record","payload":{"canonical_record":{"source":{"id":"1103.4559","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2011-03-23T15:48:51Z","cross_cats_sorted":[],"title_canon_sha256":"5b9d48c8f96c71815adbf708dd474e3b1739c957af5bec738c7e5843896b01f0","abstract_canon_sha256":"162ec013bad78a5725799bd141b9bc0d80094cda57905a57eacf33514990d345"},"schema_version":"1.0"},"canonical_sha256":"6172844408e609dce37a4048b2934f5e9a439d1c7d86136d6b54af733c1fee1f","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:16:30.737119Z","signature_b64":"a8jJYJN5JYJhl5/YtNUCPe1//AmWJn50gXzHZW8TQYXmOITBbh7j5Ilmcy/39ycfhaWlPyCJAl543l0/IMZFAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6172844408e609dce37a4048b2934f5e9a439d1c7d86136d6b54af733c1fee1f","last_reissued_at":"2026-05-18T04:16:30.736728Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:16:30.736728Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1103.4559","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":"2026-05-18T04:16:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"3gmq8+VJeqpAqbQECYq6N8M6DnFQbiPqurFXeMsfsRwR60Q5QrtTp/pHYFdSndhcpoSTtj6EVuCJSX7LHxg8DA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T18:11:36.368416Z"},"content_sha256":"466dbe72ad18171b6f42960db7969059a177fceb7ffe5ec57ef3870d99388f92","schema_version":"1.0","event_id":"sha256:466dbe72ad18171b6f42960db7969059a177fceb7ffe5ec57ef3870d99388f92"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2011:MFZIIRAI4YE5ZY32IBELFE2PL2","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"One-dimensional radiation-hydrodynamic scaling studies of imploding spherical plasma liners","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.plasm-ph","authors_text":"C. S. Adams, D. S. Hanna, J. S. Davis, J. T. Cassibry, S. C. Hsu, T. J. Awe","submitted_at":"2011-03-23T15:48:51Z","abstract_excerpt":"One-dimensional radiation-hydrodynamic simulations are performed to develop insight into the scaling of stagnation pressure with initial conditions of an imploding spherical plasma shell or \"liner.\" Simulations reveal the evolution of high-Mach-number (M), annular, spherical plasma flows during convergence, stagnation, shock formation, and disassembly, and indicate that cm- and {\\mu}s-scale plasmas with peak pressures near 1 Mbar can be generated by liners with initial kinetic energy of several hundred kilo-joules. It is shown that radiation transport and thermal conduction must be included to"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1103.4559","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":"2026-05-18T04:16:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"/tRpcI8IgBSsZnEvzPW3WQdsrRPr+O4wZVWFIefcq4MHeqkajzdP/9cgBYnXgFIczKsB1LayE3gKMriucgw5DQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-31T18:11:36.369200Z"},"content_sha256":"e26fab6ea6a19a13620ce854946453aa76378c73db949e8299d8fe26f8200a57","schema_version":"1.0","event_id":"sha256:e26fab6ea6a19a13620ce854946453aa76378c73db949e8299d8fe26f8200a57"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/MFZIIRAI4YE5ZY32IBELFE2PL2/bundle.json","state_url":"https://pith.science/pith/MFZIIRAI4YE5ZY32IBELFE2PL2/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/MFZIIRAI4YE5ZY32IBELFE2PL2/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":"2026-05-31T18:11:36Z","links":{"resolver":"https://pith.science/pith/MFZIIRAI4YE5ZY32IBELFE2PL2","bundle":"https://pith.science/pith/MFZIIRAI4YE5ZY32IBELFE2PL2/bundle.json","state":"https://pith.science/pith/MFZIIRAI4YE5ZY32IBELFE2PL2/state.json","well_known_bundle":"https://pith.science/.well-known/pith/MFZIIRAI4YE5ZY32IBELFE2PL2/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2011:MFZIIRAI4YE5ZY32IBELFE2PL2","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":"162ec013bad78a5725799bd141b9bc0d80094cda57905a57eacf33514990d345","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2011-03-23T15:48:51Z","title_canon_sha256":"5b9d48c8f96c71815adbf708dd474e3b1739c957af5bec738c7e5843896b01f0"},"schema_version":"1.0","source":{"id":"1103.4559","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1103.4559","created_at":"2026-05-18T04:16:30Z"},{"alias_kind":"arxiv_version","alias_value":"1103.4559v2","created_at":"2026-05-18T04:16:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1103.4559","created_at":"2026-05-18T04:16:30Z"},{"alias_kind":"pith_short_12","alias_value":"MFZIIRAI4YE5","created_at":"2026-05-18T12:26:34Z"},{"alias_kind":"pith_short_16","alias_value":"MFZIIRAI4YE5ZY32","created_at":"2026-05-18T12:26:34Z"},{"alias_kind":"pith_short_8","alias_value":"MFZIIRAI","created_at":"2026-05-18T12:26:34Z"}],"graph_snapshots":[{"event_id":"sha256:e26fab6ea6a19a13620ce854946453aa76378c73db949e8299d8fe26f8200a57","target":"graph","created_at":"2026-05-18T04:16:30Z","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":"One-dimensional radiation-hydrodynamic simulations are performed to develop insight into the scaling of stagnation pressure with initial conditions of an imploding spherical plasma shell or \"liner.\" Simulations reveal the evolution of high-Mach-number (M), annular, spherical plasma flows during convergence, stagnation, shock formation, and disassembly, and indicate that cm- and {\\mu}s-scale plasmas with peak pressures near 1 Mbar can be generated by liners with initial kinetic energy of several hundred kilo-joules. It is shown that radiation transport and thermal conduction must be included to","authors_text":"C. S. Adams, D. S. Hanna, J. S. Davis, J. T. Cassibry, S. C. Hsu, T. J. Awe","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2011-03-23T15:48:51Z","title":"One-dimensional radiation-hydrodynamic scaling studies of imploding spherical plasma liners"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1103.4559","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":"sha256:466dbe72ad18171b6f42960db7969059a177fceb7ffe5ec57ef3870d99388f92","target":"record","created_at":"2026-05-18T04:16:30Z","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":"162ec013bad78a5725799bd141b9bc0d80094cda57905a57eacf33514990d345","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2011-03-23T15:48:51Z","title_canon_sha256":"5b9d48c8f96c71815adbf708dd474e3b1739c957af5bec738c7e5843896b01f0"},"schema_version":"1.0","source":{"id":"1103.4559","kind":"arxiv","version":2}},"canonical_sha256":"6172844408e609dce37a4048b2934f5e9a439d1c7d86136d6b54af733c1fee1f","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"6172844408e609dce37a4048b2934f5e9a439d1c7d86136d6b54af733c1fee1f","first_computed_at":"2026-05-18T04:16:30.736728Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T04:16:30.736728Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"a8jJYJN5JYJhl5/YtNUCPe1//AmWJn50gXzHZW8TQYXmOITBbh7j5Ilmcy/39ycfhaWlPyCJAl543l0/IMZFAw==","signature_status":"signed_v1","signed_at":"2026-05-18T04:16:30.737119Z","signed_message":"canonical_sha256_bytes"},"source_id":"1103.4559","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:466dbe72ad18171b6f42960db7969059a177fceb7ffe5ec57ef3870d99388f92","sha256:e26fab6ea6a19a13620ce854946453aa76378c73db949e8299d8fe26f8200a57"],"state_sha256":"2771c5481145e38f2e0f2f5a4875cd5f09ea71dbc1844590962d9e46d96e3e99"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"q33+PkLrVT5MjraY8odLOntO59XGYatqNNIeZOi1N8Du4ShKfRy9+gInzTt87vT09fH0wWigkTUbKbZFAU90AQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-31T18:11:36.373517Z","bundle_sha256":"62b7cfe79b37c75c235a70660a67d982bfa772a79b4a36bca0063d68318176ef"}}