{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2016:VASZQE4HXLBDCEUX632YTVHOKA","short_pith_number":"pith:VASZQE4H","canonical_record":{"source":{"id":"1612.04760","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2016-12-14T18:16:58Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"14b3e466fbb608437a605ac255748c0e241c1f5b689b400b1f15ea2c119a022b","abstract_canon_sha256":"a6a36cf9e3ff5514e7ce461c6caca85f1ed3c9f0c82b7b42ecbcc98843be2b67"},"schema_version":"1.0"},"canonical_sha256":"a825981387bac2311297f6f589d4ee5016a24c78bde08ff6fc0efaffc96d977d","source":{"kind":"arxiv","id":"1612.04760","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1612.04760","created_at":"2026-05-18T00:41:58Z"},{"alias_kind":"arxiv_version","alias_value":"1612.04760v2","created_at":"2026-05-18T00:41:58Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.04760","created_at":"2026-05-18T00:41:58Z"},{"alias_kind":"pith_short_12","alias_value":"VASZQE4HXLBD","created_at":"2026-05-18T12:30:48Z"},{"alias_kind":"pith_short_16","alias_value":"VASZQE4HXLBDCEUX","created_at":"2026-05-18T12:30:48Z"},{"alias_kind":"pith_short_8","alias_value":"VASZQE4H","created_at":"2026-05-18T12:30:48Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2016:VASZQE4HXLBDCEUX632YTVHOKA","target":"record","payload":{"canonical_record":{"source":{"id":"1612.04760","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2016-12-14T18:16:58Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"14b3e466fbb608437a605ac255748c0e241c1f5b689b400b1f15ea2c119a022b","abstract_canon_sha256":"a6a36cf9e3ff5514e7ce461c6caca85f1ed3c9f0c82b7b42ecbcc98843be2b67"},"schema_version":"1.0"},"canonical_sha256":"a825981387bac2311297f6f589d4ee5016a24c78bde08ff6fc0efaffc96d977d","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:41:58.016917Z","signature_b64":"OzBcdJz1ubtHX2yFDvomtgSEI9huWFegj5pKLs8eieWXNUYJgegkgEQZ0SdfkUatLIgnsie9dPfayv56T6tjBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a825981387bac2311297f6f589d4ee5016a24c78bde08ff6fc0efaffc96d977d","last_reissued_at":"2026-05-18T00:41:58.016389Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:41:58.016389Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1612.04760","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":"2026-05-18T00:41:58Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"NOacfsMDKRzvUSnaQXlIyi2rlm9X/WQzuhYim+uCZpq6O29Xo3rcunyIxZr1jBi9tJ2ESyX7jj1DowMliAC3Bg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T15:14:50.594557Z"},"content_sha256":"74d98f5f1bcb3582aaf735b1c7657fd7be5be17b4075b90b03d0a6af49eb03b5","schema_version":"1.0","event_id":"sha256:74d98f5f1bcb3582aaf735b1c7657fd7be5be17b4075b90b03d0a6af49eb03b5"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2016:VASZQE4HXLBDCEUX632YTVHOKA","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Astrophysical and laboratory plasmas: HF properties under extreme conditions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"physics.plasm-ph","authors_text":"A. A. Mihajlov, D. Jevremovic, Lj. M. Ignjatovic, M. S. Dimitrijevic, N. M. Sakan, V. A. Sreckovic, V. Vujcic","submitted_at":"2016-12-14T18:16:58Z","abstract_excerpt":"The values of electrical conductivity of plasma of stars with a magnetic field or moving in the magnetic field of the other component in a binary system could be of significant interest, since they are useful for the study of thermal evolution of such objects, cooling, nuclear burning of accreted matter, and the investigation of their magnetic fields. So, on the basis of numerically calculated values for the dense plasma conductivity in an external HF electric field, we determine the HF characteristics of astrophysical plasmas under extreme conditions. The examined range of frequencies covers "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.04760","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":"2026-05-18T00:41:58Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"wv3ETFnVPxjuvAfCKI2UB42EYKz99i9bkCodzWj3N/hsmBSye8BZFN5Ddd97edco+qAXEF+uYKSY4nxGebB3DA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T15:14:50.594901Z"},"content_sha256":"aaded18984efe2df7e9c90971593db322d214ed7e2bb714a4cb47e9f6ae2800a","schema_version":"1.0","event_id":"sha256:aaded18984efe2df7e9c90971593db322d214ed7e2bb714a4cb47e9f6ae2800a"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/VASZQE4HXLBDCEUX632YTVHOKA/bundle.json","state_url":"https://pith.science/pith/VASZQE4HXLBDCEUX632YTVHOKA/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/VASZQE4HXLBDCEUX632YTVHOKA/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":"2026-06-01T15:14:50Z","links":{"resolver":"https://pith.science/pith/VASZQE4HXLBDCEUX632YTVHOKA","bundle":"https://pith.science/pith/VASZQE4HXLBDCEUX632YTVHOKA/bundle.json","state":"https://pith.science/pith/VASZQE4HXLBDCEUX632YTVHOKA/state.json","well_known_bundle":"https://pith.science/.well-known/pith/VASZQE4HXLBDCEUX632YTVHOKA/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2016:VASZQE4HXLBDCEUX632YTVHOKA","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":"a6a36cf9e3ff5514e7ce461c6caca85f1ed3c9f0c82b7b42ecbcc98843be2b67","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2016-12-14T18:16:58Z","title_canon_sha256":"14b3e466fbb608437a605ac255748c0e241c1f5b689b400b1f15ea2c119a022b"},"schema_version":"1.0","source":{"id":"1612.04760","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1612.04760","created_at":"2026-05-18T00:41:58Z"},{"alias_kind":"arxiv_version","alias_value":"1612.04760v2","created_at":"2026-05-18T00:41:58Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1612.04760","created_at":"2026-05-18T00:41:58Z"},{"alias_kind":"pith_short_12","alias_value":"VASZQE4HXLBD","created_at":"2026-05-18T12:30:48Z"},{"alias_kind":"pith_short_16","alias_value":"VASZQE4HXLBDCEUX","created_at":"2026-05-18T12:30:48Z"},{"alias_kind":"pith_short_8","alias_value":"VASZQE4H","created_at":"2026-05-18T12:30:48Z"}],"graph_snapshots":[{"event_id":"sha256:aaded18984efe2df7e9c90971593db322d214ed7e2bb714a4cb47e9f6ae2800a","target":"graph","created_at":"2026-05-18T00:41:58Z","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":"The values of electrical conductivity of plasma of stars with a magnetic field or moving in the magnetic field of the other component in a binary system could be of significant interest, since they are useful for the study of thermal evolution of such objects, cooling, nuclear burning of accreted matter, and the investigation of their magnetic fields. So, on the basis of numerically calculated values for the dense plasma conductivity in an external HF electric field, we determine the HF characteristics of astrophysical plasmas under extreme conditions. The examined range of frequencies covers ","authors_text":"A. A. Mihajlov, D. Jevremovic, Lj. M. Ignjatovic, M. S. Dimitrijevic, N. M. Sakan, V. A. Sreckovic, V. Vujcic","cross_cats":["astro-ph.HE"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2016-12-14T18:16:58Z","title":"Astrophysical and laboratory plasmas: HF properties under extreme conditions"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.04760","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":"sha256:74d98f5f1bcb3582aaf735b1c7657fd7be5be17b4075b90b03d0a6af49eb03b5","target":"record","created_at":"2026-05-18T00:41:58Z","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":"a6a36cf9e3ff5514e7ce461c6caca85f1ed3c9f0c82b7b42ecbcc98843be2b67","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2016-12-14T18:16:58Z","title_canon_sha256":"14b3e466fbb608437a605ac255748c0e241c1f5b689b400b1f15ea2c119a022b"},"schema_version":"1.0","source":{"id":"1612.04760","kind":"arxiv","version":2}},"canonical_sha256":"a825981387bac2311297f6f589d4ee5016a24c78bde08ff6fc0efaffc96d977d","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"a825981387bac2311297f6f589d4ee5016a24c78bde08ff6fc0efaffc96d977d","first_computed_at":"2026-05-18T00:41:58.016389Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:41:58.016389Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"OzBcdJz1ubtHX2yFDvomtgSEI9huWFegj5pKLs8eieWXNUYJgegkgEQZ0SdfkUatLIgnsie9dPfayv56T6tjBQ==","signature_status":"signed_v1","signed_at":"2026-05-18T00:41:58.016917Z","signed_message":"canonical_sha256_bytes"},"source_id":"1612.04760","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:74d98f5f1bcb3582aaf735b1c7657fd7be5be17b4075b90b03d0a6af49eb03b5","sha256:aaded18984efe2df7e9c90971593db322d214ed7e2bb714a4cb47e9f6ae2800a"],"state_sha256":"672853fb6a4fa370164ba01896042b43061969a4999069c690360d6576ee1300"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"igcIuZ3gl0kvM3hhTtZvUZkir34a6zopO49+LziOLB48DdDBLSQlm+O4TWvFuiJA+19odSn9k/AFXaFRsMbPAA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-01T15:14:50.596744Z","bundle_sha256":"68a87784f006f1067c6ac3547fd8ae06019b3cb9b6a17f36d59f4339d07cf6cf"}}