{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2017:S3ES6L5EY62LCLWPNYRB27H3SR","short_pith_number":"pith:S3ES6L5E","canonical_record":{"source":{"id":"1701.08263","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2017-01-28T07:36:16Z","cross_cats_sorted":["hep-ph","nucl-th","physics.flu-dyn"],"title_canon_sha256":"9a196e48e80e47b807bdd6c2d2deb8e5d7b085582d7e8aa2e345f6cefd681cbc","abstract_canon_sha256":"9623ad5134fc7681b230df8f31ad0f2c8600694b8203ecc1626a76d387433cc8"},"schema_version":"1.0"},"canonical_sha256":"96c92f2fa4c7b4b12ecf6e221d7cfb9464a63f221ff646159d5702f6d8a88e15","source":{"kind":"arxiv","id":"1701.08263","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1701.08263","created_at":"2026-05-18T00:34:20Z"},{"alias_kind":"arxiv_version","alias_value":"1701.08263v2","created_at":"2026-05-18T00:34:20Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.08263","created_at":"2026-05-18T00:34:20Z"},{"alias_kind":"pith_short_12","alias_value":"S3ES6L5EY62L","created_at":"2026-05-18T12:31:43Z"},{"alias_kind":"pith_short_16","alias_value":"S3ES6L5EY62LCLWP","created_at":"2026-05-18T12:31:43Z"},{"alias_kind":"pith_short_8","alias_value":"S3ES6L5E","created_at":"2026-05-18T12:31:43Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2017:S3ES6L5EY62LCLWPNYRB27H3SR","target":"record","payload":{"canonical_record":{"source":{"id":"1701.08263","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2017-01-28T07:36:16Z","cross_cats_sorted":["hep-ph","nucl-th","physics.flu-dyn"],"title_canon_sha256":"9a196e48e80e47b807bdd6c2d2deb8e5d7b085582d7e8aa2e345f6cefd681cbc","abstract_canon_sha256":"9623ad5134fc7681b230df8f31ad0f2c8600694b8203ecc1626a76d387433cc8"},"schema_version":"1.0"},"canonical_sha256":"96c92f2fa4c7b4b12ecf6e221d7cfb9464a63f221ff646159d5702f6d8a88e15","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:34:20.686756Z","signature_b64":"+FK7TLbTknFqCM997sjiDkuj+04+abNPPji6UU68y65OIwB+YYOmn3mUZRb4bIiT9F3/caHAlnsQ5UqowsceAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"96c92f2fa4c7b4b12ecf6e221d7cfb9464a63f221ff646159d5702f6d8a88e15","last_reissued_at":"2026-05-18T00:34:20.686174Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:34:20.686174Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1701.08263","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":"2026-05-18T00:34:20Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"0t2SRFtU1kEv6KOBi/4NZajNjqWeoUHlB/TfrliIUQZ4wC8ep7QrZ63qacZ6bgp61RLanrNH4x/wBaVsbPtoDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T04:34:01.266914Z"},"content_sha256":"cefbb22a0e23b86d389971086524d22a0db01a91627d036a2364943c680ae5b9","schema_version":"1.0","event_id":"sha256:cefbb22a0e23b86d389971086524d22a0db01a91627d036a2364943c680ae5b9"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2017:S3ES6L5EY62LCLWPNYRB27H3SR","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"The ideal relativistic fluid limit for a medium with polarization","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","nucl-th","physics.flu-dyn"],"primary_cat":"hep-th","authors_text":"David Montenegro, Giorgio Torrieri, Leonardo Tinti","submitted_at":"2017-01-28T07:36:16Z","abstract_excerpt":"We use Lagrangian effective field theory techniques to construct the equations of motion for an ideal relativistic fluid whose constituent degrees of freedom have microscopic polarization. We discuss the meaning of such a system, and argue that it is the first term in the EFT appropriate for describing polarization observables in heavy ion collisions, such as final state particle polarization and chiral magnetic and vortaic effects. We show that this system will generally require non-dissipative dynamics at higher order in gradient than second order, leading to potential stability issues known"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.08263","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":"2026-05-18T00:34:20Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Zxu8JhXkKLU3A6AsiwYEEUwQtUfdXzmQbCT2uTes2I1SsER2ESvbysUNFK+Cb6nysYuYjdhAG6OVcsBCg8YPDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-01T04:34:01.267269Z"},"content_sha256":"ea7722df3c942eaa5a998d83b7286b3292f57becdf1d1c14e2bc24a2c2d311bd","schema_version":"1.0","event_id":"sha256:ea7722df3c942eaa5a998d83b7286b3292f57becdf1d1c14e2bc24a2c2d311bd"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/S3ES6L5EY62LCLWPNYRB27H3SR/bundle.json","state_url":"https://pith.science/pith/S3ES6L5EY62LCLWPNYRB27H3SR/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/S3ES6L5EY62LCLWPNYRB27H3SR/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":"2026-06-01T04:34:01Z","links":{"resolver":"https://pith.science/pith/S3ES6L5EY62LCLWPNYRB27H3SR","bundle":"https://pith.science/pith/S3ES6L5EY62LCLWPNYRB27H3SR/bundle.json","state":"https://pith.science/pith/S3ES6L5EY62LCLWPNYRB27H3SR/state.json","well_known_bundle":"https://pith.science/.well-known/pith/S3ES6L5EY62LCLWPNYRB27H3SR/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2017:S3ES6L5EY62LCLWPNYRB27H3SR","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":"9623ad5134fc7681b230df8f31ad0f2c8600694b8203ecc1626a76d387433cc8","cross_cats_sorted":["hep-ph","nucl-th","physics.flu-dyn"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2017-01-28T07:36:16Z","title_canon_sha256":"9a196e48e80e47b807bdd6c2d2deb8e5d7b085582d7e8aa2e345f6cefd681cbc"},"schema_version":"1.0","source":{"id":"1701.08263","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1701.08263","created_at":"2026-05-18T00:34:20Z"},{"alias_kind":"arxiv_version","alias_value":"1701.08263v2","created_at":"2026-05-18T00:34:20Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1701.08263","created_at":"2026-05-18T00:34:20Z"},{"alias_kind":"pith_short_12","alias_value":"S3ES6L5EY62L","created_at":"2026-05-18T12:31:43Z"},{"alias_kind":"pith_short_16","alias_value":"S3ES6L5EY62LCLWP","created_at":"2026-05-18T12:31:43Z"},{"alias_kind":"pith_short_8","alias_value":"S3ES6L5E","created_at":"2026-05-18T12:31:43Z"}],"graph_snapshots":[{"event_id":"sha256:ea7722df3c942eaa5a998d83b7286b3292f57becdf1d1c14e2bc24a2c2d311bd","target":"graph","created_at":"2026-05-18T00:34:20Z","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":"We use Lagrangian effective field theory techniques to construct the equations of motion for an ideal relativistic fluid whose constituent degrees of freedom have microscopic polarization. We discuss the meaning of such a system, and argue that it is the first term in the EFT appropriate for describing polarization observables in heavy ion collisions, such as final state particle polarization and chiral magnetic and vortaic effects. We show that this system will generally require non-dissipative dynamics at higher order in gradient than second order, leading to potential stability issues known","authors_text":"David Montenegro, Giorgio Torrieri, Leonardo Tinti","cross_cats":["hep-ph","nucl-th","physics.flu-dyn"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2017-01-28T07:36:16Z","title":"The ideal relativistic fluid limit for a medium with polarization"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1701.08263","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:cefbb22a0e23b86d389971086524d22a0db01a91627d036a2364943c680ae5b9","target":"record","created_at":"2026-05-18T00:34:20Z","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":"9623ad5134fc7681b230df8f31ad0f2c8600694b8203ecc1626a76d387433cc8","cross_cats_sorted":["hep-ph","nucl-th","physics.flu-dyn"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2017-01-28T07:36:16Z","title_canon_sha256":"9a196e48e80e47b807bdd6c2d2deb8e5d7b085582d7e8aa2e345f6cefd681cbc"},"schema_version":"1.0","source":{"id":"1701.08263","kind":"arxiv","version":2}},"canonical_sha256":"96c92f2fa4c7b4b12ecf6e221d7cfb9464a63f221ff646159d5702f6d8a88e15","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"96c92f2fa4c7b4b12ecf6e221d7cfb9464a63f221ff646159d5702f6d8a88e15","first_computed_at":"2026-05-18T00:34:20.686174Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T00:34:20.686174Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"+FK7TLbTknFqCM997sjiDkuj+04+abNPPji6UU68y65OIwB+YYOmn3mUZRb4bIiT9F3/caHAlnsQ5UqowsceAg==","signature_status":"signed_v1","signed_at":"2026-05-18T00:34:20.686756Z","signed_message":"canonical_sha256_bytes"},"source_id":"1701.08263","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:cefbb22a0e23b86d389971086524d22a0db01a91627d036a2364943c680ae5b9","sha256:ea7722df3c942eaa5a998d83b7286b3292f57becdf1d1c14e2bc24a2c2d311bd"],"state_sha256":"fecbb0d8a1be6e4891306fa0b149cc93fccb5f9842f53613fcfb8501a9d8a9f2"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"u4wiWe5yIJznXmsWEUEXsCUJE6GVLHpWJq1mcQPzDYGlCMSgiB2CC9Q/zuT3BuwsZsFDgwNCIYOw5OlV1shFAQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-01T04:34:01.269492Z","bundle_sha256":"f274827b03650ea5050f75b5d678a75ba1e9d2ab704053ecdafaf7a89eca1521"}}