{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2026:2RYDE4WIN26KG5Q4HBT3Z7FO4R","short_pith_number":"pith:2RYDE4WI","canonical_record":{"source":{"id":"2608.10124","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2026-08-10T18:37:13Z","cross_cats_sorted":[],"title_canon_sha256":"b0a3400973863dcd840441dd6aa1cecdceadb15a745537ee120f1538a8d85b89","abstract_canon_sha256":"ebfd03bcdbcbec6f9ae7670931b45f1050197361f3fb5c8c631fff0fdb0c25c9"},"schema_version":"1.0"},"canonical_sha256":"d4703272c86ebca3761c3867bcfcaee46ee82a80f66c1fe1c75238ca93ccd1bc","source":{"kind":"arxiv","id":"2608.10124","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2608.10124","created_at":"2026-08-12T00:22:51Z"},{"alias_kind":"arxiv_version","alias_value":"2608.10124v1","created_at":"2026-08-12T00:22:51Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2608.10124","created_at":"2026-08-12T00:22:51Z"},{"alias_kind":"pith_short_12","alias_value":"2RYDE4WIN26K","created_at":"2026-08-12T00:22:51Z"},{"alias_kind":"pith_short_16","alias_value":"2RYDE4WIN26KG5Q4","created_at":"2026-08-12T00:22:51Z"},{"alias_kind":"pith_short_8","alias_value":"2RYDE4WI","created_at":"2026-08-12T00:22:51Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2026:2RYDE4WIN26KG5Q4HBT3Z7FO4R","target":"record","payload":{"canonical_record":{"source":{"id":"2608.10124","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2026-08-10T18:37:13Z","cross_cats_sorted":[],"title_canon_sha256":"b0a3400973863dcd840441dd6aa1cecdceadb15a745537ee120f1538a8d85b89","abstract_canon_sha256":"ebfd03bcdbcbec6f9ae7670931b45f1050197361f3fb5c8c631fff0fdb0c25c9"},"schema_version":"1.0"},"canonical_sha256":"d4703272c86ebca3761c3867bcfcaee46ee82a80f66c1fe1c75238ca93ccd1bc","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-08-12T00:22:51.930247Z","signature_b64":"XZ0lHYJ72bNcahCxrV4IM7wzvxRisFZbGpgssga1ZpelBDkcx7O9fQUmW4aAsc/08TQLsAxaQlBiOTFEuVJ1Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d4703272c86ebca3761c3867bcfcaee46ee82a80f66c1fe1c75238ca93ccd1bc","last_reissued_at":"2026-08-12T00:22:51.928635Z","signature_status":"signed_v1","first_computed_at":"2026-08-12T00:22:51.928635Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"2608.10124","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":"2026-08-12T00:22:51Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"me6EppijhZn4M2M21o1dueLJKiVOkJmFAqqKTfztpF15QfRNgCB6zEDtzKplSTbgxa1s3AywfRRH60oZB589Ag==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-14T23:15:41.120076Z"},"content_sha256":"b35b8308007cd26434f8702d98a4ea977d3ac4866d12143da281cb17ff32ba18","schema_version":"1.0","event_id":"sha256:b35b8308007cd26434f8702d98a4ea977d3ac4866d12143da281cb17ff32ba18"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2026:2RYDE4WIN26KG5Q4HBT3Z7FO4R","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Steady state, core, operational optimization of an ARC-like tokamak via plasma composition and shape","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.plasm-ph","authors_text":"A. Ho, A.J. Creely, A. Saltzman, G. Snoep, J. Hall, J. Han, J. Hillesheim, M.S. Anastopoulos Tzanis, N.T. Howard, P. Rodriguez-Fernandez, P. Snyder","submitted_at":"2026-08-10T18:37:13Z","abstract_excerpt":"Impurity composition, plasma shape, and pedestal density all provide strong levers on fusion power. Here, we explore the ways in which their variation changes fusion power and seek to find the optimum of these parameters. The key impacts of these variables are through changes in the core turbulent transport, the density of the fuel species, the pedestal pressure, and the plasma volume. ITG stabilization due to increased amounts of impurities is observed. The dependence of all of these parameters on the pedestal pressure is especially complicated because of the separate impacts on the peeling a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2608.10124","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2608.10124/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2026-08-12T00:22:51Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Ju2IDv34Mi1cFdmLBrPqcDTtunR3J1bz0SCqGNaJ8DJCxfnlKdgyGzIeVUWsM/LYHh0rW+71IhW1ujcM90bvCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-14T23:15:41.120582Z"},"content_sha256":"320fb72c00413bb6501bfb2607976df31d110985770039b987d425bf9456bee1","schema_version":"1.0","event_id":"sha256:320fb72c00413bb6501bfb2607976df31d110985770039b987d425bf9456bee1"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:2RYDE4WIN26KG5Q4HBT3Z7FO4R","target":"integrity","payload":{"note":"Identifier '10.1088/0029-5515/47/9/033(visited' is syntactically valid but the DOI registry (doi.org) returned 404, and Crossref / OpenAlex / internal corpus also have no record. The cited work could not be located through any authoritative source.","snippet":"C. Angioni, H. Weisen, O. J. W. F. Kardaun, M. Maslov, A. Zabolotsky, C. Fuchs, L. Garzotti, C. Giroud, B. Kurzan, P. Mantica, A. G. Peeters, J. Stober, the ASDEX Upgrade Team, and contributors to the EFDA-JET Workprogramme. “Scaling of den","arxiv_id":"2608.10124","detector":"doi_compliance","evidence":{"doi":"10.1088/0029-5515/47/9/033(visited","arxiv_id":null,"ref_index":96,"raw_excerpt":"C. Angioni, H. Weisen, O. J. W. F. Kardaun, M. Maslov, A. Zabolotsky, C. Fuchs, L. Garzotti, C. Giroud, B. Kurzan, P. Mantica, A. G. Peeters, J. Stober, the ASDEX Upgrade Team, and contributors to the EFDA-JET Workprogramme. “Scaling of density peaking in H-mode plasmas based on a combined database of AUG and JET observations”. en. In:Nuclear Fusion47.9 (Aug. 2007), p. 1326.issn: 0029-5515.doi:10 ","parse_status":"well_formed","verdict_class":"cross_source","checked_sources":["crossref_by_doi","openalex_by_doi","doi_org_head"],"resolution_status":"hard_miss"},"severity":"critical","ref_index":96,"audited_at":"2026-08-14T04:20:16.566052Z","event_type":"pith.integrity.v1","detected_doi":"10.1088/0029-5515/47/9/033(visited","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"unresolvable_identifier","evidence_hash":"41ad4117cce9975f9c36dae47bdd57985691aa9762c149406ef0fc6adc45decf","paper_version":1,"verdict_class":"cross_source","resolved_title":null,"detector_version":"1.1.0","detected_arxiv_id":null,"integrity_event_id":19473,"payload_sha256":"f522838c96a80bd7bd7b0032f65f3b4eded92ebf2eb43f466b706e96c4b142e1","signature_b64":"Y9Lg0o1+4sgvvsGgzFABlioDLYyT9IFFlvwztnYbDex3+umOf6OeiP0eb1seOBSsqePQ39Z2zLdEPq2LWAthDg==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-08-14T04:23:31Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"3ByO3MoK3Yu0ou8Dvg4F1cLN6F+dDccP94IZYpnf9sdD+T/aA3hPwoeY9EFHzt/Og+s6N+vHeQ+NYPIe8QrFCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-14T23:15:41.124148Z"},"content_sha256":"f501f9383a957b936211cb4e71df4a52de6334489b188ae7a0c2bf0182252f1f","schema_version":"1.0","event_id":"sha256:f501f9383a957b936211cb4e71df4a52de6334489b188ae7a0c2bf0182252f1f"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:2RYDE4WIN26KG5Q4HBT3Z7FO4R","target":"integrity","payload":{"note":"Identifier '10.1063/1.2972160(visited' is syntactically valid but the DOI registry (doi.org) returned 404, and Crossref / OpenAlex / internal corpus also have no record. The cited work could not be located through any authoritative source.","snippet":"E. A. Belli, G. W. Hammett, and W. Dorland. “Effects of plasma shaping on nonlinear gyrokinetic turbulence”. In:Physics of Plasmas15.9 (Sept. 2008), p. 092303.issn: 1070-664X.doi:10.1063/ 1.2972160.url:https://doi.org/10.1063/1.2972160(visi","arxiv_id":"2608.10124","detector":"doi_compliance","evidence":{"doi":"10.1063/1.2972160(visited","arxiv_id":null,"ref_index":72,"raw_excerpt":"E. A. Belli, G. W. Hammett, and W. Dorland. “Effects of plasma shaping on nonlinear gyrokinetic turbulence”. In:Physics of Plasmas15.9 (Sept. 2008), p. 092303.issn: 1070-664X.doi:10.1063/ 1.2972160.url:https://doi.org/10.1063/1.2972160(visited on 11/02/2025)","parse_status":"well_formed","verdict_class":"cross_source","checked_sources":["crossref_by_doi","openalex_by_doi","doi_org_head"],"resolution_status":"hard_miss"},"severity":"critical","ref_index":72,"audited_at":"2026-08-14T04:20:16.566052Z","event_type":"pith.integrity.v1","detected_doi":"10.1063/1.2972160(visited","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"unresolvable_identifier","evidence_hash":"21738fdb7f475ce8e00643899e3921d5a5f5ce0b114dd830b3d0b4940ea4cbc9","paper_version":1,"verdict_class":"cross_source","resolved_title":null,"detector_version":"1.1.0","detected_arxiv_id":null,"integrity_event_id":19472,"payload_sha256":"9117cac2fbc91accef7b17d13c9d36ce77c5fdd65cb8189f52b2006f9b98114a","signature_b64":"ncnewp7T/ijbFj9O1yIgZ5jgXBT9G9v9cpprPW1T2A6V1PVdWHNNUbDe9IzCX0mmB+PNW2hPaBOr+atL9KHzCA==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-08-14T04:23:31Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"efqpbUaRPsUken/QVzmlPW13elV1ew94ZKHb4V3Ri6YNnyRKzV0IAybkRLRZe7IunsPKHX332a7CEdoTnKp5BA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-14T23:15:41.124648Z"},"content_sha256":"8b42afb08a4e4a74f0de4a1c3edff45ff3a04849a93251d00b160778f077c728","schema_version":"1.0","event_id":"sha256:8b42afb08a4e4a74f0de4a1c3edff45ff3a04849a93251d00b160778f077c728"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:2RYDE4WIN26KG5Q4HBT3Z7FO4R","target":"integrity","payload":{"note":"Identifier '10.1088/0029-5515/47/7/006(visited' is syntactically valid but the DOI registry (doi.org) returned 404, and Crossref / OpenAlex / internal corpus also have no record. The cited work could not be located through any authoritative source.","snippet":"A.W Leonard, T.A Casper, R.J Groebner, T.H Osborne, P.B Snyder, and D.M Thomas. “Pedestal performance dependence upon plasma shape in DIII-D”. In:Nuclear Fusion47.7 (July 2007), pp. 552–562.issn: 0029-5515, 1741-4326.doi:10 . 1088 / 0029 - ","arxiv_id":"2608.10124","detector":"doi_compliance","evidence":{"doi":"10.1088/0029-5515/47/7/006(visited","arxiv_id":null,"ref_index":68,"raw_excerpt":"A.W Leonard, T.A Casper, R.J Groebner, T.H Osborne, P.B Snyder, and D.M Thomas. “Pedestal performance dependence upon plasma shape in DIII-D”. In:Nuclear Fusion47.7 (July 2007), pp. 552–562.issn: 0029-5515, 1741-4326.doi:10 . 1088 / 0029 - 5515 / 47 / 7 / 006.url:https : //iopscience.iop.org/article/10.1088/0029-5515/47/7/006(visited on 08/14/2025). 41","parse_status":"well_formed","verdict_class":"cross_source","checked_sources":["crossref_by_doi","openalex_by_doi","doi_org_head"],"resolution_status":"hard_miss"},"severity":"critical","ref_index":68,"audited_at":"2026-08-14T04:20:16.566052Z","event_type":"pith.integrity.v1","detected_doi":"10.1088/0029-5515/47/7/006(visited","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"unresolvable_identifier","evidence_hash":"6fec495e9121c4df11c1ce0bc606c2b7e0bad20d649ae06cb59257f1fc040f97","paper_version":1,"verdict_class":"cross_source","resolved_title":null,"detector_version":"1.1.0","detected_arxiv_id":null,"integrity_event_id":19471,"payload_sha256":"d025032fd0d35d142c691eb20e88cc04d7d3c2bbb83b92be0394141b605e7f5f","signature_b64":"Vgm0WOadwzlMGavyO1DT82QGJfS8sUZqpUUwO0FaRSHFsyomM0bh4UOhPRmfqNT35wEIfwhcQ4rd6ICsnsVZAg==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-08-14T04:23:31Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"c2s+fqWQkATtzpvpTZMbrebdJpwx/KtsRYK1tgBC6UenEnUaJBk+IRG0o1TU36uUQXSU+5f+yshPVYc87n27Dw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-14T23:15:41.125074Z"},"content_sha256":"36a0fbf24682cf38a4dd91b925421deeeceff5f1fbf6ff6f84edb80803a1897a","schema_version":"1.0","event_id":"sha256:36a0fbf24682cf38a4dd91b925421deeeceff5f1fbf6ff6f84edb80803a1897a"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:2RYDE4WIN26KG5Q4HBT3Z7FO4R","target":"integrity","payload":{"note":"Identifier '10.1088/1742-6596/123/1/012033(visited' is syntactically valid but the DOI registry (doi.org) returned 404, and Crossref / OpenAlex / internal corpus also have no record. The cited work could not be located through any authoritative source.","snippet":"Y R Martin, T Takizuka, and the ITPA CDBM H-mode Threshold Data Group. “Power require- ment for accessing the H-mode in ITER”. In:Journal of Physics: Conference Series123 (July 2008), p. 012033.issn: 1742-6596.doi:10 . 1088 / 1742 - 6596 / ","arxiv_id":"2608.10124","detector":"doi_compliance","evidence":{"doi":"10.1088/1742-6596/123/1/012033(visited","arxiv_id":null,"ref_index":40,"raw_excerpt":"Y R Martin, T Takizuka, and the ITPA CDBM H-mode Threshold Data Group. “Power require- ment for accessing the H-mode in ITER”. In:Journal of Physics: Conference Series123 (July 2008), p. 012033.issn: 1742-6596.doi:10 . 1088 / 1742 - 6596 / 123 / 1 / 012033.url:https : //iopscience.iop.org/article/10.1088/1742-6596/123/1/012033(visited on 08/13/2020)","parse_status":"well_formed","verdict_class":"cross_source","checked_sources":["crossref_by_doi","openalex_by_doi","doi_org_head"],"resolution_status":"hard_miss"},"severity":"critical","ref_index":40,"audited_at":"2026-08-14T04:20:16.566052Z","event_type":"pith.integrity.v1","detected_doi":"10.1088/1742-6596/123/1/012033(visited","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"unresolvable_identifier","evidence_hash":"edf712032065503a2838190e91f89050fbbc00bdf3782cd4811e14f3c709f1dd","paper_version":1,"verdict_class":"cross_source","resolved_title":null,"detector_version":"1.1.0","detected_arxiv_id":null,"integrity_event_id":19470,"payload_sha256":"bd87241daad63e898225736d78e6777e9f390e03dcff52ada4f6aee58dcb6bb8","signature_b64":"AMX6sPDfGEglQ3VJJ0y3YSYNZ62cTGTHm4DOWUjmI7mZ5J3b26Qd9Cufbxz71BbxHpMC63qnZsO1w588fDPhAA==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-08-14T04:23:31Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ISY2dIxIRNX4XnHkYvHl41BYVk8Or2EddfKDQokj5uTUoxMST/57mb90LdRbz9jmYY8G7MmeepbyskD7sJRjCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-14T23:15:41.125456Z"},"content_sha256":"5d04bc47b7af8ee73f7e86e920c40a4538f0f256ea0d70130cd5fe7d02c151c8","schema_version":"1.0","event_id":"sha256:5d04bc47b7af8ee73f7e86e920c40a4538f0f256ea0d70130cd5fe7d02c151c8"},{"event_type":"integrity_finding","subject_pith_number":"pith:2026:2RYDE4WIN26KG5Q4HBT3Z7FO4R","target":"integrity","payload":{"note":"Identifier '10.1088/0029-5515/32/8/i03(visited' is syntactically valid but the DOI registry (doi.org) returned 404, and Crossref / OpenAlex / internal corpus also have no record. The cited work could not be located through any authoritative source.","snippet":"S. Migliuolo. “Ion temperature gradient driven impurity modes”. en. In:Nuclear Fusion32.8 (Aug. 1992), p. 1331.issn: 0029-5515.doi:10 . 1088 / 0029 - 5515 / 32 / 8 / I03.url:https : //dx.doi.org/10.1088/0029-5515/32/8/I03(visited on 07/25/2","arxiv_id":"2608.10124","detector":"doi_compliance","evidence":{"doi":"10.1088/0029-5515/32/8/i03(visited","arxiv_id":null,"ref_index":25,"raw_excerpt":"S. Migliuolo. “Ion temperature gradient driven impurity modes”. en. In:Nuclear Fusion32.8 (Aug. 1992), p. 1331.issn: 0029-5515.doi:10 . 1088 / 0029 - 5515 / 32 / 8 / I03.url:https : //dx.doi.org/10.1088/0029-5515/32/8/I03(visited on 07/25/2025)","parse_status":"well_formed","verdict_class":"cross_source","checked_sources":["crossref_by_doi","openalex_by_doi","doi_org_head"],"resolution_status":"hard_miss"},"severity":"critical","ref_index":25,"audited_at":"2026-08-14T04:20:16.566052Z","event_type":"pith.integrity.v1","detected_doi":"10.1088/0029-5515/32/8/i03(visited","detector_url":"https://pith.science/pith-integrity-protocol#doi_compliance","external_url":null,"finding_type":"unresolvable_identifier","evidence_hash":"69d56eda60d211db53d0b1dd773ad889c45959aafdccf965a43cbe38d3b64ce7","paper_version":1,"verdict_class":"cross_source","resolved_title":null,"detector_version":"1.1.0","detected_arxiv_id":null,"integrity_event_id":19469,"payload_sha256":"016c39002fe0c745885684abdc4fe65f64fb9903c6c5fbd5d0638136ca9f3c62","signature_b64":"jnfY5O04kqgdpy5VRuQjqdbdQ4eX16UQSnIqG9YzdRH2GkmrXP07pDDdkYJxeELBtQhHDvt63LZosEFCGfYRAg==","signing_key_id":"pith-v1-2026-05"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-08-14T04:23:31Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"r1F5TrJtgLVksHboL8V9iDQDj/EmuobxnH4YzqiBf/jU8j1y4VpP3hjUKagNeFZaPRNEEsR+/CejEJs9ljRgDQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-14T23:15:41.125850Z"},"content_sha256":"9bf31bde45c654949eee3ed9775e748f950beb09eee3b683cc37d7643f18454d","schema_version":"1.0","event_id":"sha256:9bf31bde45c654949eee3ed9775e748f950beb09eee3b683cc37d7643f18454d"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/2RYDE4WIN26KG5Q4HBT3Z7FO4R/bundle.json","state_url":"https://pith.science/pith/2RYDE4WIN26KG5Q4HBT3Z7FO4R/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/2RYDE4WIN26KG5Q4HBT3Z7FO4R/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":"2026-08-14T23:15:41Z","links":{"resolver":"https://pith.science/pith/2RYDE4WIN26KG5Q4HBT3Z7FO4R","bundle":"https://pith.science/pith/2RYDE4WIN26KG5Q4HBT3Z7FO4R/bundle.json","state":"https://pith.science/pith/2RYDE4WIN26KG5Q4HBT3Z7FO4R/state.json","well_known_bundle":"https://pith.science/.well-known/pith/2RYDE4WIN26KG5Q4HBT3Z7FO4R/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2026:2RYDE4WIN26KG5Q4HBT3Z7FO4R","merge_version":"pith-open-graph-merge-v1","event_count":7,"valid_event_count":7,"invalid_event_count":0,"equivocation_count":1,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"ebfd03bcdbcbec6f9ae7670931b45f1050197361f3fb5c8c631fff0fdb0c25c9","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2026-08-10T18:37:13Z","title_canon_sha256":"b0a3400973863dcd840441dd6aa1cecdceadb15a745537ee120f1538a8d85b89"},"schema_version":"1.0","source":{"id":"2608.10124","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2608.10124","created_at":"2026-08-12T00:22:51Z"},{"alias_kind":"arxiv_version","alias_value":"2608.10124v1","created_at":"2026-08-12T00:22:51Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2608.10124","created_at":"2026-08-12T00:22:51Z"},{"alias_kind":"pith_short_12","alias_value":"2RYDE4WIN26K","created_at":"2026-08-12T00:22:51Z"},{"alias_kind":"pith_short_16","alias_value":"2RYDE4WIN26KG5Q4","created_at":"2026-08-12T00:22:51Z"},{"alias_kind":"pith_short_8","alias_value":"2RYDE4WI","created_at":"2026-08-12T00:22:51Z"}],"graph_snapshots":[{"event_id":"sha256:320fb72c00413bb6501bfb2607976df31d110985770039b987d425bf9456bee1","target":"graph","created_at":"2026-08-12T00:22:51Z","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"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/2608.10124/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"Impurity composition, plasma shape, and pedestal density all provide strong levers on fusion power. Here, we explore the ways in which their variation changes fusion power and seek to find the optimum of these parameters. The key impacts of these variables are through changes in the core turbulent transport, the density of the fuel species, the pedestal pressure, and the plasma volume. ITG stabilization due to increased amounts of impurities is observed. The dependence of all of these parameters on the pedestal pressure is especially complicated because of the separate impacts on the peeling a","authors_text":"A. Ho, A.J. Creely, A. Saltzman, G. Snoep, J. Hall, J. Han, J. Hillesheim, M.S. Anastopoulos Tzanis, N.T. Howard, P. Rodriguez-Fernandez, P. Snyder","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2026-08-10T18:37:13Z","title":"Steady state, core, operational optimization of an ARC-like tokamak via plasma composition and shape"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2608.10124","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:b35b8308007cd26434f8702d98a4ea977d3ac4866d12143da281cb17ff32ba18","target":"record","created_at":"2026-08-12T00:22:51Z","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":"ebfd03bcdbcbec6f9ae7670931b45f1050197361f3fb5c8c631fff0fdb0c25c9","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2026-08-10T18:37:13Z","title_canon_sha256":"b0a3400973863dcd840441dd6aa1cecdceadb15a745537ee120f1538a8d85b89"},"schema_version":"1.0","source":{"id":"2608.10124","kind":"arxiv","version":1}},"canonical_sha256":"d4703272c86ebca3761c3867bcfcaee46ee82a80f66c1fe1c75238ca93ccd1bc","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"d4703272c86ebca3761c3867bcfcaee46ee82a80f66c1fe1c75238ca93ccd1bc","first_computed_at":"2026-08-12T00:22:51.928635Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-08-12T00:22:51.928635Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"XZ0lHYJ72bNcahCxrV4IM7wzvxRisFZbGpgssga1ZpelBDkcx7O9fQUmW4aAsc/08TQLsAxaQlBiOTFEuVJ1Bw==","signature_status":"signed_v1","signed_at":"2026-08-12T00:22:51.930247Z","signed_message":"canonical_sha256_bytes"},"source_id":"2608.10124","source_kind":"arxiv","source_version":1}}},"equivocations":[{"signer_id":"pith.science","event_type":"integrity_finding","target":"integrity","event_ids":["sha256:36a0fbf24682cf38a4dd91b925421deeeceff5f1fbf6ff6f84edb80803a1897a","sha256:5d04bc47b7af8ee73f7e86e920c40a4538f0f256ea0d70130cd5fe7d02c151c8","sha256:8b42afb08a4e4a74f0de4a1c3edff45ff3a04849a93251d00b160778f077c728","sha256:9bf31bde45c654949eee3ed9775e748f950beb09eee3b683cc37d7643f18454d","sha256:f501f9383a957b936211cb4e71df4a52de6334489b188ae7a0c2bf0182252f1f"]}],"invalid_events":[],"applied_event_ids":["sha256:b35b8308007cd26434f8702d98a4ea977d3ac4866d12143da281cb17ff32ba18","sha256:320fb72c00413bb6501bfb2607976df31d110985770039b987d425bf9456bee1"],"state_sha256":"2d2fdee675af16d28ede036d56dccfc89db400946a867cbaeef4fb1394146746"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"XEzjJ8DMNayz6v3zJJiMkuvrt2p5vFtyHpzJtS7nP8wf9x7Riu3jgX0Oe16naRnw49mzchHgK4EC/Z1lDvqXBw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-14T23:15:41.129501Z","bundle_sha256":"1aeb407672010997dbba1d6eac858545f23aac1c66f4143bfc672c238974734f"}}