{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2026:NRFCTC7ZNSLASUP6XWKASPOKY4","short_pith_number":"pith:NRFCTC7Z","canonical_record":{"source":{"id":"2605.15261","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2026-05-14T18:00:00Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE"],"title_canon_sha256":"38439f4101bf27b474413ccfb43d051a61e487ecd8f46f051054464a4992dac2","abstract_canon_sha256":"8bec4836a79e18e9d31f1b5ac2d916d5766b44d147822b73e4c4df9fe5029d1f"},"schema_version":"1.0"},"canonical_sha256":"6c4a298bf96c960951febd94093dcac717ab73caace232db3377f9352eed2fca","source":{"kind":"arxiv","id":"2605.15261","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2605.15261","created_at":"2026-05-20T00:00:49Z"},{"alias_kind":"arxiv_version","alias_value":"2605.15261v1","created_at":"2026-05-20T00:00:49Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.15261","created_at":"2026-05-20T00:00:49Z"},{"alias_kind":"pith_short_12","alias_value":"NRFCTC7ZNSLA","created_at":"2026-05-20T00:00:49Z"},{"alias_kind":"pith_short_16","alias_value":"NRFCTC7ZNSLASUP6","created_at":"2026-05-20T00:00:49Z"},{"alias_kind":"pith_short_8","alias_value":"NRFCTC7Z","created_at":"2026-05-20T00:00:49Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2026:NRFCTC7ZNSLASUP6XWKASPOKY4","target":"record","payload":{"canonical_record":{"source":{"id":"2605.15261","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2026-05-14T18:00:00Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE"],"title_canon_sha256":"38439f4101bf27b474413ccfb43d051a61e487ecd8f46f051054464a4992dac2","abstract_canon_sha256":"8bec4836a79e18e9d31f1b5ac2d916d5766b44d147822b73e4c4df9fe5029d1f"},"schema_version":"1.0"},"canonical_sha256":"6c4a298bf96c960951febd94093dcac717ab73caace232db3377f9352eed2fca","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-20T00:00:49.178983Z","signature_b64":"jCT1W+Yz2eg1U40NELwgh9eVsSvMR62fONpHTrGukhBND8SWpxSwISSK3YePV8gTRRuNjMMiblK/DP9BxQo6AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6c4a298bf96c960951febd94093dcac717ab73caace232db3377f9352eed2fca","last_reissued_at":"2026-05-20T00:00:49.178200Z","signature_status":"signed_v1","first_computed_at":"2026-05-20T00:00:49.178200Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"2605.15261","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":"2026-05-20T00:00:49Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"iLA0RFQiAdUz5XTNWRdFc9f86sDqANmao8yF61CqjDNdBxuw/JNrKpDMBYBmKBeVfoRZddE+BwhnUdNNYZiaCQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-21T11:10:50.633388Z"},"content_sha256":"3e4d55fe43a461f2884fcdba36a0072524f91e325cef68ab61ab3359612e56e1","schema_version":"1.0","event_id":"sha256:3e4d55fe43a461f2884fcdba36a0072524f91e325cef68ab61ab3359612e56e1"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2026:NRFCTC7ZNSLASUP6XWKASPOKY4","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"Turbulent magnetic fields boost axion-to-gamma conversion from supernovae by up to two orders of magnitude.","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"\\'Angel Gil Muyor, Damiano F. G. Fiorillo, Edoardo Vitagliano, Georg G. Raffelt","submitted_at":"2026-05-14T18:00:00Z","abstract_excerpt":"Magnetic fields between a supernova (SN) and Earth convert axions into gamma rays. The absence of such a signal in coincidence with SN 1987A neutrinos, using the coherent Milky Way field, provides well-studied constraints on $g_{ap}\\times g_{a\\gamma}$ (axion-proton times axion-photon couplings) and on $g_{a\\gamma}$ alone. We show that the small-scale power of the turbulent magnetic field component boosts axion-photon conversion and, crucially, extends sensitivity to larger masses. The turbulent field components of the Milky Way and of the Large Magellanic Cloud (hosting SN 1987A) yield improve"},"claims":{"count":4,"items":[{"kind":"strongest_claim","text":"The turbulent field components of the Milky Way and of the Large Magellanic Cloud yield improvements of up to two orders of magnitude in g_ap × g_aγ.","source":"verdict.strongest_claim","status":"machine_extracted","claim_id":"C1","attestation":"unclaimed"},{"kind":"weakest_assumption","text":"The assumed spectrum and coherence properties of the turbulent magnetic field components are accurate for the relevant propagation distances and axion mass range.","source":"verdict.weakest_assumption","status":"machine_extracted","claim_id":"C2","attestation":"unclaimed"},{"kind":"one_line_summary","text":"Turbulent magnetic fields enhance axion-photon conversion signals from supernovae, improving limits on axion-proton and axion-photon couplings by up to two orders of magnitude.","source":"verdict.one_line_summary","status":"machine_extracted","claim_id":"C3","attestation":"unclaimed"},{"kind":"headline","text":"Turbulent magnetic fields boost axion-to-gamma conversion from supernovae by up to two orders of magnitude.","source":"verdict.pith_extraction.headline","status":"machine_extracted","claim_id":"C4","attestation":"unclaimed"}],"snapshot_sha256":"e5a83e9357f3eac6951b44cfdc5ad60635bfcb28cccd01701200eb957812ab8a"},"source":{"id":"2605.15261","kind":"arxiv","version":1},"verdict":{"id":"05e77a38-c070-4e7f-a892-f77b2ceab3ee","model_set":{"reader":"grok-4.3"},"created_at":"2026-05-19T16:06:46.311147Z","strongest_claim":"The turbulent field components of the Milky Way and of the Large Magellanic Cloud yield improvements of up to two orders of magnitude in g_ap × g_aγ.","one_line_summary":"Turbulent magnetic fields enhance axion-photon conversion signals from supernovae, improving limits on axion-proton and axion-photon couplings by up to two orders of magnitude.","pipeline_version":"pith-pipeline@v0.9.0","weakest_assumption":"The assumed spectrum and coherence properties of the turbulent magnetic field components are accurate for the relevant propagation distances and axion mass range.","pith_extraction_headline":"Turbulent magnetic fields boost axion-to-gamma conversion from supernovae by up to two orders of magnitude."},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2605.15261/integrity.json","findings":[],"available":true,"detectors_run":[{"name":"doi_title_agreement","ran_at":"2026-05-19T16:31:18.408734Z","status":"completed","version":"1.0.0","findings_count":0},{"name":"doi_compliance","ran_at":"2026-05-19T16:18:00.967166Z","status":"completed","version":"1.0.0","findings_count":0},{"name":"claim_evidence","ran_at":"2026-05-19T14:41:54.270393Z","status":"completed","version":"1.0.0","findings_count":0},{"name":"ai_meta_artifact","ran_at":"2026-05-19T13:33:22.807571Z","status":"skipped","version":"1.0.0","findings_count":0}],"snapshot_sha256":"512e6775a275394360a985d3f49d54c0b6516282a23307e0dd8f508dbe2e4c64"},"references":{"count":91,"sample":[{"doi":"","year":1977,"title":"R. D. Peccei and H. R. Quinn,CP Conservation in the Presence of Instantons,Phys. Rev. Lett.38(1977) 1440","work_id":"783abdf3-4855-4202-8a1e-488a4f1f89b4","ref_index":1,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":1977,"title":"R. D. Peccei and H. R. Quinn,Constraints Imposed by CP Conservation in the Presence of Instantons,Phys. Rev. D16(1977) 1791","work_id":"6c935795-1cd5-42e4-a0de-4257ed09e0a7","ref_index":2,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":1978,"title":"Weinberg,A New Light Boson?,Phys","work_id":"53171858-ded9-4daa-a795-1db56516f68c","ref_index":3,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":1978,"title":"Wilczek,Problem of Strong P and T Invariance in the Presence of Instantons,Phys","work_id":"a6ee0653-621e-46b6-bb17-88800ab83140","ref_index":4,"cited_arxiv_id":"","is_internal_anchor":false},{"doi":"","year":1979,"title":"J. E. Kim,Weak Interaction Singlet and Strong CP Invariance,Phys. Rev. Lett.43(1979) 103","work_id":"64c585c4-4731-4978-97c5-c30cd7876b84","ref_index":5,"cited_arxiv_id":"","is_internal_anchor":false}],"resolved_work":91,"snapshot_sha256":"280a614c8fe4d713345c4aa1065e439d05f52feb7b0b62ba33a653502cd249a7","internal_anchors":24},"formal_canon":{"evidence_count":2,"snapshot_sha256":"78728736d94899a25f6ef59cddeff99b0144d27a0a4b232a2d503c20edd2fe80"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"verdict_id":"05e77a38-c070-4e7f-a892-f77b2ceab3ee"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-20T00:00:49Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"2+2Rs1B2B36anbgCreAtecAz6Dmxx1FZcj32yDxAGGtw6cxk0LNSHU+8O4dU5gPS11Lbf3hQQzaLLIaTBjhcCA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-21T11:10:50.634150Z"},"content_sha256":"4d9d257735dabd7d7e7179408f4781db3765361a89224edf22ed5a4a437ef89b","schema_version":"1.0","event_id":"sha256:4d9d257735dabd7d7e7179408f4781db3765361a89224edf22ed5a4a437ef89b"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/NRFCTC7ZNSLASUP6XWKASPOKY4/bundle.json","state_url":"https://pith.science/pith/NRFCTC7ZNSLASUP6XWKASPOKY4/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/NRFCTC7ZNSLASUP6XWKASPOKY4/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":"2026-05-21T11:10:50Z","links":{"resolver":"https://pith.science/pith/NRFCTC7ZNSLASUP6XWKASPOKY4","bundle":"https://pith.science/pith/NRFCTC7ZNSLASUP6XWKASPOKY4/bundle.json","state":"https://pith.science/pith/NRFCTC7ZNSLASUP6XWKASPOKY4/state.json","well_known_bundle":"https://pith.science/.well-known/pith/NRFCTC7ZNSLASUP6XWKASPOKY4/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2026:NRFCTC7ZNSLASUP6XWKASPOKY4","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":"8bec4836a79e18e9d31f1b5ac2d916d5766b44d147822b73e4c4df9fe5029d1f","cross_cats_sorted":["astro-ph.CO","astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2026-05-14T18:00:00Z","title_canon_sha256":"38439f4101bf27b474413ccfb43d051a61e487ecd8f46f051054464a4992dac2"},"schema_version":"1.0","source":{"id":"2605.15261","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"2605.15261","created_at":"2026-05-20T00:00:49Z"},{"alias_kind":"arxiv_version","alias_value":"2605.15261v1","created_at":"2026-05-20T00:00:49Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2605.15261","created_at":"2026-05-20T00:00:49Z"},{"alias_kind":"pith_short_12","alias_value":"NRFCTC7ZNSLA","created_at":"2026-05-20T00:00:49Z"},{"alias_kind":"pith_short_16","alias_value":"NRFCTC7ZNSLASUP6","created_at":"2026-05-20T00:00:49Z"},{"alias_kind":"pith_short_8","alias_value":"NRFCTC7Z","created_at":"2026-05-20T00:00:49Z"}],"graph_snapshots":[{"event_id":"sha256:4d9d257735dabd7d7e7179408f4781db3765361a89224edf22ed5a4a437ef89b","target":"graph","created_at":"2026-05-20T00:00:49Z","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":4,"items":[{"attestation":"unclaimed","claim_id":"C1","kind":"strongest_claim","source":"verdict.strongest_claim","status":"machine_extracted","text":"The turbulent field components of the Milky Way and of the Large Magellanic Cloud yield improvements of up to two orders of magnitude in g_ap × g_aγ."},{"attestation":"unclaimed","claim_id":"C2","kind":"weakest_assumption","source":"verdict.weakest_assumption","status":"machine_extracted","text":"The assumed spectrum and coherence properties of the turbulent magnetic field components are accurate for the relevant propagation distances and axion mass range."},{"attestation":"unclaimed","claim_id":"C3","kind":"one_line_summary","source":"verdict.one_line_summary","status":"machine_extracted","text":"Turbulent magnetic fields enhance axion-photon conversion signals from supernovae, improving limits on axion-proton and axion-photon couplings by up to two orders of magnitude."},{"attestation":"unclaimed","claim_id":"C4","kind":"headline","source":"verdict.pith_extraction.headline","status":"machine_extracted","text":"Turbulent magnetic fields boost axion-to-gamma conversion from supernovae by up to two orders of magnitude."}],"snapshot_sha256":"e5a83e9357f3eac6951b44cfdc5ad60635bfcb28cccd01701200eb957812ab8a"},"formal_canon":{"evidence_count":2,"snapshot_sha256":"78728736d94899a25f6ef59cddeff99b0144d27a0a4b232a2d503c20edd2fe80"},"integrity":{"available":true,"clean":true,"detectors_run":[{"findings_count":0,"name":"doi_title_agreement","ran_at":"2026-05-19T16:31:18.408734Z","status":"completed","version":"1.0.0"},{"findings_count":0,"name":"doi_compliance","ran_at":"2026-05-19T16:18:00.967166Z","status":"completed","version":"1.0.0"},{"findings_count":0,"name":"claim_evidence","ran_at":"2026-05-19T14:41:54.270393Z","status":"completed","version":"1.0.0"},{"findings_count":0,"name":"ai_meta_artifact","ran_at":"2026-05-19T13:33:22.807571Z","status":"skipped","version":"1.0.0"}],"endpoint":"/pith/2605.15261/integrity.json","findings":[],"snapshot_sha256":"512e6775a275394360a985d3f49d54c0b6516282a23307e0dd8f508dbe2e4c64","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"Magnetic fields between a supernova (SN) and Earth convert axions into gamma rays. The absence of such a signal in coincidence with SN 1987A neutrinos, using the coherent Milky Way field, provides well-studied constraints on $g_{ap}\\times g_{a\\gamma}$ (axion-proton times axion-photon couplings) and on $g_{a\\gamma}$ alone. We show that the small-scale power of the turbulent magnetic field component boosts axion-photon conversion and, crucially, extends sensitivity to larger masses. The turbulent field components of the Milky Way and of the Large Magellanic Cloud (hosting SN 1987A) yield improve","authors_text":"\\'Angel Gil Muyor, Damiano F. G. Fiorillo, Edoardo Vitagliano, Georg G. Raffelt","cross_cats":["astro-ph.CO","astro-ph.HE"],"headline":"Turbulent magnetic fields boost axion-to-gamma conversion from supernovae by up to two orders of magnitude.","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2026-05-14T18:00:00Z","title":"Magnetic Turbulence Boosts Supernova Signals of Axion-Photon Conversion"},"references":{"count":91,"internal_anchors":24,"resolved_work":91,"sample":[{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":1,"title":"R. D. Peccei and H. R. Quinn,CP Conservation in the Presence of Instantons,Phys. Rev. Lett.38(1977) 1440","work_id":"783abdf3-4855-4202-8a1e-488a4f1f89b4","year":1977},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":2,"title":"R. D. Peccei and H. R. Quinn,Constraints Imposed by CP Conservation in the Presence of Instantons,Phys. Rev. D16(1977) 1791","work_id":"6c935795-1cd5-42e4-a0de-4257ed09e0a7","year":1977},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":3,"title":"Weinberg,A New Light Boson?,Phys","work_id":"53171858-ded9-4daa-a795-1db56516f68c","year":1978},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":4,"title":"Wilczek,Problem of Strong P and T Invariance in the Presence of Instantons,Phys","work_id":"a6ee0653-621e-46b6-bb17-88800ab83140","year":1978},{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":5,"title":"J. E. Kim,Weak Interaction Singlet and Strong CP Invariance,Phys. Rev. Lett.43(1979) 103","work_id":"64c585c4-4731-4978-97c5-c30cd7876b84","year":1979}],"snapshot_sha256":"280a614c8fe4d713345c4aa1065e439d05f52feb7b0b62ba33a653502cd249a7"},"source":{"id":"2605.15261","kind":"arxiv","version":1},"verdict":{"created_at":"2026-05-19T16:06:46.311147Z","id":"05e77a38-c070-4e7f-a892-f77b2ceab3ee","model_set":{"reader":"grok-4.3"},"one_line_summary":"Turbulent magnetic fields enhance axion-photon conversion signals from supernovae, improving limits on axion-proton and axion-photon couplings by up to two orders of magnitude.","pipeline_version":"pith-pipeline@v0.9.0","pith_extraction_headline":"Turbulent magnetic fields boost axion-to-gamma conversion from supernovae by up to two orders of magnitude.","strongest_claim":"The turbulent field components of the Milky Way and of the Large Magellanic Cloud yield improvements of up to two orders of magnitude in g_ap × g_aγ.","weakest_assumption":"The assumed spectrum and coherence properties of the turbulent magnetic field components are accurate for the relevant propagation distances and axion mass range."}},"verdict_id":"05e77a38-c070-4e7f-a892-f77b2ceab3ee"}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:3e4d55fe43a461f2884fcdba36a0072524f91e325cef68ab61ab3359612e56e1","target":"record","created_at":"2026-05-20T00:00:49Z","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":"8bec4836a79e18e9d31f1b5ac2d916d5766b44d147822b73e4c4df9fe5029d1f","cross_cats_sorted":["astro-ph.CO","astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2026-05-14T18:00:00Z","title_canon_sha256":"38439f4101bf27b474413ccfb43d051a61e487ecd8f46f051054464a4992dac2"},"schema_version":"1.0","source":{"id":"2605.15261","kind":"arxiv","version":1}},"canonical_sha256":"6c4a298bf96c960951febd94093dcac717ab73caace232db3377f9352eed2fca","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"6c4a298bf96c960951febd94093dcac717ab73caace232db3377f9352eed2fca","first_computed_at":"2026-05-20T00:00:49.178200Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-20T00:00:49.178200Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"jCT1W+Yz2eg1U40NELwgh9eVsSvMR62fONpHTrGukhBND8SWpxSwISSK3YePV8gTRRuNjMMiblK/DP9BxQo6AQ==","signature_status":"signed_v1","signed_at":"2026-05-20T00:00:49.178983Z","signed_message":"canonical_sha256_bytes"},"source_id":"2605.15261","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:3e4d55fe43a461f2884fcdba36a0072524f91e325cef68ab61ab3359612e56e1","sha256:4d9d257735dabd7d7e7179408f4781db3765361a89224edf22ed5a4a437ef89b"],"state_sha256":"23a4769b6cd2cc5e744da5f88d01e66f844af275745f915830eec39bb33ab839"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"XwxmLuQqTsSJErSn0uk7eW6d/vMZwEi9/YKXI+/fsUI6A9AaiGH0DmnpknoNgwU/oMKfxDa7QYLlY+LirIuICQ==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-21T11:10:50.637092Z","bundle_sha256":"c37a554be6575470b7893a5e878b373d288caaf21e05ed780e1fc6af9fcda3ca"}}