{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2010:LR5YGI73REMJK4QNUZX2YX6TT3","short_pith_number":"pith:LR5YGI73","canonical_record":{"source":{"id":"1012.2728","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-12-13T13:51:52Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"d26c45ab7bd866ab6b85da54c7a6988c86903ebfd7b5f9658f1f4f6f285f277b","abstract_canon_sha256":"e661ba372f1a1762280496d8dfb7e587f976f2968d3f38052c6e301b05627248"},"schema_version":"1.0"},"canonical_sha256":"5c7b8323fb891895720da66fac5fd39eee8fb8b525880cc61dcb77f380ab1e90","source":{"kind":"arxiv","id":"1012.2728","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1012.2728","created_at":"2026-05-18T02:04:27Z"},{"alias_kind":"arxiv_version","alias_value":"1012.2728v2","created_at":"2026-05-18T02:04:27Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1012.2728","created_at":"2026-05-18T02:04:27Z"},{"alias_kind":"pith_short_12","alias_value":"LR5YGI73REMJ","created_at":"2026-05-18T12:26:10Z"},{"alias_kind":"pith_short_16","alias_value":"LR5YGI73REMJK4QN","created_at":"2026-05-18T12:26:10Z"},{"alias_kind":"pith_short_8","alias_value":"LR5YGI73","created_at":"2026-05-18T12:26:10Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2010:LR5YGI73REMJK4QNUZX2YX6TT3","target":"record","payload":{"canonical_record":{"source":{"id":"1012.2728","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-12-13T13:51:52Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"d26c45ab7bd866ab6b85da54c7a6988c86903ebfd7b5f9658f1f4f6f285f277b","abstract_canon_sha256":"e661ba372f1a1762280496d8dfb7e587f976f2968d3f38052c6e301b05627248"},"schema_version":"1.0"},"canonical_sha256":"5c7b8323fb891895720da66fac5fd39eee8fb8b525880cc61dcb77f380ab1e90","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:04:27.625871Z","signature_b64":"Zw7vczOe/fFo8+51UHEv5huHK1DVox6yP1mMvzNimoDn3OiViLMTG+OclyhOIhA3C7oG627lGXN1M296U+BcCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5c7b8323fb891895720da66fac5fd39eee8fb8b525880cc61dcb77f380ab1e90","last_reissued_at":"2026-05-18T02:04:27.625145Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:04:27.625145Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1012.2728","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":"2026-05-18T02:04:27Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"CSKpTr/k1qm7vQclGmL9BLECX7LGk6BZsdv7PUo3iX4TLA7ihjloFgPeq7pRcQN2c8rmjOHhEfy90Hm12VbODw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-18T19:46:54.302909Z"},"content_sha256":"374fc4569cb1f0251ba82ca5444e1cfbf3b04d91a8e73a6d476a3be3dad64303","schema_version":"1.0","event_id":"sha256:374fc4569cb1f0251ba82ca5444e1cfbf3b04d91a8e73a6d476a3be3dad64303"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2010:LR5YGI73REMJK4QNUZX2YX6TT3","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"SUSY Renormalization Group Effects in Ultra High Energy Neutrinos","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"2), (2) Fermilab, (3) Valencia U., 4) ((1) Lima, (4) Frascati), A.M. Gago (1), IFIC, J. Jones-Perez (3, M. Bustamante (1, Pont. U. Catolica","submitted_at":"2010-12-13T13:51:52Z","abstract_excerpt":"We have explored the question of whether the renormalization group running of the neutrino mixing parameters in the Minimal Supersymmetric Standard Model is detectable with ultra-high energy neutrinos from active galactic nuclei (AGN). We use as observables the ratios of neutrino fluxes produced at the AGN, focusing on four different neutrino production models: $(\\Phi_{\\nu_e+\\bar{\\nu}_e}^0 : \\Phi_{\\nu_\\mu+\\bar{\\nu}_\\mu}^0 : \\Phi_{\\nu_\\tau+\\bar{\\nu}_\\tau}^0)$ = (1:2:0), (0:1:0), (1:0:0), and (1:1:0). The prospects for observing deviations experimentally are taken into consideration, and we find"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1012.2728","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":"2026-05-18T02:04:27Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Wod1ip6+9roby3eVS3qF26KeAMbTBjGYBfPea9eSTQ7IY4w5aN/mvozc7B1Y4dhfZ/2htoKXptVY0WauS28zAQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-18T19:46:54.303596Z"},"content_sha256":"eca3f44fd3c5a5a490e46c2bf925c6944c808e6ebd549cf0879bb52d42e7a873","schema_version":"1.0","event_id":"sha256:eca3f44fd3c5a5a490e46c2bf925c6944c808e6ebd549cf0879bb52d42e7a873"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/LR5YGI73REMJK4QNUZX2YX6TT3/bundle.json","state_url":"https://pith.science/pith/LR5YGI73REMJK4QNUZX2YX6TT3/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/LR5YGI73REMJK4QNUZX2YX6TT3/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":"2026-05-18T19:46:54Z","links":{"resolver":"https://pith.science/pith/LR5YGI73REMJK4QNUZX2YX6TT3","bundle":"https://pith.science/pith/LR5YGI73REMJK4QNUZX2YX6TT3/bundle.json","state":"https://pith.science/pith/LR5YGI73REMJK4QNUZX2YX6TT3/state.json","well_known_bundle":"https://pith.science/.well-known/pith/LR5YGI73REMJK4QNUZX2YX6TT3/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2010:LR5YGI73REMJK4QNUZX2YX6TT3","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":"e661ba372f1a1762280496d8dfb7e587f976f2968d3f38052c6e301b05627248","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-12-13T13:51:52Z","title_canon_sha256":"d26c45ab7bd866ab6b85da54c7a6988c86903ebfd7b5f9658f1f4f6f285f277b"},"schema_version":"1.0","source":{"id":"1012.2728","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1012.2728","created_at":"2026-05-18T02:04:27Z"},{"alias_kind":"arxiv_version","alias_value":"1012.2728v2","created_at":"2026-05-18T02:04:27Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1012.2728","created_at":"2026-05-18T02:04:27Z"},{"alias_kind":"pith_short_12","alias_value":"LR5YGI73REMJ","created_at":"2026-05-18T12:26:10Z"},{"alias_kind":"pith_short_16","alias_value":"LR5YGI73REMJK4QN","created_at":"2026-05-18T12:26:10Z"},{"alias_kind":"pith_short_8","alias_value":"LR5YGI73","created_at":"2026-05-18T12:26:10Z"}],"graph_snapshots":[{"event_id":"sha256:eca3f44fd3c5a5a490e46c2bf925c6944c808e6ebd549cf0879bb52d42e7a873","target":"graph","created_at":"2026-05-18T02:04:27Z","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 have explored the question of whether the renormalization group running of the neutrino mixing parameters in the Minimal Supersymmetric Standard Model is detectable with ultra-high energy neutrinos from active galactic nuclei (AGN). We use as observables the ratios of neutrino fluxes produced at the AGN, focusing on four different neutrino production models: $(\\Phi_{\\nu_e+\\bar{\\nu}_e}^0 : \\Phi_{\\nu_\\mu+\\bar{\\nu}_\\mu}^0 : \\Phi_{\\nu_\\tau+\\bar{\\nu}_\\tau}^0)$ = (1:2:0), (0:1:0), (1:0:0), and (1:1:0). The prospects for observing deviations experimentally are taken into consideration, and we find","authors_text":"2), (2) Fermilab, (3) Valencia U., 4) ((1) Lima, (4) Frascati), A.M. Gago (1), IFIC, J. Jones-Perez (3, M. Bustamante (1, Pont. U. Catolica","cross_cats":["astro-ph.HE"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-12-13T13:51:52Z","title":"SUSY Renormalization Group Effects in Ultra High Energy Neutrinos"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1012.2728","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":"sha256:374fc4569cb1f0251ba82ca5444e1cfbf3b04d91a8e73a6d476a3be3dad64303","target":"record","created_at":"2026-05-18T02:04:27Z","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":"e661ba372f1a1762280496d8dfb7e587f976f2968d3f38052c6e301b05627248","cross_cats_sorted":["astro-ph.HE"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2010-12-13T13:51:52Z","title_canon_sha256":"d26c45ab7bd866ab6b85da54c7a6988c86903ebfd7b5f9658f1f4f6f285f277b"},"schema_version":"1.0","source":{"id":"1012.2728","kind":"arxiv","version":2}},"canonical_sha256":"5c7b8323fb891895720da66fac5fd39eee8fb8b525880cc61dcb77f380ab1e90","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"5c7b8323fb891895720da66fac5fd39eee8fb8b525880cc61dcb77f380ab1e90","first_computed_at":"2026-05-18T02:04:27.625145Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T02:04:27.625145Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"Zw7vczOe/fFo8+51UHEv5huHK1DVox6yP1mMvzNimoDn3OiViLMTG+OclyhOIhA3C7oG627lGXN1M296U+BcCQ==","signature_status":"signed_v1","signed_at":"2026-05-18T02:04:27.625871Z","signed_message":"canonical_sha256_bytes"},"source_id":"1012.2728","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:374fc4569cb1f0251ba82ca5444e1cfbf3b04d91a8e73a6d476a3be3dad64303","sha256:eca3f44fd3c5a5a490e46c2bf925c6944c808e6ebd549cf0879bb52d42e7a873"],"state_sha256":"7920e49d13d59accfda5fbdab91f4ad4b29b3f71c9813340eb46b018695fda96"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"R2xncRvyWt/Epq/PYhuakc3AxCBtjF1wCYd/2RSc6lullumLjhLJIANcyyKthVr2AgNwwbPi36IJYq/viIZ5Bw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-18T19:46:54.305752Z","bundle_sha256":"44cbb9ab643906c80410ed5ec42d480b0e3d7cc5acf9d48f2735d9f83dd56f57"}}