{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:DJL4HW2L2GWXARFF2STDAJVSEQ","short_pith_number":"pith:DJL4HW2L","schema_version":"1.0","canonical_sha256":"1a57c3db4bd1ad7044a5d4a63026b2241555b6a0eeea21202451368ef91c9d12","source":{"kind":"arxiv","id":"2208.12823","version":1},"attestation_state":"computed","paper":{"title":"A numerical study of the interplay between Fermi acceleration mechanisms in radio lobes of FR-II radio galaxies","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrea Mignone, Bhargav Vaidya, Martin J. Hardcastle, Sayan Kundu","submitted_at":"2022-08-26T18:00:02Z","abstract_excerpt":"Context: Radio-loud AGNs are thought to possess various sites of particle acceleration, which gives rise to the observed non-thermal spectra. Stochastic turbulent acceleration (STA) and diffusive shock acceleration (DSA) are commonly cited as potential sources of high-energy particles in weakly magnetized environments. Together, these acceleration processes and various radiative losses determine the emission characteristics of these extra-galactic radio sources.\n  Aims: The purpose of this research is to investigate the dynamical interplay between the STA and DSA in the radio lobes of FR-II ra"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2208.12823","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-08-26T18:00:02Z","cross_cats_sorted":[],"title_canon_sha256":"d88e17a354a3bcd27d3ed35a9fbc0245a0e7133630412db4c4efde904ba198b1","abstract_canon_sha256":"d107a03d588c2db00e659b8e1b2af5413c05929a9bd5b863c747aa0856dd8162"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:18:37.502696Z","signature_b64":"kiarPWE0H6ZBzQuNmNUFvoaZSbBSWHI6T1bu2aZW7mAhqolayhtEEfrPWkbjHX9dh+Cw7LSIUD6wIlM6x8h+DQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1a57c3db4bd1ad7044a5d4a63026b2241555b6a0eeea21202451368ef91c9d12","last_reissued_at":"2026-07-05T05:18:37.502163Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:18:37.502163Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A numerical study of the interplay between Fermi acceleration mechanisms in radio lobes of FR-II radio galaxies","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Andrea Mignone, Bhargav Vaidya, Martin J. Hardcastle, Sayan Kundu","submitted_at":"2022-08-26T18:00:02Z","abstract_excerpt":"Context: Radio-loud AGNs are thought to possess various sites of particle acceleration, which gives rise to the observed non-thermal spectra. Stochastic turbulent acceleration (STA) and diffusive shock acceleration (DSA) are commonly cited as potential sources of high-energy particles in weakly magnetized environments. Together, these acceleration processes and various radiative losses determine the emission characteristics of these extra-galactic radio sources.\n  Aims: The purpose of this research is to investigate the dynamical interplay between the STA and DSA in the radio lobes of FR-II ra"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2208.12823","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/2208.12823/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"},"aliases":[{"alias_kind":"arxiv","alias_value":"2208.12823","created_at":"2026-07-05T05:18:37.502222+00:00"},{"alias_kind":"arxiv_version","alias_value":"2208.12823v1","created_at":"2026-07-05T05:18:37.502222+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2208.12823","created_at":"2026-07-05T05:18:37.502222+00:00"},{"alias_kind":"pith_short_12","alias_value":"DJL4HW2L2GWX","created_at":"2026-07-05T05:18:37.502222+00:00"},{"alias_kind":"pith_short_16","alias_value":"DJL4HW2L2GWXARFF","created_at":"2026-07-05T05:18:37.502222+00:00"},{"alias_kind":"pith_short_8","alias_value":"DJL4HW2L","created_at":"2026-07-05T05:18:37.502222+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.02656","citing_title":"Non-thermal emission in jets and winds: Expected emission and spectral index distributions","ref_index":51,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DJL4HW2L2GWXARFF2STDAJVSEQ","json":"https://pith.science/pith/DJL4HW2L2GWXARFF2STDAJVSEQ.json","graph_json":"https://pith.science/api/pith-number/DJL4HW2L2GWXARFF2STDAJVSEQ/graph.json","events_json":"https://pith.science/api/pith-number/DJL4HW2L2GWXARFF2STDAJVSEQ/events.json","paper":"https://pith.science/paper/DJL4HW2L"},"agent_actions":{"view_html":"https://pith.science/pith/DJL4HW2L2GWXARFF2STDAJVSEQ","download_json":"https://pith.science/pith/DJL4HW2L2GWXARFF2STDAJVSEQ.json","view_paper":"https://pith.science/paper/DJL4HW2L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2208.12823&json=true","fetch_graph":"https://pith.science/api/pith-number/DJL4HW2L2GWXARFF2STDAJVSEQ/graph.json","fetch_events":"https://pith.science/api/pith-number/DJL4HW2L2GWXARFF2STDAJVSEQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DJL4HW2L2GWXARFF2STDAJVSEQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DJL4HW2L2GWXARFF2STDAJVSEQ/action/storage_attestation","attest_author":"https://pith.science/pith/DJL4HW2L2GWXARFF2STDAJVSEQ/action/author_attestation","sign_citation":"https://pith.science/pith/DJL4HW2L2GWXARFF2STDAJVSEQ/action/citation_signature","submit_replication":"https://pith.science/pith/DJL4HW2L2GWXARFF2STDAJVSEQ/action/replication_record"}},"created_at":"2026-07-05T05:18:37.502222+00:00","updated_at":"2026-07-05T05:18:37.502222+00:00"}