{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:MP6DSVXQAHRBMRNJWC7GFQBHSE","short_pith_number":"pith:MP6DSVXQ","schema_version":"1.0","canonical_sha256":"63fc3956f001e21645a9b0be62c027910e2b5909d92e9f637057af1ea65d2126","source":{"kind":"arxiv","id":"astro-ph/0606592","version":1},"attestation_state":"computed","paper":{"title":"Non linear particle acceleration at non-relativistic shock waves in the presence of self-generated turbulence","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Elena Amato (1), Pasquale Blasi (1) ((1) INAF - Osservatorio Astrofisico di Arcetri)","submitted_at":"2006-06-23T16:08:55Z","abstract_excerpt":"Particle acceleration at astrophysical shocks may be very efficient if magnetic scattering is self-generated by the same particles. This nonlinear process adds to the nonlinear modification of the shock due to the dynamical reaction of the accelerated particles on the shock. Building on a previous general solution of the problem of particle acceleration with arbitrary diffusion coefficients (Amato & Blasi, 2005), we present here the first semi-analytical calculation of particle acceleration with both effects taken into account at the same time: charged particles are accelerated in the backgrou"},"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":"astro-ph/0606592","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-06-23T16:08:55Z","cross_cats_sorted":[],"title_canon_sha256":"31adc5322891ea08bf5b0f43a4f70796b6bbfb3a71487a1d1d2727c9f650a93f","abstract_canon_sha256":"21c15cf0314bedf4c12d42ed19053936f2256e1a3e6f2f2c0687942e5f6df006"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:58:56.132836Z","signature_b64":"7mMmbJaPGm/aJpNmGm9gWqokhQO3vFKOUhGRXhMWY5pSZSu6JPareIjFkhDgdpb4johkky3Dn/Bdll1xTjrfAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"63fc3956f001e21645a9b0be62c027910e2b5909d92e9f637057af1ea65d2126","last_reissued_at":"2026-07-04T16:58:56.132397Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:58:56.132397Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non linear particle acceleration at non-relativistic shock waves in the presence of self-generated turbulence","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"Elena Amato (1), Pasquale Blasi (1) ((1) INAF - Osservatorio Astrofisico di Arcetri)","submitted_at":"2006-06-23T16:08:55Z","abstract_excerpt":"Particle acceleration at astrophysical shocks may be very efficient if magnetic scattering is self-generated by the same particles. This nonlinear process adds to the nonlinear modification of the shock due to the dynamical reaction of the accelerated particles on the shock. Building on a previous general solution of the problem of particle acceleration with arbitrary diffusion coefficients (Amato & Blasi, 2005), we present here the first semi-analytical calculation of particle acceleration with both effects taken into account at the same time: charged particles are accelerated in the backgrou"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0606592","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/astro-ph/0606592/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":"astro-ph/0606592","created_at":"2026-07-04T16:58:56.132454+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0606592v1","created_at":"2026-07-04T16:58:56.132454+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0606592","created_at":"2026-07-04T16:58:56.132454+00:00"},{"alias_kind":"pith_short_12","alias_value":"MP6DSVXQAHRB","created_at":"2026-07-04T16:58:56.132454+00:00"},{"alias_kind":"pith_short_16","alias_value":"MP6DSVXQAHRBMRNJ","created_at":"2026-07-04T16:58:56.132454+00:00"},{"alias_kind":"pith_short_8","alias_value":"MP6DSVXQ","created_at":"2026-07-04T16:58:56.132454+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MP6DSVXQAHRBMRNJWC7GFQBHSE","json":"https://pith.science/pith/MP6DSVXQAHRBMRNJWC7GFQBHSE.json","graph_json":"https://pith.science/api/pith-number/MP6DSVXQAHRBMRNJWC7GFQBHSE/graph.json","events_json":"https://pith.science/api/pith-number/MP6DSVXQAHRBMRNJWC7GFQBHSE/events.json","paper":"https://pith.science/paper/MP6DSVXQ"},"agent_actions":{"view_html":"https://pith.science/pith/MP6DSVXQAHRBMRNJWC7GFQBHSE","download_json":"https://pith.science/pith/MP6DSVXQAHRBMRNJWC7GFQBHSE.json","view_paper":"https://pith.science/paper/MP6DSVXQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0606592&json=true","fetch_graph":"https://pith.science/api/pith-number/MP6DSVXQAHRBMRNJWC7GFQBHSE/graph.json","fetch_events":"https://pith.science/api/pith-number/MP6DSVXQAHRBMRNJWC7GFQBHSE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MP6DSVXQAHRBMRNJWC7GFQBHSE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MP6DSVXQAHRBMRNJWC7GFQBHSE/action/storage_attestation","attest_author":"https://pith.science/pith/MP6DSVXQAHRBMRNJWC7GFQBHSE/action/author_attestation","sign_citation":"https://pith.science/pith/MP6DSVXQAHRBMRNJWC7GFQBHSE/action/citation_signature","submit_replication":"https://pith.science/pith/MP6DSVXQAHRBMRNJWC7GFQBHSE/action/replication_record"}},"created_at":"2026-07-04T16:58:56.132454+00:00","updated_at":"2026-07-04T16:58:56.132454+00:00"}