{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:MHKB5MBRZZM5KP5HWCEZUKJV3C","short_pith_number":"pith:MHKB5MBR","schema_version":"1.0","canonical_sha256":"61d41eb031ce59d53fa7b0899a2935d88c00df0ff29b0beb1f059697c1dde432","source":{"kind":"arxiv","id":"2506.06593","version":2},"attestation_state":"computed","paper":{"title":"LHAASO protons versus LHAASO diffuse gamma-rays: a consistency check","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Carmelo Evoli, Francesco Lorenzo Villante, Giulia Pagliaroli, Luis Enrique Espinosa Castro, Vittoria Vecchiotti","submitted_at":"2025-06-06T23:59:53Z","abstract_excerpt":"We perform the first direct consistency check between the recently measured proton spectrum at the knee by Large High Altitude Air Shower Observatory (LHAASO) and the collaboration's own high-precision mapping of Galactic diffuse gamma-ray emission. By modeling the hadronic gamma-ray production using the updated cosmic-ray spectra, gas templates and cross-section models, we show that the predicted gamma-ray flux robustly overshoots the LHAASO data in both inner and lateral Galactic regions. This persistent mismatch in both normalization and spectral shape challenges conventional scenarios link"},"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":"2506.06593","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-06-06T23:59:53Z","cross_cats_sorted":[],"title_canon_sha256":"cb0b1b21e2b5a4153d8ec4a88b25d67f5dc919637a5693668ee9b98f7e2c3b6c","abstract_canon_sha256":"3381e3b5ecf64b970953734238cb582bea3cdc54ac0e9a39d56646306292eef2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T12:03:27.301007Z","signature_b64":"s6vYTlENoDT1HiD+6fHk/SX6ogmrrcs/obn7h24fGi7ph6lfIfrFCaLLbLjmPNu65Q5y64M9v31qbHn49O1NAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"61d41eb031ce59d53fa7b0899a2935d88c00df0ff29b0beb1f059697c1dde432","last_reissued_at":"2026-07-05T12:03:27.300435Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T12:03:27.300435Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"LHAASO protons versus LHAASO diffuse gamma-rays: a consistency check","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Carmelo Evoli, Francesco Lorenzo Villante, Giulia Pagliaroli, Luis Enrique Espinosa Castro, Vittoria Vecchiotti","submitted_at":"2025-06-06T23:59:53Z","abstract_excerpt":"We perform the first direct consistency check between the recently measured proton spectrum at the knee by Large High Altitude Air Shower Observatory (LHAASO) and the collaboration's own high-precision mapping of Galactic diffuse gamma-ray emission. By modeling the hadronic gamma-ray production using the updated cosmic-ray spectra, gas templates and cross-section models, we show that the predicted gamma-ray flux robustly overshoots the LHAASO data in both inner and lateral Galactic regions. This persistent mismatch in both normalization and spectral shape challenges conventional scenarios link"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.06593","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2506.06593/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":"2506.06593","created_at":"2026-07-05T12:03:27.300497+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.06593v2","created_at":"2026-07-05T12:03:27.300497+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.06593","created_at":"2026-07-05T12:03:27.300497+00:00"},{"alias_kind":"pith_short_12","alias_value":"MHKB5MBRZZM5","created_at":"2026-07-05T12:03:27.300497+00:00"},{"alias_kind":"pith_short_16","alias_value":"MHKB5MBRZZM5KP5H","created_at":"2026-07-05T12:03:27.300497+00:00"},{"alias_kind":"pith_short_8","alias_value":"MHKB5MBR","created_at":"2026-07-05T12:03:27.300497+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.09976","citing_title":"Too Heavy to Hide: Gamma-Ray Constraints on Annihilating Dark Matter beyond Unitarity","ref_index":131,"is_internal_anchor":false},{"citing_arxiv_id":"2604.08175","citing_title":"How many VHE gamma-ray binaries with young pulsars can be observed?","ref_index":91,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MHKB5MBRZZM5KP5HWCEZUKJV3C","json":"https://pith.science/pith/MHKB5MBRZZM5KP5HWCEZUKJV3C.json","graph_json":"https://pith.science/api/pith-number/MHKB5MBRZZM5KP5HWCEZUKJV3C/graph.json","events_json":"https://pith.science/api/pith-number/MHKB5MBRZZM5KP5HWCEZUKJV3C/events.json","paper":"https://pith.science/paper/MHKB5MBR"},"agent_actions":{"view_html":"https://pith.science/pith/MHKB5MBRZZM5KP5HWCEZUKJV3C","download_json":"https://pith.science/pith/MHKB5MBRZZM5KP5HWCEZUKJV3C.json","view_paper":"https://pith.science/paper/MHKB5MBR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.06593&json=true","fetch_graph":"https://pith.science/api/pith-number/MHKB5MBRZZM5KP5HWCEZUKJV3C/graph.json","fetch_events":"https://pith.science/api/pith-number/MHKB5MBRZZM5KP5HWCEZUKJV3C/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MHKB5MBRZZM5KP5HWCEZUKJV3C/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MHKB5MBRZZM5KP5HWCEZUKJV3C/action/storage_attestation","attest_author":"https://pith.science/pith/MHKB5MBRZZM5KP5HWCEZUKJV3C/action/author_attestation","sign_citation":"https://pith.science/pith/MHKB5MBRZZM5KP5HWCEZUKJV3C/action/citation_signature","submit_replication":"https://pith.science/pith/MHKB5MBRZZM5KP5HWCEZUKJV3C/action/replication_record"}},"created_at":"2026-07-05T12:03:27.300497+00:00","updated_at":"2026-07-05T12:03:27.300497+00:00"}