{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:CR54RGRT3O2L6BN6VVAE3UQQR6","short_pith_number":"pith:CR54RGRT","schema_version":"1.0","canonical_sha256":"147bc89a33dbb4bf05bead404dd2108f9cf7ce8038b202a31a6e67c606e1d433","source":{"kind":"arxiv","id":"1709.03897","version":2},"attestation_state":"computed","paper":{"title":"The Gluon condensation in high energy cosmic rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex"],"primary_cat":"hep-ph","authors_text":"Jiangshan Lan, Jianhong Ruan, Wei Zhu","submitted_at":"2017-09-12T15:00:35Z","abstract_excerpt":"The gluon condensation (GC)-effects in high energy cosmic rays are investigated. After a brief review of the GC, several examples including gamma-, electron-, and positron-spectra in a broad GeV$\\sim $TeV region can be explained by the GC-effects. We find that the GC may break the power-law of the cosmic ray spectra if the energy of accelerated protons exceeds the GC-threshold. The GC is a new phenomenon that is not yet known, it provides a new window to understand the high energy cosmic ray spectra."},"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":"1709.03897","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2017-09-12T15:00:35Z","cross_cats_sorted":["astro-ph.HE","hep-ex"],"title_canon_sha256":"02f543d8669cf880ea4bf03b280f23ab15d7d829715d0950945a3564f41c3a29","abstract_canon_sha256":"3417fa071f112cce90e680357d725e3bcb84993fcda3899ea2f4091c2dbc8134"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:06:06.046624Z","signature_b64":"Nd/o5VUVLmfd20BuM9i2E/2I2yMOre+AS5+ost+aCNV0ijnMSe50ESassL6Ra4OJHBigZALsY9GZXSGqujoMBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"147bc89a33dbb4bf05bead404dd2108f9cf7ce8038b202a31a6e67c606e1d433","last_reissued_at":"2026-05-18T00:06:06.046082Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:06:06.046082Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Gluon condensation in high energy cosmic rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex"],"primary_cat":"hep-ph","authors_text":"Jiangshan Lan, Jianhong Ruan, Wei Zhu","submitted_at":"2017-09-12T15:00:35Z","abstract_excerpt":"The gluon condensation (GC)-effects in high energy cosmic rays are investigated. After a brief review of the GC, several examples including gamma-, electron-, and positron-spectra in a broad GeV$\\sim $TeV region can be explained by the GC-effects. We find that the GC may break the power-law of the cosmic ray spectra if the energy of accelerated protons exceeds the GC-threshold. The GC is a new phenomenon that is not yet known, it provides a new window to understand the high energy cosmic ray spectra."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1709.03897","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1709.03897","created_at":"2026-05-18T00:06:06.046171+00:00"},{"alias_kind":"arxiv_version","alias_value":"1709.03897v2","created_at":"2026-05-18T00:06:06.046171+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1709.03897","created_at":"2026-05-18T00:06:06.046171+00:00"},{"alias_kind":"pith_short_12","alias_value":"CR54RGRT3O2L","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_16","alias_value":"CR54RGRT3O2L6BN6","created_at":"2026-05-18T12:31:10.602751+00:00"},{"alias_kind":"pith_short_8","alias_value":"CR54RGRT","created_at":"2026-05-18T12:31:10.602751+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.23726","citing_title":"A Unified Explanation of Gamma-Ray and Neutrino Spectra from Astrophysical Sources Based on the Gluon Condensation Model","ref_index":12,"is_internal_anchor":false},{"citing_arxiv_id":"2604.23726","citing_title":"A Unified Explanation of Gamma-Ray and Neutrino Spectra from Astrophysical Sources Based on the Gluon Condensation Model","ref_index":12,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CR54RGRT3O2L6BN6VVAE3UQQR6","json":"https://pith.science/pith/CR54RGRT3O2L6BN6VVAE3UQQR6.json","graph_json":"https://pith.science/api/pith-number/CR54RGRT3O2L6BN6VVAE3UQQR6/graph.json","events_json":"https://pith.science/api/pith-number/CR54RGRT3O2L6BN6VVAE3UQQR6/events.json","paper":"https://pith.science/paper/CR54RGRT"},"agent_actions":{"view_html":"https://pith.science/pith/CR54RGRT3O2L6BN6VVAE3UQQR6","download_json":"https://pith.science/pith/CR54RGRT3O2L6BN6VVAE3UQQR6.json","view_paper":"https://pith.science/paper/CR54RGRT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1709.03897&json=true","fetch_graph":"https://pith.science/api/pith-number/CR54RGRT3O2L6BN6VVAE3UQQR6/graph.json","fetch_events":"https://pith.science/api/pith-number/CR54RGRT3O2L6BN6VVAE3UQQR6/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CR54RGRT3O2L6BN6VVAE3UQQR6/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CR54RGRT3O2L6BN6VVAE3UQQR6/action/storage_attestation","attest_author":"https://pith.science/pith/CR54RGRT3O2L6BN6VVAE3UQQR6/action/author_attestation","sign_citation":"https://pith.science/pith/CR54RGRT3O2L6BN6VVAE3UQQR6/action/citation_signature","submit_replication":"https://pith.science/pith/CR54RGRT3O2L6BN6VVAE3UQQR6/action/replication_record"}},"created_at":"2026-05-18T00:06:06.046171+00:00","updated_at":"2026-05-18T00:06:06.046171+00:00"}