{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2002:LRWQCCFGVFPHZ4KXS2UKXQLEAG","short_pith_number":"pith:LRWQCCFG","schema_version":"1.0","canonical_sha256":"5c6d0108a6a95e7cf15796a8abc16401bd7ce19b306b88e3e1ad2f86f5bd6398","source":{"kind":"arxiv","id":"hep-ph/0204343","version":2},"attestation_state":"computed","paper":{"title":"Photon and Gluon Emission in Relativistic Plasmas","license":"","headline":"","cross_cats":["nucl-th"],"primary_cat":"hep-ph","authors_text":"Guy D. Moore, Laurence G. Yaffe, Peter Arnold","submitted_at":"2002-04-29T19:34:39Z","abstract_excerpt":"We recently derived, using diagrammatic methods, the leading-order hard photon emission rate in ultra-relativistic plasmas. This requires a correct treatment of multiple scattering effects which limit the coherence length of emitted radiation (the Landau-Pomeranchuk-Migdal effect). In this paper, we provide a more physical derivation of this result, and extend the treatment to the case of gluon radiation."},"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":"hep-ph/0204343","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"2002-04-29T19:34:39Z","cross_cats_sorted":["nucl-th"],"title_canon_sha256":"3ca3575bdfb9a7e1554ccf4694548d13fc3d46f4de3b50ed9827f6beb0257d96","abstract_canon_sha256":"a9a1b3f3f85cc8296aed00fd0ba8e0889d204cf6e519ebcf5a1df304c379a62d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T17:21:48.075648Z","signature_b64":"6Zk4Yrq89YHQ1G09rKWRjeCZ1kqmBnO7dTiu+ST+tUG23rYiS0Rae0P9lCmd4TLxFGkACIC3CaG26pCRp6WuDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5c6d0108a6a95e7cf15796a8abc16401bd7ce19b306b88e3e1ad2f86f5bd6398","last_reissued_at":"2026-07-04T17:21:48.075204Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T17:21:48.075204Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Photon and Gluon Emission in Relativistic Plasmas","license":"","headline":"","cross_cats":["nucl-th"],"primary_cat":"hep-ph","authors_text":"Guy D. Moore, Laurence G. Yaffe, Peter Arnold","submitted_at":"2002-04-29T19:34:39Z","abstract_excerpt":"We recently derived, using diagrammatic methods, the leading-order hard photon emission rate in ultra-relativistic plasmas. This requires a correct treatment of multiple scattering effects which limit the coherence length of emitted radiation (the Landau-Pomeranchuk-Migdal effect). In this paper, we provide a more physical derivation of this result, and extend the treatment to the case of gluon radiation."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0204343","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/hep-ph/0204343/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":"hep-ph/0204343","created_at":"2026-07-04T17:21:48.075258+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/0204343v2","created_at":"2026-07-04T17:21:48.075258+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/0204343","created_at":"2026-07-04T17:21:48.075258+00:00"},{"alias_kind":"pith_short_12","alias_value":"LRWQCCFGVFPH","created_at":"2026-07-04T17:21:48.075258+00:00"},{"alias_kind":"pith_short_16","alias_value":"LRWQCCFGVFPHZ4KX","created_at":"2026-07-04T17:21:48.075258+00:00"},{"alias_kind":"pith_short_8","alias_value":"LRWQCCFG","created_at":"2026-07-04T17:21:48.075258+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":8,"internal_anchor_count":7,"sample":[{"citing_arxiv_id":"2606.26039","citing_title":"In-medium QCD splittings beyond the soft, large-$N_c$ and harmonic-oscillator approximations all at once","ref_index":24,"is_internal_anchor":true},{"citing_arxiv_id":"2606.02414","citing_title":"Probing Pair Correlations in QCD Matter with Photon Spectra","ref_index":49,"is_internal_anchor":true},{"citing_arxiv_id":"2605.28788","citing_title":"Energy-energy correlators inside single inclusive jets in heavy-ion collisions with CoLBT-hydro model","ref_index":10,"is_internal_anchor":true},{"citing_arxiv_id":"2509.10743","citing_title":"Glauber quark and gluon contributions to quark energy loss at next-to-leading order and next-to-leading twist","ref_index":51,"is_internal_anchor":true},{"citing_arxiv_id":"2510.25669","citing_title":"Minijet thermalization and jet transport coefficients in QCD kinetic theory","ref_index":93,"is_internal_anchor":true},{"citing_arxiv_id":"2512.12959","citing_title":"Energy Loss of a Heavy Quark in a Collisional Quark-Gluon Plasma","ref_index":24,"is_internal_anchor":true},{"citing_arxiv_id":"2603.27846","citing_title":"Full energy fraction and angular dependence of medium-induced splittings in the large-$N_c$ limit","ref_index":24,"is_internal_anchor":true},{"citing_arxiv_id":"2605.08336","citing_title":"Primordial Black Hole Hotspots Beyond Flat Spacetime","ref_index":65,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LRWQCCFGVFPHZ4KXS2UKXQLEAG","json":"https://pith.science/pith/LRWQCCFGVFPHZ4KXS2UKXQLEAG.json","graph_json":"https://pith.science/api/pith-number/LRWQCCFGVFPHZ4KXS2UKXQLEAG/graph.json","events_json":"https://pith.science/api/pith-number/LRWQCCFGVFPHZ4KXS2UKXQLEAG/events.json","paper":"https://pith.science/paper/LRWQCCFG"},"agent_actions":{"view_html":"https://pith.science/pith/LRWQCCFGVFPHZ4KXS2UKXQLEAG","download_json":"https://pith.science/pith/LRWQCCFGVFPHZ4KXS2UKXQLEAG.json","view_paper":"https://pith.science/paper/LRWQCCFG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/0204343&json=true","fetch_graph":"https://pith.science/api/pith-number/LRWQCCFGVFPHZ4KXS2UKXQLEAG/graph.json","fetch_events":"https://pith.science/api/pith-number/LRWQCCFGVFPHZ4KXS2UKXQLEAG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LRWQCCFGVFPHZ4KXS2UKXQLEAG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LRWQCCFGVFPHZ4KXS2UKXQLEAG/action/storage_attestation","attest_author":"https://pith.science/pith/LRWQCCFGVFPHZ4KXS2UKXQLEAG/action/author_attestation","sign_citation":"https://pith.science/pith/LRWQCCFGVFPHZ4KXS2UKXQLEAG/action/citation_signature","submit_replication":"https://pith.science/pith/LRWQCCFGVFPHZ4KXS2UKXQLEAG/action/replication_record"}},"created_at":"2026-07-04T17:21:48.075258+00:00","updated_at":"2026-07-04T17:21:48.075258+00:00"}