{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2011:7O27I4FT7ENAAMXEOIXTQLNW5O","short_pith_number":"pith:7O27I4FT","schema_version":"1.0","canonical_sha256":"fbb5f470b3f91a0032e4722f382db6eb9d6ac46951b57a73cafdc6b1f88c68bf","source":{"kind":"arxiv","id":"1101.2689","version":1},"attestation_state":"computed","paper":{"title":"Jet quenching in hot strongly coupled gauge theories simplified","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","nucl-th"],"primary_cat":"hep-th","authors_text":"Diana Vaman, Peter Arnold","submitted_at":"2011-01-13T23:07:35Z","abstract_excerpt":"Theoretical studies of jet stopping in strongly-coupled QCD-like plasmas have used gauge-gravity duality to find that the maximum stopping distance scales like E^{1/3} for large jet energies E. In recent work studying jets that are created by finite-size sources in the gauge theory, we found an additional scale: the typical (as opposed to maximum) jet stopping distance scales like (EL)^{1/4}, where L is the size of the space-time region where the jet is created. In this paper, we show that the results of our previous, somewhat involved computation in the gravity dual, and the (EL)^{1/4} scale "},"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":"1101.2689","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2011-01-13T23:07:35Z","cross_cats_sorted":["hep-ph","nucl-th"],"title_canon_sha256":"1db422d17237d67425e4bdd3520144d524e1f0cd2236035a38234b9db050826f","abstract_canon_sha256":"5a796089f1025e572bd4ce47b52e212f2363e8d42647d1bf7f214ba1830038f0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:22:57.697132Z","signature_b64":"yzxot98rWP1vwQjFa5OtOtklR47iUpQJmxmudEeR8gbRqhDq2og+TUBGjXxIYtpCevvIW3Y2uX51Bxv0I70RAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"fbb5f470b3f91a0032e4722f382db6eb9d6ac46951b57a73cafdc6b1f88c68bf","last_reissued_at":"2026-05-18T02:22:57.696658Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:22:57.696658Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Jet quenching in hot strongly coupled gauge theories simplified","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","nucl-th"],"primary_cat":"hep-th","authors_text":"Diana Vaman, Peter Arnold","submitted_at":"2011-01-13T23:07:35Z","abstract_excerpt":"Theoretical studies of jet stopping in strongly-coupled QCD-like plasmas have used gauge-gravity duality to find that the maximum stopping distance scales like E^{1/3} for large jet energies E. In recent work studying jets that are created by finite-size sources in the gauge theory, we found an additional scale: the typical (as opposed to maximum) jet stopping distance scales like (EL)^{1/4}, where L is the size of the space-time region where the jet is created. In this paper, we show that the results of our previous, somewhat involved computation in the gravity dual, and the (EL)^{1/4} scale "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1101.2689","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":""},"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":"1101.2689","created_at":"2026-05-18T02:22:57.696733+00:00"},{"alias_kind":"arxiv_version","alias_value":"1101.2689v1","created_at":"2026-05-18T02:22:57.696733+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1101.2689","created_at":"2026-05-18T02:22:57.696733+00:00"},{"alias_kind":"pith_short_12","alias_value":"7O27I4FT7ENA","created_at":"2026-05-18T12:26:22.705136+00:00"},{"alias_kind":"pith_short_16","alias_value":"7O27I4FT7ENAAMXE","created_at":"2026-05-18T12:26:22.705136+00:00"},{"alias_kind":"pith_short_8","alias_value":"7O27I4FT","created_at":"2026-05-18T12:26:22.705136+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2606.26598","citing_title":"Holographic light-quark energy loss in a spinning plasma","ref_index":20,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/7O27I4FT7ENAAMXEOIXTQLNW5O","json":"https://pith.science/pith/7O27I4FT7ENAAMXEOIXTQLNW5O.json","graph_json":"https://pith.science/api/pith-number/7O27I4FT7ENAAMXEOIXTQLNW5O/graph.json","events_json":"https://pith.science/api/pith-number/7O27I4FT7ENAAMXEOIXTQLNW5O/events.json","paper":"https://pith.science/paper/7O27I4FT"},"agent_actions":{"view_html":"https://pith.science/pith/7O27I4FT7ENAAMXEOIXTQLNW5O","download_json":"https://pith.science/pith/7O27I4FT7ENAAMXEOIXTQLNW5O.json","view_paper":"https://pith.science/paper/7O27I4FT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1101.2689&json=true","fetch_graph":"https://pith.science/api/pith-number/7O27I4FT7ENAAMXEOIXTQLNW5O/graph.json","fetch_events":"https://pith.science/api/pith-number/7O27I4FT7ENAAMXEOIXTQLNW5O/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/7O27I4FT7ENAAMXEOIXTQLNW5O/action/timestamp_anchor","attest_storage":"https://pith.science/pith/7O27I4FT7ENAAMXEOIXTQLNW5O/action/storage_attestation","attest_author":"https://pith.science/pith/7O27I4FT7ENAAMXEOIXTQLNW5O/action/author_attestation","sign_citation":"https://pith.science/pith/7O27I4FT7ENAAMXEOIXTQLNW5O/action/citation_signature","submit_replication":"https://pith.science/pith/7O27I4FT7ENAAMXEOIXTQLNW5O/action/replication_record"}},"created_at":"2026-05-18T02:22:57.696733+00:00","updated_at":"2026-05-18T02:22:57.696733+00:00"}