{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:LNPPXKCGXWPOUZQMZONXAKCYHW","short_pith_number":"pith:LNPPXKCG","schema_version":"1.0","canonical_sha256":"5b5efba846bd9eea660ccb9b7028583d808a49e782895e8b285013da2dbb7417","source":{"kind":"arxiv","id":"2108.08479","version":3},"attestation_state":"computed","paper":{"title":"Vector meson spectral function in a dynamical AdS/QCD model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Defu Hou, Yan-qing Zhao","submitted_at":"2021-08-19T03:49:00Z","abstract_excerpt":"By using gauge/gravity duality, we calculate the spectral function of the heavy vector mesons with the presence of an intense magnetic field in a hot and dense medium. The results show that, a general conclusion, as the increases of magnetic field, chemical potential and temperature, the height of the peak of the spectral function decreases and the width increases. A nontrivial result is the change from the peak position of spectral function. We explain this non-trivial behavior by the interplay of the interaction between the two heavy quarks and the interaction between the medium with each of"},"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":"2108.08479","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2021-08-19T03:49:00Z","cross_cats_sorted":[],"title_canon_sha256":"b13116f0e765b8663c700f3c77404799b6424b36d46042a29ec50326ea0940f7","abstract_canon_sha256":"323e5ec261c66f124378ac482f1aae377785c88f67e8881f11a2172cffe66537"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:38:40.048593Z","signature_b64":"5ypOrXp6WfwXeN65uf7LoYaEPbfkVPQXCr++Sv0DtavSMLIRpAhO5/6WDiEIp9TFURfYCrfDrZ2zTMlz/70AAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5b5efba846bd9eea660ccb9b7028583d808a49e782895e8b285013da2dbb7417","last_reissued_at":"2026-07-05T05:38:40.048093Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:38:40.048093Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Vector meson spectral function in a dynamical AdS/QCD model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Defu Hou, Yan-qing Zhao","submitted_at":"2021-08-19T03:49:00Z","abstract_excerpt":"By using gauge/gravity duality, we calculate the spectral function of the heavy vector mesons with the presence of an intense magnetic field in a hot and dense medium. The results show that, a general conclusion, as the increases of magnetic field, chemical potential and temperature, the height of the peak of the spectral function decreases and the width increases. A nontrivial result is the change from the peak position of spectral function. We explain this non-trivial behavior by the interplay of the interaction between the two heavy quarks and the interaction between the medium with each of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2108.08479","kind":"arxiv","version":3},"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/2108.08479/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":"2108.08479","created_at":"2026-07-05T05:38:40.048143+00:00"},{"alias_kind":"arxiv_version","alias_value":"2108.08479v3","created_at":"2026-07-05T05:38:40.048143+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2108.08479","created_at":"2026-07-05T05:38:40.048143+00:00"},{"alias_kind":"pith_short_12","alias_value":"LNPPXKCGXWPO","created_at":"2026-07-05T05:38:40.048143+00:00"},{"alias_kind":"pith_short_16","alias_value":"LNPPXKCGXWPOUZQM","created_at":"2026-07-05T05:38:40.048143+00:00"},{"alias_kind":"pith_short_8","alias_value":"LNPPXKCG","created_at":"2026-07-05T05:38:40.048143+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.17279","citing_title":"Interplay of magnetic field and chemical potential induced anisotropy and frame dependent chaos of a $Q\\bar{Q}$ pair in holographic QCD","ref_index":95,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LNPPXKCGXWPOUZQMZONXAKCYHW","json":"https://pith.science/pith/LNPPXKCGXWPOUZQMZONXAKCYHW.json","graph_json":"https://pith.science/api/pith-number/LNPPXKCGXWPOUZQMZONXAKCYHW/graph.json","events_json":"https://pith.science/api/pith-number/LNPPXKCGXWPOUZQMZONXAKCYHW/events.json","paper":"https://pith.science/paper/LNPPXKCG"},"agent_actions":{"view_html":"https://pith.science/pith/LNPPXKCGXWPOUZQMZONXAKCYHW","download_json":"https://pith.science/pith/LNPPXKCGXWPOUZQMZONXAKCYHW.json","view_paper":"https://pith.science/paper/LNPPXKCG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2108.08479&json=true","fetch_graph":"https://pith.science/api/pith-number/LNPPXKCGXWPOUZQMZONXAKCYHW/graph.json","fetch_events":"https://pith.science/api/pith-number/LNPPXKCGXWPOUZQMZONXAKCYHW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LNPPXKCGXWPOUZQMZONXAKCYHW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LNPPXKCGXWPOUZQMZONXAKCYHW/action/storage_attestation","attest_author":"https://pith.science/pith/LNPPXKCGXWPOUZQMZONXAKCYHW/action/author_attestation","sign_citation":"https://pith.science/pith/LNPPXKCGXWPOUZQMZONXAKCYHW/action/citation_signature","submit_replication":"https://pith.science/pith/LNPPXKCGXWPOUZQMZONXAKCYHW/action/replication_record"}},"created_at":"2026-07-05T05:38:40.048143+00:00","updated_at":"2026-07-05T05:38:40.048143+00:00"}