{"record":{"author":{"account_ref":null,"orcid":null},"builds_on":[],"content_schema":"pubphys.content.topic/1","content_sha256":"51e6970c48311a6b78bd083fb8aa2ecd32a44dea76ca223501ab07dfbc696df6","created":"2026-10-03T07:17:52Z","files":[],"origin":{"assisted_by":[],"kind":"seed"},"parents":[],"salt":"01b1683832008ed2e8512f539d6946c1207f0665a2a142522da2d0fb6bb3308e","schema":"pubphys.record/2","site":"pubphys.com","target":null,"type":"topic"},"content":{"external_id":"plasma.warm-dense-matter","field":"plasma","n":"1","review_cite":"M. Bonitz, T. Dornheim, Zh. A. Moldabekov, S. Zhang et al., Ab initio simulation of warm dense matter, Physics of Plasmas, 2020","review_link":"https://doi.org/10.1063/1.5143225","review_verified":"true","summary":"Warm dense matter is material compressed to solid density or beyond and heated to tens of thousands of degrees, so it is neither an ordinary solid nor a thin plasma. It fills giant-planet interiors and every fusion capsule during implosion, yet its pressure, heat conduction and ability to slow fast particles are poorly known.","title":"Warm dense matter: equation of state and transport","topic_ref":null,"why":"Inertial-fusion design codes and models of planetary and white-dwarf interiors depend on equation-of-state and transport data in a regime where standard approximations fail."},"attested":{"attestation":{"batch":null,"client_id":null,"id_token_sha256":null,"kind":"platform"},"record_hash":"7b89d006c6b826eefaa6dd12fe5a55f76897cd2410bf60673fc30e5084ab9054","schema":"pubphys.attested/1"},"envelope":{"attested_hash":"54e2014c2491b08f4888fe4d84c2f101961179b5b97240f73028d91b35c542f6","platform_signature":{"key_id":"c6afc19b31429869751f06879c75cd64ea92654423d15b44be775bf1310a60da","sig":"PJPd6D_olV3mFxQsFdXcCxyTM4j68qJy1b4yMOuUXPZ-guGDcKxdNo5vSyabURxA8O-HnDnhEJyaQAg-tt_qCw"},"schema":"pubphys.envelope/1"},"record_hash":"7b89d006c6b826eefaa6dd12fe5a55f76897cd2410bf60673fc30e5084ab9054","leaf_index":311}