Barranco Gómez, ManuelBuchler, Jean-Robert2010-04-222010-04-2219810556-2813https://hdl.handle.net/2445/12235The properties of hot, dense stellar matter are investigated with a finite temperature nuclear Thomas-Fermi model.12 p.application/pdfeng(c) The American Physical Society, 1981Estructura nuclearAstrofísica nuclearEcuacions d'estatNuclear structureNuclear astrophysicsEquations of stateEquation of state of hot, dense stellar matter. Finite temperature nuclear Thomas-Fermi approachinfo:eu-repo/semantics/article75989info:eu-repo/semantics/openAccess