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Equation of state of hot, dense stellar matter. Finite temperature nuclear Thomas-Fermi approach

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The properties of hot, dense stellar matter are investigated with a finite temperature nuclear Thomas-Fermi model.

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Reproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevC.24.1191

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Articles publicats en revistes (Física Quàntica i Astrofísica)

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Equation of state of hot, dense stellar matter. Finite temperature nuclear Thomas-Fermi approach