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- W2078558831 abstract "We provide an equation of state for hot nuclear matter in $ensuremath{beta}$ equilibrium by applying a momentum-dependent effective interaction. We focus on the study of the equation of state of high-density and high-temperature nuclear matter, containing leptons (electrons and muons) under the chemical equilibrium condition in which neutrinos have left the system. The conditions of charge neutrality and equilibrium under the $ensuremath{beta}$-decay process lead first to the evaluation of proton and lepton fractions and then to the evaluation of internal energy, free energy, and pressure, and in total to the equation of state of hot nuclear matter. Thermal effects on the properties and equation of state of nuclear matter are assessed and analyzed in the framework of the proposed effective interaction model. Special attention is given to the study of the contribution of the components of $ensuremath{beta}$-stable nuclear matter to the entropy per particle, a quantity of great interest in the study of structure and collapse of supernova." @default.
- W2078558831 created "2016-06-24" @default.
- W2078558831 creator A5044320792 @default.
- W2078558831 creator A5048838626 @default.
- W2078558831 date "2009-04-20" @default.
- W2078558831 modified "2023-10-17" @default.
- W2078558831 title "Equation of state for<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mrow><mml:mi>β</mml:mi></mml:mrow></mml:math>-stable hot nuclear matter" @default.
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- W2078558831 doi "https://doi.org/10.1103/physrevc.79.045806" @default.
- W2078558831 hasPublicationYear "2009" @default.
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