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Equation of State for hot dense matter
Nuclear equation of state for hot dense matter is an essential part of the core-collapsing supernva simualtion.
Liquid drop model is the most accurate and fastest method to construct the hot dense matter EOS table.
Nuclei in dense nuclear matter
Nuclear density in the crust of neutron stars.
In this simulation, 1450 neutrons and 50 protons exist in the box of 32fm x 32 fm x 32fm.
Note that most of neutrons are unbound and protons are clustered to make bound states
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