VARIATIONAL CALCULATION FOR THE NUCLEAR EQUATION OF STATE TOWARD SUPERNOVA EXPLOSIONS
Keyword(s):
The equation of state (EOS) is calculated for uniform nuclear matter at zero and finite temperatures with the variational method. Making use of uncertainty of the three-body nuclear force, adjustable parameters in the nuclear EOS are tuned so that the Thomas-Fermi calculations for β-stable nuclei with the EOS reproduce the empirical data. The calculated nuclear properties imply that larger symmetry energy of the EOS is preferable to reproduce the empirical β-stability line. The expectation value of the nuclear Hamiltonian caused by the 2π-exchange three-body nuclear force is uncertain and related to the symmetry energy.
2010 ◽
Vol 19
(08n09)
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pp. 1727-1733
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2014 ◽
Vol 29
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pp. 1460221
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2003 ◽
Vol 17
(28)
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pp. 5127-5137
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2010 ◽
Vol 19
(08n09)
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pp. 1712-1719
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2011 ◽
Vol 312
(8)
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pp. 082005