CHINESE JOURNAL OF COMPUTATIONAL PHYSICS ›› 1987, Vol. 4 ›› Issue (3): 317-328.
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Wang Yi-ren1, Huang Wei-zhang1, Zhang Suo-chun1, Zhang Tian-shu2
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Abstract: In this paper, the properties of system consisting of various nuclear species and free nucleons are described by a nuclear statistical equilibrium system consisting of a typical heavy nucleus, a particles, free neutrons and protons.starting from a semiempirical expression for the mass of the heavy nucleus and the entropy (energy) of their excited states, an equation of state is developed by a restricted minimization of the total free energy of a fixed volume of matter at given temperature and electron fraction.his scheme gave good agreement with the equation of El Eid & Hillebrandt at density 109-1012g cm-3 and with lamb et al (ILPR's equation of state at density 1012-1014g cm-3,ye=3,σ/k=1.5k.The imput physics such as the rate of electron capture on matter has been treated also more carefully.
Wang Yi-ren, Huang Wei-zhang, Zhang Suo-chun, Zhang Tian-shu. STELLAR CORE COLLAPSE AND EQUATION OF STATE (Ⅰ)——IMPUTTING PHYSICS FACTOR OF COLLAPSE CALCULATION[J]. CHINESE JOURNAL OF COMPUTATIONAL PHYSICS, 1987, 4(3): 317-328.
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http://www.cjcp.org.cn/EN/Y1987/V4/I3/317