We c~nstruct the equation of state (EOS) of nuclear matter using the relativistic mean field (RMF) theory in the wide density, temperature range with various proton fractions for the use of supernova simulation and the neutron star calculations. We first construct the EOS of homogeneous nuclear matt
β¦ LIBER β¦
Properties of a relativistic equation of state for collapse-driven supernovae
β Scribed by K. Sumiyoshi; H. Suzuki; S. Yamada; H. Toki
- Publisher
- Elsevier Science
- Year
- 2004
- Tongue
- English
- Weight
- 493 KB
- Volume
- 730
- Category
- Article
- ISSN
- 0375-9474
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