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
Supernova and neutron stars with relativistic equations of state
โ Scribed by K. Sumiyoshi; H. Toki; R. Brockmann
- Book ID
- 113361197
- Publisher
- Elsevier Science
- Year
- 1992
- Tongue
- English
- Weight
- 389 KB
- Volume
- 276
- Category
- Article
- ISSN
- 0370-2693
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