Relativistic Mean Field calculations of nuclear properties in early stages of stellar collapse

Details Relativistic Mean Field calculations of nuclear properties in early stages of stellar collapse Relativistic Mean Field calculations of nuclear properties in early stages of stellar collapse

1996-12-15

arxiv.org/abs/astro-ph/9612147v1

Astronomy and Astrophysics

Astrophysics

4 pages , Latex, 4 figures, uses espcrc1.sty. To appear in Nucl. Phys. A, proceedings of "Nuclei in the Cosmos 1996" 4th Inter

Scientific paper

10.1016/S0375-9474(97)00274-1

We use the Relativistic Mean Field (RMF) method to calculate properties of neutron rich, usually deformed nuclei, important for equation of state calculations and which have significant abundance in the early stages of stellar collapse. We compare the results of our microscopic calculations with existing cold nuclear equations of state based on macroscopic liquid drop model and the FRLDM model.

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