Neutron star models based on an improved equation of state |
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| Authors: | Jeffrey M. Cohen William D. Langer Leonard C. Rosen A. G. W. Cameron |
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| Affiliation: | (1) Goddard Institute for Space Studies, NASA, New York, N.Y., USA;(2) Belfer Graduate School of Science, Yeshiva University, New York, N.Y., USA |
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| Abstract: | Using an equation of state for cold degenerate matter which takes nuclear forces and nuclear clustering into account, neutron star models are constructed. Stable models were obtained in the mass range above 0.065M and density range 1014.08 to 1015.4 gm/cm3. All of these models were found to be bound. The outer crystalline layer of the star was found to have a thickness of 200 m or more depending on the mass of the model. |
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