Publication Abstracts
Cohen et al. 1970
Cohen, J.M., W.D. Langer, L.C. Rosen, and A.G.W. Cameron, 1970: Neutron star models based on an improved equation of state. Astrophys. Space Sci., 6, 228-239, doi:10.1007/BF00651224.
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 0.065 M☉ 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 200m or more depending on the mass of the model.
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BibTeX Citation
@article{co01100t,
author={Cohen, J. M. and Langer, W. D. and Rosen, L. C. and Cameron, A. G. W.},
title={Neutron star models based on an improved equation of state},
year={1970},
journal={Astrophysics and Space Science},
volume={6},
pages={228--239},
doi={10.1007/BF00651224},
}
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RIS Citation
TY - JOUR ID - co01100t AU - Cohen, J. M. AU - Langer, W. D. AU - Rosen, L. C. AU - Cameron, A. G. W. PY - 1970 TI - Neutron star models based on an improved equation of state JA - Astrophys. Space Sci. JO - Astrophysics and Space Science VL - 6 SP - 228 EP - 239 DO - 10.1007/BF00651224 ER -
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