Neutron Star Models based on an Improved Equation of State

Details Neutron Star Models based on an Improved Equation of State Neutron Star Models based on an Improved Equation of State

Feb 1970

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1970ap%26ss...6..228c&link_type=abstract

Astrophysics and Space Science, Volume 6, Issue 2, pp.228-239

Astronomy and Astrophysics

Astrophysics

43

Scientific paper

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 &sun; 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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