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Core-envelope models for massive fluid spheres
Authors:R S Fuloria  S C Pandey  M C Durgapal
Institution:(1) Department of Physics, Kumaon University, Nainital, India
Abstract:The solution of equation of state corresponding to equality Gamma=Gamma3 gives non-terminating solutions for isothermal neutron star cores. Hence, for this equality, core-envelope models have been developed by taking another equation of state, corresponding to the condition Gamma3, in the envelope. Various static, pulsational, and rotational parameters pertaining to neutron star models are calculated. These models are gravitationally bound and stable for radial perturbations and slow rotations.
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