Abstract
Two new equations of state obtained for matter constituting isothermal neutron star core by using isentropic nature of matter for the equalities Γ=Γ2 and Γ=Γ3 (where Γ's are usual adiabatic exponents) have been utilised to discuss the internal temperature of core. The temperature of matter has been obtained asT=Ta(P+E)/ϱ. Variation ofT/Ta(≡t) with energy density has been discussed for these new equations of state and some standard equations of state for nuclear matter.
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